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1011.2096 | i | active galactic nuclei ( agn ) are increasingly recognised as a key element in the overall galaxy evolution process ( e.g. * ? ? ? * ) , yet the nature of the link between agn and galaxy evolution is not understood in depth . the link can take two main forms : the triggering of agn as gas is driven into the nuclear reg... | in this paper we discuss the results of a programme of spectral synthesis modelling of a sample of starburst radio galaxies in the context of scenarios for the triggering of the activity and the evolution of the host galaxies . new optical spectra are also presented for a subset of the objects discussed . [ firstpage ]... | in this paper we discuss the results of a programme of spectral synthesis modelling of a sample of starburst radio galaxies in the context of scenarios for the triggering of the activity and the evolution of the host galaxies . new optical spectra are also presented for a subset of the objects discussed . the starburst... |
1011.2096 | r | detailed discussions of the individual starburst radio galaxies , including the new spectroscopic results , are presented in the appendix . in this section we consider the general results and patterns obtained for the population of starburst radio galaxies as a whole . it is striking that a large proportion of starburs... | 25% of all powerful extragalactic radio sources frequently show disturbed morphologies at optical wavelengths , and unusual radio structures , although their stellar masses are typical of radio galaxies as a class . in terms of the characteristic ages of their young stellar populations ( ysp ) , the objects can be div... | in this paper we discuss the results of a programme of spectral synthesis modelling of a sample of starburst radio galaxies in the context of scenarios for the triggering of the activity and the evolution of the host galaxies . new optical spectra are also presented for a subset of the objects discussed . the starburst... |
1011.2096 | c | it is clear that many of the optical morphological features of starburst radio galaxies are consistent with the idea that both the agn / jet and starburst activity have been triggered as the result of the gas infall associated with galaxy mergers . hydrodynamical simulations of mergers reveal that they are complex even... | although% of starburst radio galaxies are sufficiently bright at mfir wavelengths to be classified as ultra - luminous infrared galaxies ( ulirgs ) , we show that only the most massive ulirgs are capable of evolving into radio galaxies . finally , for a small subset of starburst radio galaxies in rich clusters of galax... | in this paper we discuss the results of a programme of spectral synthesis modelling of a sample of starburst radio galaxies in the context of scenarios for the triggering of the activity and the evolution of the host galaxies . new optical spectra are also presented for a subset of the objects discussed . the starburst... |
1011.2096 | c | in this paper we have discussed the properties of the young stellar populations ( ysp ) in the @xmath015 25% of powerful radio galaxies that show strong evidence for recent star formation activity at optical wavelengths . combined with information about the morphologies of the host galaxies , the ysp properties of mos... | most of former group are associated with large mid- to far - ir ( mfir ) continuum and [ oiii ] emission line luminosities ( l , w ) , while most of the latter have lower luminosities . combining the information on the ysp with that on the optical morphologies of the host galaxies , we deduce that the majority of the... | in this paper we discuss the results of a programme of spectral synthesis modelling of a sample of starburst radio galaxies in the context of scenarios for the triggering of the activity and the evolution of the host galaxies . new optical spectra are also presented for a subset of the objects discussed . the starburst... |
0901.0574 | i | it is well known that in a chaotic dynamics the pointwise , future behavior of an initial condition is unpredictable and even impossible to be described by using a finite quantity of information . on the other hand many of its statistical properties are rather regular and often described by suitable versions of classic... | in this paper we prove that the poincar map associated to a lorenz like flow has exponential decay of correlations with respect to lipschitz observables . this implies that the hitting time associated to the flow satisfies a logarithm law . its asymptotic behavior is a power law whose exponent is related to the local d... | in this paper we prove that the poincar map associated to a lorenz like flow has exponential decay of correlations with respect to lipschitz observables . this implies that the hitting time associated to the flow satisfies a logarithm law . the hitting time is the time needed for the orbit of a point to enter for the f... |
1012.0263 | i | two dimensional electronic systems on a honeycomb lattice have seen tremendous activity over the last couple of years . this development was triggered by the experimental isolation of single layer graphene which comes with a variety of fascinating and unusual properties @xcite . commonly , graphene is considered an ex... | the effect of either order is to break the sublattice inversion symmetry which induces a finite gap for the electronic single - particle excitations . we analyze two related formulations of the model by means of ( i ) a controlled renormalization group calculation and ( ii ) the large - n method , both of which in comb... | in this paper we study transport properties of electrons on the two - dimensional honeycomb lattice . we consider a half - filled system in the vicinity of a symmetry - breaking transition from a semimetallic phase towards an insulating phase with either charge density or spin density wave order . the effect of either ... |
1409.4313 | i | many engineering problems such as chemical reaction processes , heat conduction , nuclear reactors , population dynamics etc . are governed by coupled convection - diffusion - reaction partial differential equations ( pdes ) with non - linear source or sink terms . it is a significant challenge to solve such pdes numer... | in this work , we apply the adaptive discontinuous galerkin ( dgafem ) method to the convection dominated non - linear , quasi - stationary diffusion - convection - reaction equations . we propose an efficient preconditioner using a matrix reordering scheme to solve the sparse linear systems iteratively arising from th... | in this work , we apply the adaptive discontinuous galerkin ( dgafem ) method to the convection dominated non - linear , quasi - stationary diffusion - convection - reaction equations . we propose an efficient preconditioner using a matrix reordering scheme to solve the sparse linear systems iteratively arising from th... |
1502.02010 | i | population dynamics are a fundamental aspect of many biological processes . in this paper , we introduce and investigate a mathematical model for the population dynamics of an invasive species in a three - species food chain model . exotic species are defined as any species , capable of propagating themselves into a no... | in this work we develop and analyze a mathematical model of biological control to prevent or attenuate the explosive increase of an invasive species population in a three - species food chain . the controls avoid chemical treatments and/or natural enemy introduction , thus eliminating various non - target effects assoc... | in this work we develop and analyze a mathematical model of biological control to prevent or attenuate the explosive increase of an invasive species population in a three - species food chain . we allow for finite time blow - up in the model as a mathematical construct to mimic the explosive increase in population , en... |
0711.0705 | i | the compound channel consists of a set of channels indexed by @xmath1 with the same input and output alphabets but different conditional probabilities . in the setting of the compound channel only one actual channel @xmath2 is used in all transmissions . the transmitter and the receiver know the family of channels but ... | , we show that feedback does not increase the capacity of the compound gilbert - elliot channel . additionally , we show that for a stationary and uniformly ergodic markovian channel , if the compound channel capacity is zero without feedback then it is zero with feedback . finally , we use our result on the finite - s... | in this work we find the capacity of a compound finite - state channel with time - invariant deterministic feedback . the model we consider involves the use of fixed length block codes . our achievability result includes a proof of the existence of a universal decoder for the family of finite - state channels with feed... |
1111.2210 | i | the study of dirac points , i.e. the contact points between different energy bands with an approximate linear dispersion relation , has become a major issue since the experimental breakthrough in graphene - based electronics @xcite . indeed , the low - energy electronic properties of graphene are governed by a pseudo -... | inspired by the recent creation of the honeycomb optical lattice and the realization of the mott insulating state in a square lattice by shaking , we study here the shaken honeycomb optical lattice . for a periodic shaking of the lattice , a floquet theory may be applied to derive a time - independent hamiltonian . in ... | inspired by the recent creation of the honeycomb optical lattice and the realization of the mott insulating state in a square lattice by shaking , we study here the shaken honeycomb optical lattice . for a periodic shaking of the lattice , a floquet theory may be applied to derive a time - independent hamiltonian . in ... |
1111.2210 | r | honeycomb optical lattices have recently been realized experimentally , although the existing setups have only been used to investigate bosonic atoms @xcite . shaking of a lattice has been experimentally implemented in a one - dimensional one by a periodic modulation on the position of the reflecting mirrors @xcite . f... | furthermore , we include weak repulsive on - site interactions and find the density profiles for different values of the hopping parameters and interactions , both in a homogeneous system and in the presence of a trapping potential . our results may be experimentally observed by using momentum - resolved raman spectros... | inspired by the recent creation of the honeycomb optical lattice and the realization of the mott insulating state in a square lattice by shaking , we study here the shaken honeycomb optical lattice . for a periodic shaking of the lattice , a floquet theory may be applied to derive a time - independent hamiltonian . in ... |
0807.3481 | i | recently , considerable experimental progress has been made in the spectroscopy of baryons containing a single heavy quark . the cdf collaboration has observed four bottom baryons @xmath1 and @xmath2 @xcite . the do @xcite and cdf @xcite collaborations have seen the @xmath3 . the babar collaboration discovered the @xma... | inspired by the results of recent experimental discoveries for charm and bottom baryons , the masses and magnetic moments of the heavy baryons with containing a single heavy quark are studied within light cone qcd sum rules method . a comparison of our results on the magnetic moments of these baryons and the hyper cent... | inspired by the results of recent experimental discoveries for charm and bottom baryons , the masses and magnetic moments of the heavy baryons with containing a single heavy quark are studied within light cone qcd sum rules method . our results on the masses of heavy baryons are in good agreement with predictions of ot... |
1611.01635 | c | as demonstrated in refs . @xcite , both the scalar and vector lq scenarios could explain the anomalies observed in @xmath0 and @xmath1 decays and , for each scenario , there exist two best - fit solutions for the operator coefficients , because the other two solutions for scalar lq are already excluded by the @xmath137... | , we study their effects in the semi - leptonic decay . using the best - fit solutions for the operator coefficients allowed by the current data of mesonic decays , we find that ( i ) the two scenarios give the similar amounts of enhancements to the branching fraction and the ratio , ( ii ) the two best - fit solutions... | it has been shown that the anomalies observed in and decays can be resolved by adding a single scalar or vector leptoquark to the standard model , while constraints from other precision measurements in the flavour sector can be satisfied without fine - tuning . to further explore these two interesting scenarios , in th... |
hep-ph0601139 | i | a search through the spires database reveals over 350 articles whose titles contain the expressions ` quark jet(s ) ' or ` gluon jet(s ) ' @xcite . the idea of quark and gluon jets appears so intuitive that it hardly seems necessary to examine the question of what it means . yet , when going beyond leading order pertur... | it is common , in both theoretical and experimental studies , to separately discuss quark and gluon jets . however , even at parton level , widely - used jet algorithms fail to provide an infrared safe way of making this distinction . this can be a powerful tool when combining fixed - order calculations with multi - je... | it is common , in both theoretical and experimental studies , to separately discuss quark and gluon jets . however , even at parton level , widely - used jet algorithms fail to provide an infrared safe way of making this distinction . we examine the origin of the problem , and propose a solution in terms of a new ` fla... |
1107.4029 | i | when a low to intermediate mass star exhausts its core supply of hydrogen , contraction and heating of the core causes the outer layers of the star to expand and cool , whereby the star becomes a red giant ( rg ) with an average effective temperature of 5000k or lower . once the core temperature rises to about 3@xmath3... | known bright s stars , recognized as such by their enhanced s - process abundances and c / o ratio , are typically members of the asymptotic giant branch ( agb ) or the red giant branch ( rgb ) . few modern digital spectra for these objects have been published , from which intermediate resolution spectral indices and c... | known bright s stars , recognized as such by their enhanced s - process abundances and c / o ratio , are typically members of the asymptotic giant branch ( agb ) or the red giant branch ( rgb ) . few modern digital spectra for these objects have been published , from which intermediate resolution spectral indices and c... |
1303.4218 | i | multigraphs arise in many applications including modelling transportation networks @xcite , the structure of rna @xcite and in nonparametric statistics @xcite . we use terminology `` multigraphs '' inclusively , with both multiple edges and ( possibly multiple ) loops allowed . we seek an asymptotic enumeration form... | we find an asymptotic expression for the number of multigraphs on the vertex set with degree sequence given by , such that every loop has multiplicity in and every non - loop edge has multiplicity in . equivalently , these are symmetric integer matrices with values allowed on the diagonal and off the diagonal . our ... | let and be subsets of such that and . for infinitely many , let be a vector of nonnegative integers whose sum is even . we find an asymptotic expression for the number of multigraphs on the vertex set with degree sequence given by , such that every loop has multiplicity in and every non - loop edge has multiplicity i... |
1006.0444 | i | since the seminal work of tutte @xcite maps and graphs on 2-dimensional surfaces have become widely studied combinatorial objects in discrete mathematics . the enumerative and structural problems around maps , i.e. _ embedded _ graphs on a surface , are relatively well settled . starting from the number of planar map... | we study the component structure of . combining counting arguments with analytic techniques , the first one , of width , is analogous to the phase transition observed in the standard random graph models and takes place for , when the largest complex component is formed . then , for , when the complex components cover n... | let be a graph chosen uniformly at random from the family of all labeled planar graphs with vertices and edges . in the paper we study the component structure of . combining counting arguments with analytic techniques , we show that there are two critical periods in the evolution of . the first one , of width , is anal... |
1510.00129 | i | graph theory provide tools to study the algebraic properties of algebraic structures . in particular , there are several graphs associated with groups to study some specific properties of groups , for instance , intersection graph of subgroups of groups , prime graph of groups , non - commuting graphs of groups and per... | we define the _ coprime graph of subgroups _ of , denoted by , is a graph whose vertex set is the set of all proper subgroups of , and two distinct vertices are adjacent if and only if the order of the corresponding subgroups are coprime . in this paper , we study some connections between algebraic properties of a grou... | let be a group . we define the _ coprime graph of subgroups _ of , denoted by , is a graph whose vertex set is the set of all proper subgroups of , and two distinct vertices are adjacent if and only if the order of the corresponding subgroups are coprime . in this paper , we study some connections between algebraic pro... |
1510.00129 | r | [ order prime graph of subgroups 14 ] let @xmath40 and @xmath41 be two groups . if @xmath42 , then @xmath43 . let @xmath44 be a group isomorphism . define a map @xmath45 by @xmath46 , for every @xmath47 . since a group isomorphism preserves the order of subgroups , so it follows that @xmath48 is a graph isomorphism . *... | let be a group . [ [ mathematics - subject - classification ] ] mathematics subject classification : + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + 05c25 , 20k27 , 05c69 , 05c10 . | let be a group . we define the _ coprime graph of subgroups _ of , denoted by , is a graph whose vertex set is the set of all proper subgroups of , and two distinct vertices are adjacent if and only if the order of the corresponding subgroups are coprime . in this paper , we study some connections between algebraic pro... |
0903.0079 | i | an international array of first - generation long - baseline laser interferometric gravitational - wave ( gw ) detectors ( ligo @xcite , virgo @xcite , geo @xcite and tama @xcite ) are reaching their design sensitivities . these michelson interferometers have been built to measure gw - driven relative length change... | this result , along with the prospect for further improvements , heralds the new possibility of experimentally probing macroscopic quantum mechanics ( mqm ) quantum mechanical behavior of objects in the realm of everyday experience using gravitational - wave detectors . in this paper , we provide the mathematical fou... | long - baseline laser - interferometer gravitational - wave detectors are operating at a factor of ( in amplitude ) above the standard quantum limit ( sql ) within a broad frequency band ( in the sense that ) . such a low classical noise budget has already allowed the creation of a controlled 2.7 kg macroscopic oscilla... |
1612.07297 | i | the last two decades have seen an explosion in the study of complex systems , caused by the increasing relevance for society of such large interconnected structures , and by an unprecedented availability of data to analyze them . many of these systems can be modelled as networks , in which the system elements are repre... | many real - world complex networks exhibit a community structure , in which the modules correspond to actual functional units . identifying these communities is a key challenge for scientists . a common approach is to search for the network partition that maximizes a quality function . here in addition , we show that m... | many real - world complex networks exhibit a community structure , in which the modules correspond to actual functional units . identifying these communities is a key challenge for scientists . a common approach is to search for the network partition that maximizes a quality function . here , we present a detailed anal... |
1612.07297 | c | communities are a fundamental structure that is often present in real - world complex networks . thus , the ability to accurately and efficiently detect them is of great relevance to the analysis of complex data sets . despite their success , traditional methods based on modularity have been shown to suffer from limita... | , we present a detailed analysis of a recently proposed function , namely modularity density . we show that it does not incur in the drawbacks suffered by traditional modularity , and that it can identify networks without ground - truth community structure , deriving its analytical dependence on link density in generic... | many real - world complex networks exhibit a community structure , in which the modules correspond to actual functional units . identifying these communities is a key challenge for scientists . a common approach is to search for the network partition that maximizes a quality function . here , we present a detailed anal... |
1408.4767 | i | recently , a class of two - dimensional integrate and fire type models have been developed which can be fit to properties of real neurons . this class of models includes the adapting , leaky integrate and fire neuron ( lif ) @xcite , the izhikevich model @xcite , the quartic integrate and fire model @xcite , and the ad... | mean - field systems have been recently derived that adequately predict the behaviors of large networks of coupled integrate - and - fire neurons . the mean - field system for a network of neurons with spike frequency adaptation is typically a pair of differential equations for the mean adaptation and mean synaptic gat... | mean - field systems have been recently derived that adequately predict the behaviors of large networks of coupled integrate - and - fire neurons . the mean - field system for a network of neurons with spike frequency adaptation is typically a pair of differential equations for the mean adaptation and mean synaptic gat... |
1408.4767 | c | through our analysis of the mean field systems for large networks of coupled neurons , a number of new non - smooth bifurcations have been discovered that have been previously been unknown in the literature . these include two co - dimension 1 branches of boundary equilibrium bifurcations that have homoclinic limit cyc... | these two co - dimension 2 bifurcations can coalesce into a co - dimension 3 non - smooth bifurcation . as the mean - field system we study is a non - generic piecewise smooth continuous system , we discuss possible regularizations of this system and how the bifurcations which occur are related to non - smooth bifurcat... | mean - field systems have been recently derived that adequately predict the behaviors of large networks of coupled integrate - and - fire neurons . the mean - field system for a network of neurons with spike frequency adaptation is typically a pair of differential equations for the mean adaptation and mean synaptic gat... |
cs0609148 | i | although low - density parity - check block codes ( ldpc - bcs ) have very good performance under message - passing iterative ( mpi ) decoding , they are known to be subject to decoding failures due to so - called pseudo - codewords . these are real - valued vectors that can be loosely described as error patterns that ... | message - passing iterative decoders for low - density parity - check ( ldpc ) block codes are known to be subject to decoding failures due to so - called pseudo - codewords . these failures can cause the large signal - to - noise ratio performance of message - passing iterative decoding to be worse than that predicted... | message - passing iterative decoders for low - density parity - check ( ldpc ) block codes are known to be subject to decoding failures due to so - called pseudo - codewords . these failures can cause the large signal - to - noise ratio performance of message - passing iterative decoding to be worse than that predicted... |
astro-ph0009078 | i | ngc 1068 is a nearby heavily obscured seyfert 2 galaxy with a bright active galactic nucleus ( agn ) which has been studied in nearly every available wavelength band and at many spatial resolutions . its classification as a seyfert 2 nucleus rests on the basis of narrow emission lines . antonucci & miller ( 1985 ) h... | mid - infrared observations of the central source of ngc 1068 have been obtained with a spatial resolution in the deconvolved image of 0.1 ( pc ) . about two - thirds of its flux can be ascribed to a core structure which is itself elongated north - south and does not show a distinct unresolved compact source . | mid - infrared observations of the central source of ngc 1068 have been obtained with a spatial resolution in the deconvolved image of 0.1 ( pc ) . the central source is extended by in the north - south direction but appears unresolved in the east - west direction over most of its length . about two - thirds of its f... |
astro-ph0009078 | c | an overview of the energetics of ngc 1068 and how the present observations fit into the luminosity of ngc 1068 is provided by figure 2 which compares the flux per octave of the keck observations with the overall spectral energy distribution measured from ngc 1068 . the latter has been determined from the published ... | the source is strongly asymmetric , extending significantly further to the north than to the south . the morphology of the mid - infrared emission appears similar to that of the radio jet , and has features which correlate with the images in [ oiii ] . there are , however , detailed difficulties with existing models , ... | mid - infrared observations of the central source of ngc 1068 have been obtained with a spatial resolution in the deconvolved image of 0.1 ( pc ) . the central source is extended by in the north - south direction but appears unresolved in the east - west direction over most of its length . about two - thirds of its f... |
astro-ph0009078 | i | \1 ) mid - infrared observations of ngc 1068 at the diffraction limit of the keck 10-m telescope show a bright core containing about 1/3 the total flux accompanied by north - south emission about 70 pc long which is unresolved in the east west direction . thus most of the emission from the nuclear region of ngc 1068... | its 12.524.5 m color temperature ranges from 215 to 260k and does not decrease smoothly with distance from the core . silicate absorption is strongest in the core and to the south and is small in the north . the core , apparently containing two - thirds of the bolometric luminosity of the inner 4 diameter area , ma... | mid - infrared observations of the central source of ngc 1068 have been obtained with a spatial resolution in the deconvolved image of 0.1 ( pc ) . the central source is extended by in the north - south direction but appears unresolved in the east - west direction over most of its length . about two - thirds of its f... |
astro-ph9903158 | i | most attempts at modeling the emission from accreting black hole systems typically assume that the particle energy distribution responsible for the emission is either purely `` thermal '' ( i.e. , a maxwellian ) or purely `` non - thermal '' ( i.e. , a power law ) . this is partly due to the desire for convenience and ... | here , i review the arguments for `` thermal '' versus `` non - thermal '' plasmas in accreting black hole systems and discuss the physics and emission properties of `` hybrid '' plasmas , where the particle distribution energy is approximately a maxwellian plus a power law tail . using results from a new emission code... | models of the continuum radiation from accreting hot plasmas typically assume that the plasma heating mechanism produces energetic particles distributed in energy either as a maxwellian ( the `` thermal '' models ) or as an extended power law ( the `` non - thermal '' models ) . the reality , however , is that neither ... |
astro-ph9903158 | i | most attempts at modeling the emission from accreting black hole systems have typically assumed the underlying particle energy distribution is either a maxwellian ( `` thermal '' ) or a power law ( `` non - thermal '' ) . while such an assumption may be convenient analytically , it is no longer required given the adven... | models of the continuum radiation from accreting hot plasmas typically assume that the plasma heating mechanism produces energetic particles distributed in energy either as a maxwellian ( the `` thermal '' models ) or as an extended power law ( the `` non - thermal '' models ) . the reality , however , is that neither ... | models of the continuum radiation from accreting hot plasmas typically assume that the plasma heating mechanism produces energetic particles distributed in energy either as a maxwellian ( the `` thermal '' models ) or as an extended power law ( the `` non - thermal '' models ) . the reality , however , is that neither ... |
hep-ph0608140 | i | theoretical models constructed to understand physics beyond the standard model ( sm ) ( most notably string theory ) frequently imply the existence of extra dimensions . it has been a particular challenge in phenomenology to understand how these extra dimensions would be realized and manifested in our observable @xmath... | models of universal extra dimensions ( ued ) at the tev scale lead to the presence of kaluza klein ( kk ) excitations of the ordinary fermions and bosons of the standard model that may be observed at hadron and lepton colliders . a conserved discrete symmetry , kk - parity , ensures the stability of the lightest kk par... | models of universal extra dimensions ( ued ) at the tev scale lead to the presence of kaluza klein ( kk ) excitations of the ordinary fermions and bosons of the standard model that may be observed at hadron and lepton colliders . a conserved discrete symmetry , kk - parity , ensures the stability of the lightest kk par... |
1602.00656 | i | bulk iron selenide ( fese ) is an unconventional superconductor with a relatively modest transition temperature @xmath4 k at ambient pressures @xcite ; however , its @xmath5 can be increased by upwards of a factor of ten when a monolayer of fese is deposited on srtio@xmath6 ( sto ) @xcite or batio@xmath6 ( bto ) substr... | a number of proposals have been advanced for the mechanism of this enhancement . motivated by this , we explore the consequences of such an interaction on the superconducting state and electronic structure of a two - dimensional system using migdal - eliashberg theory . we also discuss the applicability of migdal - eli... | mono- and multilayer fese thin films grown on srtio and bitio substrates exhibit a greatly enhanced superconductivity over that found in bulk fese . a number of proposals have been advanced for the mechanism of this enhancement . one possibility is the introduction of a cross - interface electron - phonon (- ) interact... |
1602.00656 | r | we begin by presenting details of the spectral properties of our model , which illustrates the formation of the replica bands . this section will also serve to briefly review some of our results from ref [ fig : akw ] shows @xmath105 for @xmath113 and @xmath114 . results are shown for @xmath106 k @xmath115 k , and th... | one possibility is the introduction of a cross - interface electron - phonon (- ) interaction between the fese electrons and oxygen phonons in the substrates that is peaked in the forward scattering ( small direction due to the two - dimensional nature of the interface system . this interaction produces not only deviat... | mono- and multilayer fese thin films grown on srtio and bitio substrates exhibit a greatly enhanced superconductivity over that found in bulk fese . a number of proposals have been advanced for the mechanism of this enhancement . one possibility is the introduction of a cross - interface electron - phonon (- ) interact... |
math-ph0702005 | i | @xmath0 `` numerical ranges and @xmath0 '' numerical radii @xcite naturally relate to optimization problems on the unitary orbit of a given matrix . a particularly interesting class of applications concerns quantum systems as shown in more detail in the accompanying paper @xcite . this is because quantum dynamics and... | motivated by applications in quantum information and quantum control , a new type of `` numerical range , the relative '' numerical range denoted , is introduced . furthermore , we concentrate on the subgroup , i.e. the-fold tensor product of , which is of particular interest in applications . in this case , sufficie... | motivated by applications in quantum information and quantum control , a new type of `` numerical range , the relative '' numerical range denoted , is introduced . it arises upon replacing the unitary group in the definition of the classical " numerical range by any of its compact and connected subgroups . the ge... |
1105.0484 | r | the model is defined on a 1d lattice . at any time @xmath0 , a lattice site @xmath1 has @xmath2 particles of type @xmath3 and @xmath4 particles of type @xmath5 . we start with an empty lattice with @xmath6 sites at @xmath7 . at each instant , a site @xmath1 is chosen at random and one of the following moves ( illustrat... | it is found that , depending on the rates of various processes and the asymmetry in the hopping , the system may exist either in a steady phase , in which the average mass at each site attains a time - independent value , or in a `` growing '' phase , in which the total mass grows indefinitely in time , even in a finit... | motivated by the phenomenology of transport through the golgi apparatus of cells , we study a multi - species model with boundary injection of one species of particle , interconversion between the different species of particle , and driven diffusive movement of particles through the system by chipping of a single parti... |
1105.0484 | c | [ [ section-46 ] ] in this paper , motivated by the phenomenology of traffic in the golgi apparatus of the cell , we have studied a stochastic two - species model with boundary injection of type a , interconversion between types a and b , and transport of both species through the lattice ( in general , in a driven d... | motivated by the phenomenology of transport through the golgi apparatus of cells , we study a multi - species model with boundary injection of one species of particle , interconversion between the different species of particle , and driven diffusive movement of particles through the system by chipping of a single parti... | motivated by the phenomenology of transport through the golgi apparatus of cells , we study a multi - species model with boundary injection of one species of particle , interconversion between the different species of particle , and driven diffusive movement of particles through the system by chipping of a single parti... |
1011.0996 | i | there has been recent progress in understanding the phase diagram of higher - dimensional asymptotically flat vacuum black holes . the purpose of this work is to extend some of the techniques used to the case of asymptotically anti - de sitter ( ads ) black holes . let us first review the asymptotically flat case . whi... | myers - perry black holes with a single spin in have been shown to be unstable if rotating sufficiently rapidly . we extend the numerical analysis which allowed for that result to the asymptotically ads case . we determine numerically the stationary perturbations that mark the onset of the instabilities for the modes t... | myers - perry black holes with a single spin in have been shown to be unstable if rotating sufficiently rapidly . we extend the numerical analysis which allowed for that result to the asymptotically ads case . we determine numerically the stationary perturbations that mark the onset of the instabilities for the modes t... |
1608.03673 | i | near earth objects ( neos ) are small solar system bodies whose orbits bring them close to the earth s orbit . neos lie at the intersection of science , space exploration , and civil defense . because neos are constantly being replenished from sources elsewhere in the solar system , they act as compositional and dynami... | near earth objects ( neos ) are small solar system bodies whose orbits bring them close to the earth s orbit . we are carrying out a warm spitzer cycle 11 exploration science program entitled neosurvey a fast and efficient flux - limited survey of 597 known neos in which we derive diameter and albedo for each target... | near earth objects ( neos ) are small solar system bodies whose orbits bring them close to the earth s orbit . we are carrying out a warm spitzer cycle 11 exploration science program entitled neosurvey a fast and efficient flux - limited survey of 597 known neos in which we derive diameter and albedo for each target... |
astro-ph0611226 | i | theory suggests that supernovae and/or winds from massive stars existing in clusters confined to the disk of the galaxy produce bubbles in the interstellar medium which expand , becoming superbubbles , and burst out of the galactic disk producing collimated outflows into the galactic halo ( norman & ikeuchi 1989 ; teno... | new observations at high latitudes above the region w4 show that the structure formerly identified as a chimney candidate , an opening to the galactic halo , is instead a superbubble in the process of fragmenting and possibly evolving into a chimney . we explore the connection between w4 and the galactic halo , consid... | new observations at high latitudes above the region w4 show that the structure formerly identified as a chimney candidate , an opening to the galactic halo , is instead a superbubble in the process of fragmenting and possibly evolving into a chimney . data at high galactic latitudes ( ) above the w3/w4 star forming re... |
astro-ph0611226 | r | mosaics showing the spectral line emission at velocities of interest are shown in figures [ fig : hi-43.40_general ] , [ fig : hi-43.40_faint ] , [ fig : hi-40 ] , and [ fig : hi-48 ] . the mosaics of continuum emission at 408 mhz and 1420 mhz , stokes i , q and u are presented in figures [ fig:408 ] through [ fig :... | data at high galactic latitudes ( ) above the w3/w4 star forming region at 1420 and 408 mhz stokes i ( total power ) and 1420 mhz stokes q and u ( linear polarization ) reveal an egg - shaped structure with morphological correlations between our data and the data of dennison , topasna , & simonetti . we conclude that ... | new observations at high latitudes above the region w4 show that the structure formerly identified as a chimney candidate , an opening to the galactic halo , is instead a superbubble in the process of fragmenting and possibly evolving into a chimney . data at high galactic latitudes ( ) above the w3/w4 star forming re... |
astro-ph0608188 | i | with the measurement of visible linear polarization of field stars , followed by developments of near and far infrared ( respectively nir and fir ) and submillimetric polarimetry , it is now possible to trace magnetic field structures from the scale of the milky way to that of star forming regions and cores . in the di... | new visible polarization data combined with existing ir and fir polarization data are used to study how the magnetic field threading the filamentary molecular cloud gf 9 connects to larger structures in its general environment . the visible polarization is smooth and has a well - defined orientation . hence , in spite ... | new visible polarization data combined with existing ir and fir polarization data are used to study how the magnetic field threading the filamentary molecular cloud gf 9 connects to larger structures in its general environment . we find that when both visible and nir polarization data are plotted as a function of extin... |
astro-ph0608188 | c | as can be seen in figure [ polmap ] and in the histogram of position angles in figure [ anghisto ] , the polarization pattern in the vicinity of gf 9 is relatively well oriented on the plane of the sky with a mean direction of @xmath31 and a standard deviation @xmath50 . since the filament has an incurved concentric sh... | we find that when both visible and nir polarization data are plotted as a function of extinction , there is no evidence for a plateau or a saturation effect in the polarization at 1.3 as seen in dark clouds in taurus . the ir data are also well defined but with a different direction , and the fir data in the core regio... | new visible polarization data combined with existing ir and fir polarization data are used to study how the magnetic field threading the filamentary molecular cloud gf 9 connects to larger structures in its general environment . we find that when both visible and nir polarization data are plotted as a function of extin... |
astro-ph0608188 | c | visible linear polarization data taken at the mont - mgantic observatory on 78 stars in the vicinity of the dark filamentary cloud gf 9 were presented and compared with available nir and fir polarization data covering part of the same region . our main conclusions are : there is no evidence for saturation of pol... | this lack of saturation effect suggests that even in the denser parts of gf 9 we are still probing the magnetic field . a global interpretation of the results is that in the core region an original poloidal field could have been twisted by a rotating elongated ( coreenvelope ) structure . there is no evidence for turbu... | new visible polarization data combined with existing ir and fir polarization data are used to study how the magnetic field threading the filamentary molecular cloud gf 9 connects to larger structures in its general environment . we find that when both visible and nir polarization data are plotted as a function of extin... |
1308.5238 | i | our @xmath97 , nmr and nd data clearly demonstrate that @xmath239 exhibits a collinear afm ground state below @xmath4 = 9.8(2 ) k. the @xmath52al - nmr spectrum exhibits a symmetric broadening below 10 k which indicates the presence of a long - range afm ordered ground state for this compound . furthermore , the line ... | nuclear magnetic resonance ( nmr ) , neutron diffraction ( nd ) , x - ray diffraction , magnetic susceptibility and specific heat measurements on the frustrated-site spinel coalo compound reveal a collinear antiferromagnetic ordering below = 9.8(2 ) k. a high quality powder sample characterized by x - ray diffraction ... | nuclear magnetic resonance ( nmr ) , neutron diffraction ( nd ) , x - ray diffraction , magnetic susceptibility and specific heat measurements on the frustrated-site spinel coalo compound reveal a collinear antiferromagnetic ordering below = 9.8(2 ) k. a high quality powder sample characterized by x - ray diffraction ... |
1212.5172 | c | in order to assess the suitability of nanodiamonds as photonic ldos probes and as building blocks for hybrid photonic systems , we have investigated the brightness , decay rate , and quantum efficiency of single nv centers in nanodiamonds of 25 nm , and of 100 nm median size . for both size ranges a wide distribution i... | we report an experimental quantification of the brightness , radiative decay rate , nonradiative decay rate and quantum efficiency of single nv centers in diamond nanocrystals . we report that nv centers in 25 nm nanocrystals are essentially insensitive to local density of states ( ldos ) variations that we induce at a... | nv centers in diamond are generally recognized as highly promising as indefinitely stable highly efficient single - photon sources . we report an experimental quantification of the brightness , radiative decay rate , nonradiative decay rate and quantum efficiency of single nv centers in diamond nanocrystals . our exper... |
1204.0063 | i | the nature of the interaction between an accreting super - massive black hole ( smbh ) and its host galaxy remains a challenging problem in the study of galaxy evolution . numerical simulations reveal that gas can be drawn inward toward the nucleus by gravitational torques arising from a series of gravitational instabi... | observational and theoretical arguments suggest that the momentum carried in mass outflows from agn can reach several times , corresponding to outflow rates of hundreds of solar masses per year . radiation pressure on resonant absorption lines alone may not be sufficient to provide this momentum deposition , and the tr... | observational and theoretical arguments suggest that the momentum carried in mass outflows from agn can reach several times , corresponding to outflow rates of hundreds of solar masses per year . radiation pressure on resonant absorption lines alone may not be sufficient to provide this momentum deposition , and the tr... |
1701.04892 | r | table 1 lists the basic results for all of the models , namely the final times reached , the final spatial resolution employed , and the maximum number of virtual planets ( @xmath103 ) that formed and existed simultaneously , usually close to the final number of vps . the final times reached ranged from 244 yrs to 978 ... | the controversy extends to population synthesis models of exoplanet demographics and to hydrodynamical models of the fragmentation process . we show that the choice of is equal in importance to the value assumed : high disks can be stable for small , when the initial disk temperature is taken as a lower bound , while l... | observational evidence exists for the formation of gas giant planets on wide orbits around young stars by disk gravitational instability , but the roles of disk instability and core accretion for forming gas giants on shorter period orbits are less clear . the controversy extends to population synthesis models of exopl... |
astro-ph9911045 | i | diffraction limited mid - infrared observations of a sample of seven ulirgs obtained on the keck 10 m telescopes have shown : 1 - extremely compact structures , corresponding to emission on spatial scales of @xmath24100@xmath21200 pc , are seen in six of the seven systems observed . the mid - infrared emission in th... | we find extremely compact structures , with spatial scales of ( diameter ) in six of the seven ulirgs observed . we have utilized the compact mid - infrared structures as a diagnostic of whether an agn or a compact ( 100 300 pc ) starburst is the primary power source in these ulirgs . in markarian 231 , the upper limi... | observations of ultraluminous infrared galaxies ( ulirgs ) with an achieved resolution approaching the diffraction limit in the mid - infrared from 8 - 25 m using the keck telescopes are reported . we find extremely compact structures , with spatial scales of ( diameter ) in six of the seven ulirgs observed . these com... |
1112.6406 | i | in the recent years , deep near - infrared imaging surveys have begun to yield a significant number of candidate galaxies at very high redshifts . the wide - field surveys from the ground have produced a handful of bright candidates at @xmath6 ( e.g. , ouchi et al . 2009 ; hickey et al . 2010 ; castellano et al . 2010 ... | one key goal of the _ hubble space telescope _ cosmic assembly near - infrared deep extragalactic legacy survey is to track galaxy evolution back to . its two - tiered `` wide and deep '' strategy bridges significant gaps in existing near - infrared surveys . here we report on galaxy candidates selected as f105w - band... | one key goal of the _ hubble space telescope _ cosmic assembly near - infrared deep extragalactic legacy survey is to track galaxy evolution back to . its two - tiered `` wide and deep '' strategy bridges significant gaps in existing near - infrared surveys . here we report on galaxy candidates selected as f105w - band... |
1112.6406 | i | in this work , we search for candidate galaxies at @xmath0 in the candels deep goods - s field and study their properties . our sample of @xmath14-dropouts hints that the number density of @xmath0 galaxies at the bright - end might be higher than expected from the previous schechter lf estimates , which lends support t... | we derive constraints on the bright - end of the rest - frame ultraviolet luminosity function of galaxies at , and show that the number density of such very bright objects is higher than expected from the previous schechter luminosity function estimates at this redshift . another two candidates are securely detected in... | one key goal of the _ hubble space telescope _ cosmic assembly near - infrared deep extragalactic legacy survey is to track galaxy evolution back to . its two - tiered `` wide and deep '' strategy bridges significant gaps in existing near - infrared surveys . here we report on galaxy candidates selected as f105w - band... |
1511.08679 | i | exoplanetary system architectures have revealed numerous surprises since the first exoplanets were discovered . one of the earliest surprises was the discovery of exoplanets in highly eccentric orbits , for which there is no analog in the solar system . these eccentric orbits were discovered for giant planets , such as... | planets in highly eccentric orbits form a class of objects not seen within our solar system . here we present new data and analysis for this system as part of the transit ephemeris refinement and monitoring survey ( terms ) . we obtained chiron spectra to perform an independent estimation of the fundamental stellar par... | planets in highly eccentric orbits form a class of objects not seen within our solar system . the most extreme case known amongst these objects is the planet orbiting hd 20782 , with an orbital period of 597 days and an eccentricity of 0.96 . here we present new data and analysis for this system as part of the transi... |
1511.08390 | i | plasmon resonances , collective oscillations of a free - electron gas against a positive ion background , are subject to significant attentions.@xcite plasmon resonances , including both localized - plasmon resonances and plasmon waveguiding modes , can confine electric fields beyond the optical diffraction limit.@xcit... | plasmons are commonly interpreted with classical electrodynamics , while nonclassical effects may influence the dynamics of plasmon resonances as the plasmon confinement is approaching the few nanometer scale . however , an unambiguous approach to quantify the degree of nonclassical dynamics remains . we propose a _ n... | plasmons are commonly interpreted with classical electrodynamics , while nonclassical effects may influence the dynamics of plasmon resonances as the plasmon confinement is approaching the few nanometer scale . however , an unambiguous approach to quantify the degree of nonclassical dynamics remains . we propose a _ n... |
astro-ph0209560 | i | power spectrum estimation and evaluation of the associated errors in the presence of incomplete sky coverage ; non - homogeneous , correlated instrumental noise ; and foreground emission is a problem of central importance for the extraction of cosmological information from the cosmic microwave background . from a bayes... | power spectrum estimation and evaluation of associated errors in the presence of incomplete sky coverage ; non - homogeneous , correlated instrumental noise ; and foreground emission is a problem of central importance for the extraction of cosmological information from the cosmic microwave background . maps of the cmb ... | power spectrum estimation and evaluation of associated errors in the presence of incomplete sky coverage ; non - homogeneous , correlated instrumental noise ; and foreground emission is a problem of central importance for the extraction of cosmological information from the cosmic microwave background . we develop a mon... |
1608.07175 | i | [ [ section ] ] when experimenting with primes in division algebras , an affinity of primes in @xmath0 and @xmath1 with the structure in the standard model of particle physics emerged : primes in @xmath0 resemble leptons , while equivalence classes of primes in @xmath1 have hadron like features @xcite . in @xmath0 ,... | primes in the two complete associative normed division algebras and have affinities with structures seen in the standard model of particle physics . on the integers in the two algebras , weak equivalence classes within the strong equivalence classes of odd primes in case relate to leptons , the inert ones being neutrin... | primes in the two complete associative normed division algebras and have affinities with structures seen in the standard model of particle physics . on the integers in the two algebras , there are two equivalence relations : a strong one , related to a and symmetry allowing to permute and switch signs of the coordinate... |
0811.1081 | i | principal component analysis ( pca ) is one of the most valuable results from applied linear algebra , and probably the most popular method used for compacting higher dimensional data sets into lower dimensional ones for data analysis , visualization , feature extraction , or data compression @xcite . pca provides a st... | principal component analysis ( pca ) is a key statistical technique for multivariate data analysis . for large data sets the common approach to pca computation is based on the standard nipals - pca algorithm , which unfortunately suffers from loss of orthogonality , and therefore it s applicability is usually limited t... | principal component analysis ( pca ) is a key statistical technique for multivariate data analysis . for large data sets the common approach to pca computation is based on the standard nipals - pca algorithm , which unfortunately suffers from loss of orthogonality , and therefore it s applicability is usually limited t... |
hep-th9504098 | i | since the previous erice school on ` string quantum gravity ' a host of impressive developments has taken place on strings in curved spacetime . for the state of the art in 1992 we refer to the 1992 proceedings @xcite where the programme on string quantization in curved spacetimes initiated by us in 1987 @xcite is revi... | progress on string theory in curved spacetimes since 1992 are reviewed . after a short introduction on strings in minkowski and curved spacetimes , we focus on strings in cosmological spacetimes . the classical behaviour of strings in frw and inflationary spacetimes is now understood in a large extent from various t... | progress on string theory in curved spacetimes since 1992 are reviewed . after a short introduction on strings in minkowski and curved spacetimes , we focus on strings in cosmological spacetimes . the classical behaviour of strings in frw and inflationary spacetimes is now understood in a large extent from various t... |
gr-qc0406121 | i | the purpose of this paper is to present a novel approach to the unification of space - time physics and quantum theory . we take the view that classical space - time itself is not to be regarded as a primary object which is then subjected to some form of quantisation procedure . in our framework the central object is a... | it is shown that the causal geometry of such a quantum space - time possesses a rich hierarchical structure . in particular , we prove that the symmetry group of a quantum space - time is generated in general by a system of irreducible killing tensors . it is shown that the general such map satisfying appropriate causa... | quantum mechanics , quantum entanglement , causal spaces , + density matrices , cosmological models , hyperspinors + working paper : 29 june 2004 a generalised equivalence principle is put forward according to which _ space - time symmetries and internal quantum symmetries are indistinguishable before symmetry breaking... |
cond-mat0307619 | i | linear response theory ( lrt ) @xcite is the leading formalism to deal with driven systems . such systems are described by a hamiltonian @xmath2 where @xmath3 is a set of time dependent classical parameters ( `` fields '' ) . the kubo formula is the corner stone of lrt . it allows the calculation of the response coeffi... | we explain that the kubo formula contains all the physically relevant ingredients for the calculation of the pumped charge ( ) within the framework of linear response theory . we distinguish between adiabatic and dissipative contributions to . on the one hand we observe that adiabatic pumping does not have to be quant... | quantum pumping in closed systems is considered . we explain that the kubo formula contains all the physically relevant ingredients for the calculation of the pumped charge ( ) within the framework of linear response theory . the relation to the common formulations of adiabatic transport and geometric magnetism " is c... |
1311.3675 | i | spectrahedra are fundamental objects in convex algebraic geometry @xcite . a spectrahedron is the intersection of the cone of positive - semidefinite matrices with an affine subspace of the space of real symmetric @xmath2-matrices . in this paper , the subspace has dimension three and is identified with @xmath3 . the a... | quartic spectrahedra in-space form a semialgebraic set of dimension . there are twenty maximal strata , identified recently by degtyarev and itenberg , via the global torelli theorem for real k3 surfaces . we here give a new proof that is self - contained and algorithmic . this paper represents a first step towards the... | quartic spectrahedra in-space form a semialgebraic set of dimension . this set is stratified by the location of the ten nodes of the corresponding real quartic surface . there are twenty maximal strata , identified recently by degtyarev and itenberg , via the global torelli theorem for real k3 surfaces . we here give a... |
1512.00202 | i | one paradigm in studies of quantum chaos is the kicked harper model ( khm ) . it was originally introduced in ref . @xcite to model a kicked charge in a magnetic field . later a whole class of generalized versions of khm were introduced , which may also be realized via a periodically kicked charge in a magnetic field ... | recent discoveries on topological characterization of gapless systems have attracted interest in both theoretical studies and experimental realizations . examples of such gapless topological phases are weyl semimetals , which exhibit 3d dirac cones ( weyl points ) , and nodal line semimetals , which are characterized ... | recent discoveries on topological characterization of gapless systems have attracted interest in both theoretical studies and experimental realizations . examples of such gapless topological phases are weyl semimetals , which exhibit 3d dirac cones ( weyl points ) , and nodal line semimetals , which are characterized ... |
0708.3660 | i | the pipe nebula , at a distance of 130 pc , is one of the closest molecular cloud complexes in the galaxy . with a mass of 10@xmath6@xmath0 , it spans @xmath5 48 degs@xmath10 on the sky but contains little evidence for active star formation . in addition to tracing the larger - scale molecular gas associated with the p... | recent extinction studies of the pipe nebula ( d=130 pc ) reveal many cores spanning a range in mass from 0.2 to 20.4 . we present a survey of nh ( 1,1 ) , nh ( 2,2 ) , ccs ( 2 ) , and hcn ( 9,8)emission toward 46 of these cores . an atlas of the 2mass extinction maps is also presented . in total the derived properties... | recent extinction studies of the pipe nebula ( d=130 pc ) reveal many cores spanning a range in mass from 0.2 to 20.4 . these dense cores were identified via their high extinction and comprise a starless population in a very early stage of development . here we present a survey of nh ( 1,1 ) , nh ( 2,2 ) , ccs ( 2 ) , ... |
0708.3660 | c | using the 100 m gbt we have conducted an nh@xmath1 ( 1,1 ) , nh@xmath1 ( 2,2 ) , ccs ( 2@xmath21@xmath3 ) , and hc@xmath4n ( 9,8 ) survey toward a sample of 46 cores within the pipe nebula . these cores were identified via their high extinction and appear to be dense starless cores which likely represent the initial co... | these dense cores were identified via their high extinction and comprise a starless population in a very early stage of development . here , we detect 63% of the cores in nh ( 1,1 ) , 22% in nh ( 2,2 ) , 28% in ccs , and 9% in hcn emission . . such weak nh emission could arise due to low column densities and abundances... | recent extinction studies of the pipe nebula ( d=130 pc ) reveal many cores spanning a range in mass from 0.2 to 20.4 . these dense cores were identified via their high extinction and comprise a starless population in a very early stage of development . here we present a survey of nh ( 1,1 ) , nh ( 2,2 ) , ccs ( 2 ) , ... |
1611.02901 | i | a dessin denfant , introduced by grothendieck in its _ esquisse de un programme _ @xcite , is a @xmath0-cell embedding of a finite and connected bipartite graph @xmath1 on a closed orientable surface @xmath2 ; see @xcite for some generalities . the dessin denfant is called orientable if its faces can be labelled by sig... | recently , dessins denfants has been proven to be a powerful tool in certain types of supersymmetry gauge theories , bringing a relationship to combinatorics and number theory . dessins denfants are-cell embeddings of a finite and connected bipartite graph in a closed orientable surface . in general , a finite and conn... | recently , dessins denfants has been proven to be a powerful tool in certain types of supersymmetry gauge theories , bringing a relationship to combinatorics and number theory . dessins denfants are-cell embeddings of a finite and connected bipartite graph in a closed orientable surface . in general , a finite and conn... |
1504.05667 | i | there is a large number of problems that are well known to be hardly tractable with standard computational approaches and resources , mainly due to the many - body nature of strongly correlated many particle systems . to overcome this limitation , the idea of a quantum simulator was originally proposed by feynman @xcit... | a solution has been foreseen by directly simulating the time evolution through sequences of quantum gates applied to arrays of qubits , i.e. by implementing a _ digital quantum simulator_. superconducting circuits and resonators are emerging as an extremely - promising platform for quantum computation architectures , b... | resolving quantum many - body problems represents one of the greatest challenges in physics and physical chemistry , due to the prohibitively large computational resources that would be required by using classical computers . a solution has been foreseen by directly simulating the time evolution through sequences of qu... |
1611.06360 | i | in this paper , we present a numerical method for solving scattering problems from locally perturbed periodic surfaces . scattering problems for periodic or quasiperiodic incident fields from periodic structures have been well studied over at least 25 years . the common way of solving is reduction to one periodicity ce... | is to reduce such problems to one periodicity cell . in contrast to periodic settings , scattering from locally perturbed periodic surfaces is way more challenging . in this paper , we introduce and analyze a new numerical method to simulate scattering from locally perturbed periodic structures based on the bloch trans... | scattering problems for periodic structures have been studied a lot in the past few years . a main idea for numerical solution methods is to reduce such problems to one periodicity cell . in contrast to periodic settings , scattering from locally perturbed periodic surfaces is way more challenging . in this paper , we ... |
1412.7547 | i | algorithms for solving polynomial systems have become increasingly important over the past years , because of the many situations where such algebraic systems appear , including both theoretical problems ( algorithmic geometry , polynomial inversion ) , and real - life applications ( cryptography , robotics ) . examp... | solving polynomial systems arising from applications is frequently made easier by the structure of the systems . weighted homogeneity ( or quasi - homogeneity ) is one example of such a structure : given a system of weights ,-homogeneous polynomials are polynomials which are homogeneous w.r.t the weighted degree . g... | solving polynomial systems arising from applications is frequently made easier by the structure of the systems . weighted homogeneity ( or quasi - homogeneity ) is one example of such a structure : given a system of weights ,-homogeneous polynomials are polynomials which are homogeneous w.r.t the weighted degree . g... |
1404.1863 | i | spectral measures associated to the compact lie group @xmath1 and its maximal torus , nimrep graphs associated to the @xmath2 modular invariants , and the mckay graphs for finite subgroups of @xmath2 were studied in @xcite using information about the generating series of the moments of the spectral measure and the jone... | spectral measures provide invariants for braided subfactors via fusion modules . in this paper we study joint spectral measures associated to the rank two lie group , including the mckay graphs for the irreducible representations of and its maximal torus , and fusion modules associated to all known modular invariants . | spectral measures provide invariants for braided subfactors via fusion modules . in this paper we study joint spectral measures associated to the rank two lie group , including the mckay graphs for the irreducible representations of and its maximal torus , and fusion modules associated to all known modular invariants . |
1108.3564 | r | in this section , we present the evolution of the collapsing cloud and the outflow for typical models in [ sec : typical ] ( model n08 , less massive cloud case ) and [ sec : typical2 ] ( model n06 , massive cloud case ) . then , we describe the mass accretion rate ( [ sec : accretion ] ) and masses of the protostar... | , the protostellar outflow is driven by the circumstellar disk . the outflow extends also in the transverse direction until its width becomes comparable to the initial cloud scale , and thus , the outflow has a wide opening angle of . as a result , the protostellar outflow sweeps up a large fraction of the infalling ma... | star formation efficiency controlled by the protostellar outflow in a single cloud core is investigated by three - dimensional resistive mhd simulations . starting from the prestellar cloud core , the star formation process is calculated until the end of the main accretion phase . in the calculations , the mass of the ... |
1108.3564 | i | in this study , we investigated the impact of protostellar outflow on the star formation process . we constructed nine models with different initial cloud masses in the range of @xmath63 , and calculated the cloud evolution until the cloud mass is depleted . in the calculation , without artificially inputting outflow (... | the outflow can eject at most over half of the host cloud mass , significantly decreasing star formation efficiency . the outflow weakens significantly and disappears in several free - fall timescales of the initial cloud after the cloud begins to collapse . calculations show that typically ,% of the initial cloud mass... | star formation efficiency controlled by the protostellar outflow in a single cloud core is investigated by three - dimensional resistive mhd simulations . starting from the prestellar cloud core , the star formation process is calculated until the end of the main accretion phase . in the calculations , the mass of the ... |
cond-mat0109250 | i | questions concerning the nature of thermal fluctuations in fluids in thermal nonequilibrium states have been the subject of many studies during the past two decades . specifically , in this paper we consider thermal fluctuations in a horizontal layer of a one - component fluid that is heated either from above or from b... | the relevance of this theoretical result for the interpretation of light scattering and shadowgraph experiments is elucidated . the relationship with studies on various aspects of the problem by other investigators is discussed . the paper thus provides a unified treatment for dealing with fluctuations in fluid layers ... | starting from the linearized fluctuating boussinesq equations we derive an expression for the structure factor of fluids in stationary convection - free thermal nonequilibrium states , taking into account both gravity and finite - size effects . it is demonstrated how the combined effects of gravity and finite size cau... |
gr-qc0111028 | i | following up the investigation of holonomy in the schwarzschild spacetime by rothman et al @xcite , maartens et al @xcite have extended the work in @xcite on closed circular trajectories to the kerr spacetime where the spacetime rotation further complicates matters by introducing new features . maartens et al @xcite st... | the band of holonomy invariance found for a dense subset of special geodesic orbits outside a certain radius in the static case does not exist in the nonstatic case . in the kerr spacetime the dimensionless frequencies associated with parallel transport rotations can be expressed as ratios of the proper and average coo... | stationary axisymmetric spacetimes containing a pair of oppositely - rotating periodically - intersecting circular geodesics allow the study of various so - called ` clock effects ' by comparing either observer or geodesic proper time periods of orbital circuits defined by the observer or the geodesic crossing points .... |
1406.0442 | i | superconductivity in transition metal oxides ( copper oxides or cuprates ) , pnictides ( iron arsenides ) , or chalcogenides ( fese , kfe@xmath0se@xmath0 ) have attracted increasing attention recently , not only because of the extraordinary high transition temperatures achieved in some systems , but also because of the... | superconductivity in a novel class of layered materials , ti - based pnictide oxides , was recently discovered . these compounds have attracted interest since they combine features of copper oxide and iron pnictide superconductors . here the transition metal ( titanium ) forms two - dimensional tio layers ( anti struct... | superconductivity in a novel class of layered materials , ti - based pnictide oxides , was recently discovered . these compounds have attracted interest since they combine features of copper oxide and iron pnictide superconductors . here the transition metal ( titanium ) forms two - dimensional tio layers ( anti struct... |
1507.02308 | i | data on the cosmic microwave background ( cmb ) from the planck satellite @xcite and other experiments are qualitatively consistent with generic expectations from cosmological inflation @xcite . in particular , they are consistent with the prototypical starobinsky model based an @xmath0 extension of minimal einstein ... | no - scale inflation yields naturally predictions similar to those of the starobinsky model based on gravity , with a tilted spectrum of scalar perturbations : , and small values of the tensor - to - scalar perturbation ratio , as favoured by planck and other data on the cosmic microwave background ( cmb ) . detailed m... | supersymmetry is the most natural framework for physics above the tev scale , and the corresponding framework for early - universe cosmology , including inflation , is supergravity . no - scale supergravity emerges from generic string compactifications and yields a non - negative potential , and is therefore a plausibl... |
1507.02308 | i | as we have reviewed in this article , no - scale supergravity is an attractive framework for constructing models of inflation , since supersymmetry accommodates naturally the required hierarchy between the scale of inflation and the planck scale @xcite , gravity must be incorporated in any discussion of cosmology , an... | supersymmetry is the most natural framework for physics above the tev scale , and the corresponding framework for early - universe cosmology , including inflation , is supergravity . no - scale supergravity emerges from generic string compactifications and yields a non - negative potential , and is therefore a plausibl... | supersymmetry is the most natural framework for physics above the tev scale , and the corresponding framework for early - universe cosmology , including inflation , is supergravity . no - scale supergravity emerges from generic string compactifications and yields a non - negative potential , and is therefore a plausibl... |
0803.1924 | i | the lyman @xmath1 emission line has attracted large attention as a spectral signature for identifying galaxies and securing redshifts at large distances . this emission line , however , is fraught with difficulty . because ly@xmath1 photons are resonantly scattered by neutral hydrogen , they may suffer more dust attenu... | the _ galex ( galaxy evolution explorer ) _ spectroscopic survey mode , with a resolution of 8 in the fuv ( 1350 - 1750 ) and 20 in the nuv ( 1950 - 2750 ) is used for a systematic search of ly emitting galaxies at low redshift . | the _ galex ( galaxy evolution explorer ) _ spectroscopic survey mode , with a resolution of 8 in the fuv ( 1350 - 1750 ) and 20 in the nuv ( 1950 - 2750 ) is used for a systematic search of ly emitting galaxies at low redshift . this aims at filling a gap between high - redshift surveys and a small set of object... |
0803.1924 | c | a blind search of potential ly@xmath1 emission features has been conducted on 7018 spectra obtained in 5 deep spectroscopic exposures with _ galex_. 96 ly@xmath1 emitting galaxy candidates are identified , after a separation from agns essentially on the basis of the fwhm . they are mostly in the reshift range ( 0.2 @xm... | this aims at filling a gap between high - redshift surveys and a small set of objects studied in detail in the nearby universe . a blind search of 7018 spectra extracted in 5 deep exposures ( 5.65 sq.deg ) a sub - sample of 66 objects in the range has been used to build a ly lf ( luminosity function ) . | the _ galex ( galaxy evolution explorer ) _ spectroscopic survey mode , with a resolution of 8 in the fuv ( 1350 - 1750 ) and 20 in the nuv ( 1950 - 2750 ) is used for a systematic search of ly emitting galaxies at low redshift . this aims at filling a gap between high - redshift surveys and a small set of object... |
1303.2071 | i | the _ sp theory of intelligence _ aims to simplify and integrate ideas in artificial intelligence , mainstream computing , and human perception and cognition , with information compression as a unifying theme . the theory is described in several peer - reviewed articles , and links from there . ] and most fully in @xci... | the _ sp theory of intelligence _ aims to simplify and integrate concepts in computing and cognition , with information compression as a unifying theme . this article discusses how it may be applied to the understanding of natural vision and the development of computer vision . a strength of the sp theory is that it pr... | the _ sp theory of intelligence _ aims to simplify and integrate concepts in computing and cognition , with information compression as a unifying theme . this article discusses how it may be applied to the understanding of natural vision and the development of computer vision . the theory , which is described quite ful... |
1303.2071 | c | despite some limitations in how the sp theory is currently realised in computer models , it has what i believe are some useful things to say about several aspects of vision : * low level perceptual features such as edges or corners may be identified by the extraction of redundancy in uniform areas in a manner that i... | low level perceptual features such as edges or corners may be identified by the extraction of redundancy in uniform areas in a manner that is comparable with the run - length encoding technique for information compression . the concept of _ multiple alignment _ in the sp theory may be applied to the recognition of o... | the _ sp theory of intelligence _ aims to simplify and integrate concepts in computing and cognition , with information compression as a unifying theme . this article discusses how it may be applied to the understanding of natural vision and the development of computer vision . the theory , which is described quite ful... |
1108.1252 | i | the emission from narrow - line region ( nlr ) of active galactic nucleus ( agn ) is an important tool to study the relation between the activity of the central supermassive black hole ( smbh ) and the growth of its host galaxy in which the smbh resides , both because the nlr emission is mainly resulted from the illumi... | the agn - host co - evolution issue is investigated here by focusing on the evolution of the [ ] emission - line profile . in order to simultaneously measure both [ ] line profile and circumnuclear stellar population in individual spectrum , the evolutionary significance revealed here suggests that both nlr kinematics ... | the agn - host co - evolution issue is investigated here by focusing on the evolution of the [ ] emission - line profile . in order to simultaneously measure both [ ] line profile and circumnuclear stellar population in individual spectrum , a large sample of narrow emission - line galaxies is selected from the mpa / j... |
1108.1252 | c | we systematically examined the evolutionary issue of the [ ] @xmath0 emission - line profile by using a large sample of narrow emission - line galaxies selected from the mpa / jhu sdss dr7 value - added catalog . the sample is separated into three sub - samples ( i.e. , star - forming galaxies , transition galaxies and... | we show that the transition galaxies are systematically associated with narrower line widths and weaker [ ] broad wings than the agns , which implies that the kinematics of the emission - line gas is different in the two kinds of objects . by combining the measured host properties and line shape parameters , we find th... | the agn - host co - evolution issue is investigated here by focusing on the evolution of the [ ] emission - line profile . in order to simultaneously measure both [ ] line profile and circumnuclear stellar population in individual spectrum , a large sample of narrow emission - line galaxies is selected from the mpa / j... |
physics9912023 | i | the aim of this work is to develop the framework for the description of low - energy positron annihilation on molecules , and to analyse its two main mechanisms : direct and resonant annihilation . there are a number of remarkable phenomena associated with this process : very large annihilation rates @xcite , high sens... | the aim of this work is to identify the mechanisms responsible for very large rates and other peculiarities observed in low - energy positron annihilation on molecules . the two mechanisms considered are : ( i ) direct annihilation of the incoming positron with one of the molecular electrons . averaged over some energy... | the aim of this work is to identify the mechanisms responsible for very large rates and other peculiarities observed in low - energy positron annihilation on molecules . the two mechanisms considered are : ( i ) direct annihilation of the incoming positron with one of the molecular electrons . this mechanism dominates ... |
physics9912023 | r | if low - energy positron scattering is dominated by the presence of a virtual or weakly bound state at @xmath172 , the corresponding cross section has the form ( for scattering by a short - range potential @xcite ) @xmath173 where @xmath174 . according to eq . ( [ eq : zdir1 ] ) a similar maximum should appear in the m... | this mechanism dominates for atoms and small molecules . ( ii ) resonant annihilation , which takes place when the positron undergoes resonant capture into a vibrationally excited quasibound state of the positron - molecule complex . this mechanism dominates for larger molecules capable of forming bound states with the... | the aim of this work is to identify the mechanisms responsible for very large rates and other peculiarities observed in low - energy positron annihilation on molecules . the two mechanisms considered are : ( i ) direct annihilation of the incoming positron with one of the molecular electrons . this mechanism dominates ... |
physics9912023 | i | in this work i have considered two possible mechanisms of low - energy positron annihilation in binary collisions with molecules . the first mechanisms is direct annihilation . it describes positron annihilation with atoms and small molecules , as well as molecules which do not form bound states with the positron . the... | this mechanism is characterized by strong energy dependence of at small positron energies and high values ( up to ) for room temperature positrons , if a low - lying virtual level or a weakly bound state exists for the positron . the resonant mechanism can produce very large annihilation rates corresponding to . | the aim of this work is to identify the mechanisms responsible for very large rates and other peculiarities observed in low - energy positron annihilation on molecules . the two mechanisms considered are : ( i ) direct annihilation of the incoming positron with one of the molecular electrons . this mechanism dominates ... |
cond-mat9903146 | i | quantum corrections to the classical drude formula for the electrical conductivity give rise to singular terms in low - dimensional systems@xcite . there are two types of such terms . the first is known as the weak localization correction ( wl ) and arises as a result of the quantum interference of electron waves in di... | we discuss in a unifying way both weak localization and interaction effects in disordered systems . this allows us to show how dephasing arises both in the particle - particle channel ( weak localization ) and in the particle - hole channel ( interaction effect ) . we find that the latter may be suppressed by a static ... | the calculation of the dephasing time in electron systems is presented . by means of the keldysh formalism we discuss in a unifying way both weak localization and interaction effects in disordered systems . this allows us to show how dephasing arises both in the particle - particle channel ( weak localization ) and in ... |
1605.01504 | r | in its ground electronic state c@xmath1 has a fairly strong bond @xcite . the equilibrium bond distance of the state at 1.2425 is short for a double bond ( considerably shorter than the c = c bond of ethylene at @xmath151(c = c ) = 1.331 ) , but long for a triple bond ( in c@xmath1h@xmath1 @xmath151(cc ) = 1.203 ... | this well - determined energy difference should facilitate observations of singlet triplet intercombination lines which are thought to occur in the interstellar medium and comets . the large number of highly accurate and clearly labeled transitions that can be derived by combining marvel energy levels with computed te... | the carbon dimer , thec molecule , is ubiquitous in astronomical environments . experimental - quality rovibronic energy levels are reported forc , based on rovibronic transitions measured for and among its singlet , triplet , and quintet electronic states , reported in 42 publications . the determination utilizes the ... |
1605.01504 | i | this study utilizes the marvel technique to accurately determine close to 6,000 experimental rovibronic energies of @xmath0c@xmath1 for six singlet , six triplet , and two quintet electronic states , including the eight lowest valence states which gives coverage up to 35 000 @xmath4 . we survey all available laborator... | experimental - quality rovibronic energy levels are reported forc , based on rovibronic transitions measured for and among its singlet , triplet , and quintet electronic states , reported in 42 publications . the 23,343 transitions measured experimentally and validated within this study determine 5,699 rovibronic energ... | the carbon dimer , thec molecule , is ubiquitous in astronomical environments . experimental - quality rovibronic energy levels are reported forc , based on rovibronic transitions measured for and among its singlet , triplet , and quintet electronic states , reported in 42 publications . the determination utilizes the ... |
1207.3070 | i | in cataclysmic variable stars ( cvs ) , a white dwarf primary star accretes matter by way of roche lobe overflow from a binary companion , which resembles a main - sequence star . the variety of cv behaviors leads to a complicated taxonomy @xcite . many cvs undergo dwarf nova outbursts , thought to be caused by accreti... | the catalina real time survey ( crts ) has found over 500 cataclysmic variable ( cv ) candidates , most of which were previously unknown . we report here on followup spectroscopy of 36 of the brighter objects . one object appears to be a flare star , while another has a spectrum consistent with a cv but lies , intrigui... | the catalina real time survey ( crts ) has found over 500 cataclysmic variable ( cv ) candidates , most of which were previously unknown . we report here on followup spectroscopy of 36 of the brighter objects . nearly all the spectra are typical of cvs at minimum light . one object appears to be a flare star , while an... |
nucl-ex0002006 | i | beginning in the 1970 s significant advances in the understanding of nuclear multifragmentation were made possible with the advent of high statistics inclusive experiments . typically , only one intermediate mass fragment ( @xmath0 ) was detected per event . from these inclusive studies came the first evidence that in... | the cluster distributions of different systems are examined to search for signatures of a continuous phase transition . in a system known to possess such a phase transition , both sensitive and insensitive signatures are present ; while in systems known not to possess such a phase transition , only insensitive signatu... | the cluster distributions of different systems are examined to search for signatures of a continuous phase transition . in a system known to possess such a phase transition , both sensitive and insensitive signatures are present ; while in systems known not to possess such a phase transition , only insensitive signatu... |
1006.1271 | i | dilute magnetic semiconductors , such as ( ga , mn)as , form a class of materials with many outstanding properties@xcite and functionalities.@xcite a number of these result from the complex structure of the valence band , which hosts holes mediating magnetic order between spins localized on transition metal impurities ... | the collective behavior of spins in a dilute magnetic semiconductor is determined by their mutual interactions and influenced by the underlying crystal structure . hence , we begin with the atomic quantum - mechanical description of this system using the proposed variational - perturbation calculus , and then turn to t... | the collective behavior of spins in a dilute magnetic semiconductor is determined by their mutual interactions and influenced by the underlying crystal structure . hence , we begin with the atomic quantum - mechanical description of this system using the proposed variational - perturbation calculus , and then turn to t... |
1006.1271 | i | we have investigated spin waves and exchange stiffness in thin layers and bulk crystals of ferromagnetic ( ga , mn)as described by the @xmath1 tight - binding computational scheme . using the proposed variational - perturbation calculus , we have described the analyzed systems and their spin - wave excitations . their ... | we study spin waves and exchange stiffness in the zener model of ( ga , mn)as , its thin layers and bulk crystals described by the tight - binding approximation . analyzing the anisotropic part of exchange , we find that the dzyaloshinskii - moriya interaction may lead to a cycloidal spin arrangement and uniaxial in - ... | the collective behavior of spins in a dilute magnetic semiconductor is determined by their mutual interactions and influenced by the underlying crystal structure . hence , we begin with the atomic quantum - mechanical description of this system using the proposed variational - perturbation calculus , and then turn to t... |
1109.0154 | i | the coma cluster which was observed with the x - ray imaging spectrometer ( xis ) onboard suzaku , was analyzed by the x - ray satellite in six pointings , centered on the x - ray peak and offset by west , , , , and . because of its low background , suzaku is the most sensitive x - ray satellite for observing k@xmath1 ... | the coma cluster was observed with an x - ray imaging spectrometer ( xis ) onboard suzaku in six pointings , including the central x - ray peak region , the 14 west offset region , 30 and 34 north - west offset regions , and 44 and 60 south - west offset regions . the observed spectra were well - represented by a singl... | the coma cluster was observed with an x - ray imaging spectrometer ( xis ) onboard suzaku in six pointings , including the central x - ray peak region , the 14 west offset region , 30 and 34 north - west offset regions , and 44 and 60 south - west offset regions . owing to its lower background level , suzaku has better... |
1408.4134 | i | let @xmath13 or @xmath3 denote a compact , connected , orientable surface of genus @xmath14 , where @xmath1 . a simple closed curve on @xmath13 is _ essential _ if does not bound a disk in @xmath13 . the complex of curves , introduced by harvey @xcite , is the simplicial complex , @xmath15 , whose vertices ( or @xmath1... | the complex of curves of a closed orientable surface of genus is the simplicial complex whose vertices , , are isotopy classes of essential simple closed curves in . two vertices co - bound an edge of the-skeleton , , if there are disjoint representatives in . thus , the distance between two vertices , , corresponds to... | the complex of curves of a closed orientable surface of genus is the simplicial complex whose vertices , , are isotopy classes of essential simple closed curves in . two vertices co - bound an edge of the-skeleton , , if there are disjoint representatives in . a metric is obtained on by assigning unit length to each ed... |
1004.3492 | c | we have revisited the control landscape for several classes of canonical quantum control problems , in particular pure - state transfer and unitary gate optimization problems . although the pure - state transfer fidelity as a function over the unitary group only has two types of critical points , corresponding to eithe... | the control landscape for various canonical quantum control problems is considered . for the class of pure - state transfer problems , analysis of the fidelity as a functional over the unitary group reveals no suboptimal attractive critical points ( traps ) . for the actual optimization problem over controls in , howev... | the control landscape for various canonical quantum control problems is considered . for the class of pure - state transfer problems , analysis of the fidelity as a functional over the unitary group reveals no suboptimal attractive critical points ( traps ) . for the actual optimization problem over controls in , howev... |
1408.6505 | i | quantum optimal control theory ( oct ) provides a basis to explore applied field tuning of quantum system dynamics @xcite . recent successes include achieving control of electrons in quantum dots through time - varying gate voltages @xcite , controlling electronic correlations in molecules @xcite , manipulating the ... | the control of quantum system dynamics is generally performed by seeking a suitable applied field . the physical objective as a functional of the field forms the quantum control landscape , whose _ topology _ , under certain conditions , has been shown to contain no critical point suboptimal traps , thereby enabling ef... | the control of quantum system dynamics is generally performed by seeking a suitable applied field . the physical objective as a functional of the field forms the quantum control landscape , whose _ topology _ , under certain conditions , has been shown to contain no critical point suboptimal traps , thereby enabling ef... |
astro-ph9804012 | i | a galaxy can be well described by an ecosystem . there is an intimate relationship , much like a symbiosis , between the discrete components of the galaxy such as stars , and its interstellar medium ( ism ) . the ism provides the foundation for the birth of a new generation of stars , while at the same time it is enric... | the diffuse x - ray emission from the thin disk surrounding the galactic mid - plane ( the so - called galactic ridge ) was measured with _ rxte _ possible contributions from non - thermal bremsstrahlung of cosmic ray electrons and protons , inverse compton scattering of energetic electrons from ambient microwave , inf... | the diffuse x - ray emission from the thin disk surrounding the galactic mid - plane ( the so - called galactic ridge ) was measured with _ rxte _ pca in order to determine the spatial extent , spectral nature , and origin of the emission . spatial examination of the diffuse emission in the central of the plane in gala... |
astro-ph9804012 | c | we first consider the contribution of unresolved discrete sources to the diffuse emission spectrum . the important question is whether there exist classes of unresolved discrete sources with appropriate spatial number densities and similar spectra to that of the diffuse emission that can comprise the bulk of the spectr... | pca in order to determine the spatial extent , spectral nature , and origin of the emission spectral examination of the emission clearly reveals the presence of a hard power law tail above 10 kev and an emission line from he - like iron , indicating both thermal and possibly non - thermal origins for the diffuse emiss... | the diffuse x - ray emission from the thin disk surrounding the galactic mid - plane ( the so - called galactic ridge ) was measured with _ rxte _ pca in order to determine the spatial extent , spectral nature , and origin of the emission . spatial examination of the diffuse emission in the central of the plane in gala... |
astro-ph9804012 | c | our results are summarized as follows : ( 1 ) from the _ rxte _ survey of the galactic plane , we find that the diffuse emission from the galactic ridge has two spatial components : a thin disk of width @xmath240 , and a broad component with a functional form that can be approximated by a gaussian distribution of abou... | . spatial examination of the diffuse emission in the central of the plane in galactic longitude reveals the presence of two components : a thin disk of full width centered roughly on the galactic mid - plane , and a broad component which can be approximated as a gaussian distribution with fwhm of about . assuming an av... | the diffuse x - ray emission from the thin disk surrounding the galactic mid - plane ( the so - called galactic ridge ) was measured with _ rxte _ pca in order to determine the spatial extent , spectral nature , and origin of the emission . spatial examination of the diffuse emission in the central of the plane in gala... |
0901.0208 | i | let @xmath0 be a properly embedded , separating surface with no torus components in a compact , orientable 3-manifold @xmath5 . then the _ disk complex _ , @xmath6 , is defined as follows : 1 . vertices of @xmath6 are isotopy classes of compressions for @xmath0 . 2 . a set of @xmath7 vertices forms an @xmath8-simp... | the disk complex of a surface in a 3-manifold is used to define its _ topological index_. surfaces with well - defined topological index are shown to generalize well known classes , such as incompressible , strongly irreducible , and critical surfaces . the main result is that one may always isotope a surface with topo... | the disk complex of a surface in a 3-manifold is used to define its _ topological index_. surfaces with well - defined topological index are shown to generalize well known classes , such as incompressible , strongly irreducible , and critical surfaces . the main result is that one may always isotope a surface with topo... |
1004.5444 | i | for a heavy hadron which contains a single heavy quark ( bottom or charm ) , the heavy quark mass @xmath4 is much larger than the qcd energy scale @xmath5 which characterizes the light degrees of freedom in the heavy hadron . the four momentum of the heavy quark can be expressed as @xmath6 , where @xmath7 is taken to b... | a heavy quark expansion in terms of the inverse of the dressed heavy quark mass is presented with a complete decomposition of the full field and integrating out the small components . the heavy quark - antiquark coupling effects are included in the finite mass corrections . the extraction of from exclusive b decays is ... | the dressed heavy quark mass with being the binding energy is introduced to characterize the heavy hadrons containing a single heavy quark . a heavy quark expansion in terms of the inverse of the dressed heavy quark mass is presented with a complete decomposition of the full field and integrating out the small componen... |
1703.02911 | i | engines are machines that convert some form of energy ( e.g. , thermal or electrical energy ) into work . their efficiency , defined as the ratio of the extracted work to the invested energy , is restricted to @xmath0 at most by the energy - conservation law . while mechanical engines may reach this bound , carnot show... | quantum engines fuelled by non - thermal ( e.g. , squeezed - thermal ) baths have been shown to surpass this bound . yet , their maximum efficiency can not be determined by the reversibility condition , which may yield an unachievable efficiency bound above . this prompts the question : what does really limit the effi... | the efficiency of heat engines is limited by the carnot bound , attained when the engine cycle is reversible . quantum engines fuelled by non - thermal ( e.g. , squeezed - thermal ) baths have been shown to surpass this bound . yet , their maximum efficiency can not be determined by the reversibility condition , which ... |
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