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1312.5184
i
the lie co - algebra @xmath0 with coordinate functions @xmath1 has the lie poisson bracket @xmath2 for a given function @xmath3 the system of equations written as @xmath4 is called euler equations on @xmath0 with the hamilton function @xmath5 @xcite . suppose we have a rigid body rotating about a fixed point @xmath6 a...
we consider an example of a system with two degrees of freedom admitting separation of variables but having a subset of codimension 1 on which the 2-form defining the symplectic structure degenerates . new types of non - orientable 3-atoms are found . _ keywords _ : phase topology , separated variables , kowalevski ...
we consider an example of a system with two degrees of freedom admitting separation of variables but having a subset of codimension 1 on which the 2-form defining the symplectic structure degenerates . we show how to use separation of variables to calculate the exact topological invariant of non - degenerate singularit...
0901.1183
i
conductance quantization in a quantum point contact ( qpc ) , first observed in 1988@xcite , constitutes a classic textbook effect of mesoscopic physics . on top of the integer conductance plateaus @xmath0 ( where @xmath1 ) observed as a function of gate voltage @xmath2 , many experiments have found a temperature - dep...
we consider electron - electron interaction effects in quantum point contacts on the first quantization plateau , taking into account all scattering processes . we compute the low - temperature linear and nonlinear conductance , shot noise , and thermopower , by perturbation theory and a self - consistent nonperturbati...
we consider electron - electron interaction effects in quantum point contacts on the first quantization plateau , taking into account all scattering processes . we compute the low - temperature linear and nonlinear conductance , shot noise , and thermopower , by perturbation theory and a self - consistent nonperturbati...
1607.01764
i
quantum systems can ` tunnel ' through barriers , a wave - like behaviour that is a prototypical of non - classical behaviour . tunnelling plays a crucial role in a range of systems , including the theory of radioactivity , in which tunnelling is used to explain how radioactivity emerges from a nucleus despite the surr...
we consider in what sense quantum tunnelling is associated with non - classical probabilistic behaviour . we use the wigner function quasi - probability description of quantum states . we prove that this can only happen if either the wigner function is negative and/or a certain measurement operator which we call the tu...
we consider in what sense quantum tunnelling is associated with non - classical probabilistic behaviour . we use the wigner function quasi - probability description of quantum states . we give a definition of tunnelling that allows us to say whether in a given scenario there is tunnelling or not . we prove that this ca...
1604.07169
i
_ probabilistic programs . _ classic imperative programs extended with _ random - value generators _ gives rise to probabilistic programs . probabilistic programs provide the appropriate framework to model applications ranging from randomized algorithms @xcite , to stochastic network protocols @xcite , to robot plann...
we consider nondeterministic probabilistic programs with the most basic liveness property of termination . we present efficient methods for termination analysis of nondeterministic probabilistic programs with polynomial guards and assignments . our approach is through synthesis of polynomial ranking supermartingales , ...
we consider nondeterministic probabilistic programs with the most basic liveness property of termination . we present efficient methods for termination analysis of nondeterministic probabilistic programs with polynomial guards and assignments . our approach is through synthesis of polynomial ranking supermartingales , ...
1406.0969
i
in this paper we are interested in the polynomials @xmath0 that are orthogonal with respect to the weight function @xmath1 on @xmath2 , where @xmath1 is the bessel function of order @xmath8 . the bessel function is oscillatory with an amplitude that decays like @xmath9 as @xmath10 , and therefore the moments @xmath11 d...
we consider polynomials orthogonal with respect to the weight on , where is the bessel function of order . asheim and huybrechs considered these polynomials in connection with complex gaussian quadrature for oscillatory integrals . they observed that the zeros are complex and accumulate as near the vertical line . our ...
we consider polynomials orthogonal with respect to the weight on , where is the bessel function of order . asheim and huybrechs considered these polynomials in connection with complex gaussian quadrature for oscillatory integrals . they observed that the zeros are complex and accumulate as near the vertical line . we p...
1002.1404
i
in quantum transport theory , a nanosystem inside which the electrons do not interact has a zero temperature conductance which is given ( in units of the conductance quantum @xmath19 for spin polarized electrons , @xmath20 with spin degeneracy ) by @xmath21 where @xmath22 is the probability for an electron at the fermi...
we consider quantum transport of spinless fermions in a 1d lattice embedding an interacting region ( two sites with inter - site repulsion and inter - site hopping , coupled to leads by hopping terms ) . this universality characterizes the non - interacting regime where , the perturbative regime ( ) where can be obtain...
we consider quantum transport of spinless fermions in a 1d lattice embedding an interacting region ( two sites with inter - site repulsion and inter - site hopping , coupled to leads by hopping terms ) . using the numerical renormalization group for the particle - hole symmetric case , we study the quantum conductance ...
1503.04314
i
the hamiltonian @xmath0 of a physical system represents its energy , which is a real observable . it is therefore required that the expectation values of the quantum operator @xmath0 be real @xcite . this can be guaranteed by imposing that @xmath0 be hermitian , @xmath1 , as it is known that the spectrum of a hermitian...
we consider the class of non - hermitian operators represented by infinite tridiagonal matrices , selfadjoint in an indefinite inner product space with one negative square . we approximate them with their finite truncations . both infinite and truncated matrices have eigenvalues of nonpositive type : either a single on...
we consider the class of non - hermitian operators represented by infinite tridiagonal matrices , selfadjoint in an indefinite inner product space with one negative square . we approximate them with their finite truncations . both infinite and truncated matrices have eigenvalues of nonpositive type : either a single on...
1510.05909
i
ever since the concept of topological order in condensed matter systems picked up momentum during the last decade,@xcite there has been the question as to which kind of perturbations can cause topological phase transitions . in this paper , we investigate the possibility to utilize inhomogeneous perturbations , like th...
we start by identifying the general conditions under which the eigenenergies of an arbitrary hamiltonian belonging to one of the altland - zirnbauer symmetry classes undergo a robust zero energy crossing as a function of an external parameter which can be , for example , the impurity strength . we use the generalized r...
we consider the effects of impurities on topological insulators and superconductors . we start by identifying the general conditions under which the eigenenergies of an arbitrary hamiltonian belonging to one of the altland - zirnbauer symmetry classes undergo a robust zero energy crossing as a function of an external p...
1510.05909
i
in summary , we have identified the general conditions under which the eigenenergies of the hamiltonian undergo a robust zero - energy crossing as a function of external parameters in different altland - zirnbauer symmetry classes . we defined @xmath8 as a generalized root of @xmath1 and used it to predict or to rule o...
we define a generalized root of , and use it to predict or rule out robust zero - energy crossings in all symmetry classes . we complement this result with an analysis based on almost degenerate perturbation theory , which allows a derivation of the asymptotic low - energy behavior of the ensemble averaged density of s...
we consider the effects of impurities on topological insulators and superconductors . we start by identifying the general conditions under which the eigenenergies of an arbitrary hamiltonian belonging to one of the altland - zirnbauer symmetry classes undergo a robust zero energy crossing as a function of an external p...
astro-ph0403200
i
since @xcite , following early proposals by @xcite and @xcite , suggested that strange quark matter , consisting of @xmath0- , @xmath1- and @xmath2-quarks is energetically the most favorable state of the matter , the problem of existence of strange quark stars has been intensively investigated in the physical and astro...
the dynamics of the nucleation essentially depends on the physical properties of the medium it takes place . the conditions for quark bubble formation are analyzed within the frameworks of both dissipative and non - dissipative ( with zero bulk and shear viscosity coefficients ) approaches . we analyze the first order ...
we consider the general conditions of quark droplets formation in high density neutron matter . the growth of the quark bubble ( assumed to contain a sufficiently large number of particles ) can be described by means of a fokker - planck equation . the dynamics of the nucleation essentially depends on the physical prop...
1512.00681
i
the solution of the time - dependent schrdinger equation ( tdse ) that describes the interaction of an intense electromagnetic pulse with an atom or a molecule is a very challenging problem from the numerical point of view . this is particularly true in the long wavelength limit where the numerical calculations become ...
we consider the interaction of hydrogen - like atoms with a strong laser field and show that the strong field approximation and all its variants may be grouped into a set of families of approximation schemes . furthermore , this new formulation of the strong field approximations allows us to gain deeper insight into th...
we consider the interaction of hydrogen - like atoms with a strong laser field and show that the strong field approximation and all its variants may be grouped into a set of families of approximation schemes . this is done by introducing an ansatz describing the electron wave packet as the sum of the initial state wave...
1512.00681
c
in this contribution , we showed that the various treatments based on the strong field approximation may be grouped into a set of families of approximation schemes . we introduced different ansatzes that describe the electron wave packet as the sum of the initial state wave function multiplied by a phase factor and a f...
this is done by introducing an ansatz describing the electron wave packet as the sum of the initial state wave function times a phase factor and a function which is the perturbative solution in the coulomb potential of an inhomogeneous time - dependent schrdinger equation . it is the phase factor that characterizes a g...
we consider the interaction of hydrogen - like atoms with a strong laser field and show that the strong field approximation and all its variants may be grouped into a set of families of approximation schemes . this is done by introducing an ansatz describing the electron wave packet as the sum of the initial state wave...
1407.5369
i
in a seminal work , haldane demonstrated that a magnetic field is not required to induce integer quantum hall states @xcite . adding a complex hopping to the tight - binding hamiltonian on the honeycomb lattice opens a gap at the dirac points of the electron band structure . this gap leads to a topologically nontrivia...
these singularites include dirac points , quadratic fermi points in contact with a flat band , and van hove saddle points . by combining a controlled analytical approach with large - scale numerical simulations , in particular , some of these magnetic orderings produce a spontaneous quantum anomalous hall state .
we consider the kondo - lattice model on the kagome lattice and study its weak - coupling instabilities at band filling fractions for which the fermi surface has singularities . these singularites include dirac points , quadratic fermi points in contact with a flat band , and van hove saddle points . by combining a con...
1604.06430
c
we explore the low scale implications in the @xmath0 extended mssm ( umssm ) . we restrict the parameter space such that the lightest supersymmetric particle ( lsp ) is always the lightest neutralino . in addition , we impose quasi yukawa unification ( qyu ) at the grand unification scale ( @xmath1 ) . the fundamental ...
we consider the low scale implications in the extended mssm ( umssm ) . we restrict the parameter space such that the lightest supersymmetric particle ( lsp ) is always the lightest neutralino . in addition , we impose quasi yukawa unification ( qyu ) at the grand unification scale ( ) . qyu strictly requires the ratio...
we consider the low scale implications in the extended mssm ( umssm ) . we restrict the parameter space such that the lightest supersymmetric particle ( lsp ) is always the lightest neutralino . in addition , we impose quasi yukawa unification ( qyu ) at the grand unification scale ( ) . qyu strictly requires the ratio...
cs0605041
i
we consider the basic multiple - access communication problem in a distributed setting . in gallager s survey paper @xcite , it is pointed out that the multiple - access problem has been studied from a number of different perspectives , each having its own advantages and shortcomings . in the data networking community ...
we consider the multiple - access communication problem in a distributed setting for both the additive white gaussian noise channel and the discrete memoryless channel . we propose a scheme called distributed rate splitting to achieve the optimal rates allowed by information theory in a distributed manner . in this sch...
we consider the multiple - access communication problem in a distributed setting for both the additive white gaussian noise channel and the discrete memoryless channel . we propose a scheme called distributed rate splitting to achieve the optimal rates allowed by information theory in a distributed manner . in this sch...
1103.1489
r
we start with some preliminary definitions and facts . for any lebesgue integrable function @xmath32 the fourier transform @xmath33 $ ] of @xmath34 is defined as @xmath33(t ) = \int_{\mathbb{r}}h(x)e^{-itx}\,dx$ ] , @xmath35 and we use the natural extension of @xmath36 to @xmath37 . we further denote by @xmath38 the in...
we then derive lower bounds for the minimax sup - norm risk over besov balls in this estimation problem and show that wavelet deconvolution density estimators attain these bounds . we further show that linear estimators adapt to the unknown smoothness of if the fourier transform of decays exponentially and that a corre...
we consider the statistical deconvolution problem where one observes replications from the model , where is the unobserved random signal of interest and is an independent random error with distribution . under weak assumptions on the decay of the fourier transform of we derive upper bounds for the finite - sample sup ...
1508.01193
i
the geometrization of duality groups has been the source of many insights both in string and field theories . perhaps the simplest example is that of montonen - olive duality in four - dimensional @xmath6 sym , where the discrete @xmath7 group acting on the complexified coupling @xmath8 is interpreted as the modular gr...
we construct a class of codimension-2 solutions in supergravity that realize t - folds with arbitrary monodromy and we develop a geometric point of view in which the monodromy is identified with a product of dehn twists of an auxiliary surface fibered on a base . these defects , that we call t - fects , are identified ...
we construct a class of codimension-2 solutions in supergravity that realize t - folds with arbitrary monodromy and we develop a geometric point of view in which the monodromy is identified with a product of dehn twists of an auxiliary surface fibered on a base . these defects , that we call t - fects , are identified ...
math0309049
i
since rubinstein s announcement of an algorithm to recognize the 3-sphere in 1993 @xcite , almost normal surfaces , the main technical innovation of that work , have received wide attention . in 1994 thompson @xcite reworked rubinstein s proof of the existence of an almost normal 2-sphere in @xmath7 using gabai s langu...
our main result is the following : suppose ( or ) is an irreducible submanifold of a triangulated 3-manifold , bounded by a normal or almost normal surface , and containing at most one maximal normal 2-sphere . if is a strongly irreducible hst splitting of then we may isotope it so that for each even value of the surfa...
we define a heegaard - scharlemann - thompson ( hst ) splitting of a 3-manifold to be a sequence of pairwise - disjoint , embedded surfaces , , such that for each odd value of , is a heegaard splitting of the submanifold of cobounded by and . our main result is the following : suppose ( or ) is an irreducible submanifo...
1411.7807
i
lagrangian floer homology for open subsets in cotangent bundles was introduced by kasturirangan and oh in @xcite as a part of a project of `` quantization of eilenberg steenrod axioms '' ( see @xcite ) . the construction goes as follows . let @xmath1 be an open subset of a compact smooth manifold @xmath3 , with a sm...
we define and investigate spectral invariants for floer homology of an open subset in , defined by kasturirangan and oh as a direct limit of floer homologies of approximations . we define a module structure product on and prove the triangle inequality for invariants with respect to this product . we also prove the cont...
we define and investigate spectral invariants for floer homology of an open subset in , defined by kasturirangan and oh as a direct limit of floer homologies of approximations . we define a module structure product on and prove the triangle inequality for invariants with respect to this product . we also prove the cont...
0708.2533
i
in special and general relativity the spin of a gyroscope is represented by a four - vector @xmath0 . assuming that we move the gyroscope without applying any torque to it ( in a system comoving with the gyroscope ) , the spin vector will obey the fermi transport equation @xmath1 here @xmath2 is the four - velocity of ...
starting from the fermi transport equation for the standard spin vector we derive a corresponding transport equation for the stopped spin vector . employing a spacetime transport equation for a vector along a worldline , corresponding to spatial parallel transport with respect to the congruence , we can write down a pr...
we derive an effectively three - dimensional relativistic spin precession formalism . the formalism is applicable to any spacetime where an arbitrary timelike reference congruence of worldlines is specified . we employ what we call a _ stopped _ spin vector which is the spin vector that we would get if we momentarily m...
math0603410
i
the aim of this paper is to explore the connections between the problem of counting the number of partial matchings in graphs and positive hyperbolic polynomials , and ryser - like formulas for partial matchings . given a graph @xmath1 on @xmath2 vertices , i.e. @xmath3 , we want to compute the number of @xmath4-matchi...
we derive here the friedland - tverberg inequality for positive hyperbolic polynomials . this inequality is applied to give lower bounds for the number of matchings in-regular bipartite graphs . it is shown that some of these bounds are asymptotically sharp . we improve the known lower bound for the three dimensional m...
we derive here the friedland - tverberg inequality for positive hyperbolic polynomials . this inequality is applied to give lower bounds for the number of matchings in-regular bipartite graphs . it is shown that some of these bounds are asymptotically sharp . we improve the known lower bound for the three dimensional m...
astro-ph0202402
r
as noted in 1 , oblique shocks are likely to play a major role in the understanding of evolving parsec - scale jets , and in the detailed morphology of kiloparsec - scale flows such as m 87 . while models based on transverse propagating shocks have been extremely successful in explaining both the radio polarization a...
we find that even quite fast jets ( ) can be significantly influenced by impinging on an oblique density gradient , exhibiting a rotation of the mach disk in the jet s head . the flow is bent via a potentially strong , oblique internal shock that arises due to asymmetric perturbation of the flow by its cocoon . in extr...
we describe a new numerical 3d relativistic hydrodynamical code and present the results of three validation tests . a comparison of an axisymmetric jet simulation using the 3d code , with corresponding results from an earlier 2d code , reveal that a ) the enforcement of axisymmetry in the 2d case had no significant inf...
cond-mat9703179
c
we have discussed a number of recently developed cluster algorithms for the simulation of classical spin systems , including : the wolff algorithm , which flips a single cluster of spins at each update step and almost completely eliminates critical slowing down from the simulation of the ising model ; the swendsen - wa...
we describe a number of recently developed cluster - flipping algorithms for the efficient simulation of classical spin models near their critical temperature . these include the algorithms of wolff , swendsen and wang , and niedermeyer , as well as the limited cluster algorithm , the multigrid methods of kandel and co...
we describe a number of recently developed cluster - flipping algorithms for the efficient simulation of classical spin models near their critical temperature . these include the algorithms of wolff , swendsen and wang , and niedermeyer , as well as the limited cluster algorithm , the multigrid methods of kandel and co...
astro-ph9802356
c
we have performed a radial velocity survey of a total of 153 field wds and sdbs , most of which were not previously known to be binary . in the combined sample , we have discovered 18 new dd candidates with wd or sdb primaries , and 1 new confirmed wd+ms pair . among the 7 sdb variables , we have obtained orbital solut...
we describe radial velocity observations of a large sample of apparently single white dwarfs ( wds ) , obtained in a long - term effort to discover close , double - degenerate ( dd ) pairs which might comprise viable type ia supernova ( ) progenitors . follow - up observations are in progress to solve for the orbital p...
we describe radial velocity observations of a large sample of apparently single white dwarfs ( wds ) , obtained in a long - term effort to discover close , double - degenerate ( dd ) pairs which might comprise viable type ia supernova ( ) progenitors . we augment the wd sample with a previously observed sample of appar...
1002.3366
i
one of the great hopes for current and future particle colliders is that they will be able to produce dark matter . in this study , we determine the prospects for finding dark matter through the production of exotic 4th generation quarks @xmath0 that decay through @xmath1 , where @xmath2 is dark matter . current direct...
we determine the prospects for finding dark matter at the tevatron and lhc through the production of exotic 4th generation quarks that decay through , where is dark matter . the resulting signal of has not previously been considered in searches for 4th generation quarks , but there are both general and specific dark ma...
we determine the prospects for finding dark matter at the tevatron and lhc through the production of exotic 4th generation quarks that decay through , where is dark matter . the resulting signal of has not previously been considered in searches for 4th generation quarks , but there are both general and specific dark ma...
1505.06535
i
electron - transport calculations are important tools to investigate and develop materials for new electronic devices . recently , to obtain more practical knowledge on electron - transport properties of nanoscale structures , long - range and large - scale transport simulations have attracted much interest . however ,...
we develop a first - principles electron - transport simulator based on the lippmann schwinger ( ls ) equation within the framework of the real - space finite - difference scheme . in our fully real - space based ls ( grid ls ) method , the ratio expression technique for the scattering wave functions and the green s f...
we develop a first - principles electron - transport simulator based on the lippmann schwinger ( ls ) equation within the framework of the real - space finite - difference scheme . in our fully real - space based ls ( grid ls ) method , the ratio expression technique for the scattering wave functions and the green s f...
hep-th9502003
c
in this paper we have emphasised that the quantum fluctuations of the goldstone bosons have some drastic effects which are not encountered either in a tree level or loopwise analysis of the linear or the non - linear @xmath3- models.nevertheless,the leading infrared behaviour of the correlation functions again become i...
renormalization group flows , ii ) . schwinger - dyson equations.we also obtain an explicit form for the generating functional of one - particle irreducible vertices of the o(n ) ( non)linearmodels in the leading approximation.we show that this incorporates all infrared behaviour correctly both in linear and non - line...
we develop various complementary concepts and techniques for handling quantum fluctuations of goldstone bosons.we emphasise that one of the consequences of the masslessness of goldstone bosons is that the longitudinal fluctuations also have a diverging susceptibility characterised by an anomalous dimension in space - t...
1411.2607
i
over the recent decades , matrix product states ( mps ) @xcite and related numerical techniques have become the standard framework for simulating low energy states of local hamiltonians in 1d . mps with finite bond dimension provide an exact representation of the ground state only for a certain well - designed class of...
we discuss how to analytically obtain an essentially infinite matrix product state ( mps ) representation of the ground state of the xy model . on the one hand this allows to illustrate how the ornstein - zernike form of the correlation function emerges in the exact case using standard mps language . this provides a ...
we discuss how to analytically obtain an essentially infinite matrix product state ( mps ) representation of the ground state of the xy model . on the one hand this allows to illustrate how the ornstein - zernike form of the correlation function emerges in the exact case using standard mps language . on the other han...
1001.5071
i
much experimental progress has recently been achieved in the area of ultra - cold atoms . it is now possible @xcite to make systems of atoms confined in optical lattices formed by laser beams and at the same time control the strength of the two - body interaction with magnetic fields . the atoms are cooled down to extr...
we discuss the problem of two particles interacting via short - range interactions within a harmonic - oscillator trap . the interactions are organized according to their number of derivatives and defined in truncated model spaces made from a bound - state basis . we show explicitly that next - to - lo and next - to - ...
we discuss the problem of two particles interacting via short - range interactions within a harmonic - oscillator trap . the interactions are organized according to their number of derivatives and defined in truncated model spaces made from a bound - state basis . leading - order ( lo ) interactions are iterated to all...
1111.4049
c
the existence of traversable wormholes in the context of general relativity relies on the presence of some form of exotic matter . however , in the framework of a string - inspired generalized theory of gravity , the situation may be completely different . here we have investigated wormhole solutions in egbd theory , w...
these wormholes do not need any form of exotic matter for their existence . a subset of these wormholes is shown to be linearly stable with respect to radial perturbations . we perform a comprehensive study of their domain of existence , and derive a generalised smarr relation for these wormholes .
we discuss the properties of lorentzian wormholes in dilatonic einstein - gauss - bonnet theory in four spacetime dimensions . these wormholes do not need any form of exotic matter for their existence . a subset of these wormholes is shown to be linearly stable with respect to radial perturbations . we perform a compre...
1105.5113
i
the origin and chemical composition of uhe crs ( @xmath5 ev ) is a long - standing enigma in cr physics @xcite . the spectrum at these energies is expected to be dominated by extragalactic sources that have not yet been unambiguously identified . the average mass number of the composition can be inferred directly fro...
we discuss the prospects of detecting the sources of ultra - high energy ( uhe ) cosmic ray ( cr ) nuclei via their emission of cosmogenic-rays in the gev to tev energy range . these-rays result from electromagnetic cascades initiated by high energy photons , electrons and positrons that are emitted by crs during their...
we discuss the prospects of detecting the sources of ultra - high energy ( uhe ) cosmic ray ( cr ) nuclei via their emission of cosmogenic-rays in the gev to tev energy range . these-rays result from electromagnetic cascades initiated by high energy photons , electrons and positrons that are emitted by crs during their...
1312.2687
i
gaussian process models are widely used in spatial statistics and machine learning . in most applications , the covariance structure of the process is at least partially unknown and must be estimated from the available data . likelihood - based methods , including bayesian methods , are natural choices for carrying out...
we discuss a modification of the stochastic approximation in which design elements of the stochastic terms mimic patterns from a factorial design . our findings are validated by numerical experiments on simulated data sets of up to 1 million observations . we apply the approach to fit a space time model to over 80,000...
we discuss the statistical properties of a recently introduced unbiased stochastic approximation to the score equations for maximum likelihood calculation for gaussian processes . under certain conditions , including bounded condition number of the covariance matrix , the approach achieves storage and nearly computatio...
1312.2687
r
[ secexp ] in this section we show a few experimental results based on a partially occluded regular grid . the rationale for using such a partial grid is to illustrate a setting where spectral techniques do not work so well but efficient matrix vector multiplications are available . a partially occluded grid can occur...
we discuss the statistical properties of a recently introduced unbiased stochastic approximation to the score equations for maximum likelihood calculation for gaussian processes . under certain conditions , including bounded condition number of the covariance matrix , the approach achieves storage and nearly computatio...
we discuss the statistical properties of a recently introduced unbiased stochastic approximation to the score equations for maximum likelihood calculation for gaussian processes . under certain conditions , including bounded condition number of the covariance matrix , the approach achieves storage and nearly computatio...
hep-ph0405303
i
elastic electron - nucleon scattering in the one - photon exchange approximation is a time - honoured tool to access information on the structure of hadrons . experiments with increasing precision have become possible in recent years , mainly triggered by new techniques to perform polarization experiments at the electr...
we express this imaginary part as a phase space integral over the doubly virtual compton scattering tensor on the nucleon . we use unitarity to model the doubly virtual compton scattering tensor in the resonance region in terms of electroabsorption amplitudes . taking those amplitudes from a phenomenological analysis o...
we discuss the target and beam normal spin asymmetries in elastic electron - nucleon scattering which depend on the imaginary part of two - photon exchange processes between electron and nucleon . we express this imaginary part as a phase space integral over the doubly virtual compton scattering tensor on the nucleon ....
1508.06037
i
primordial angular momentum is believed to decay with the expansion of the universe and the observed rotations of galaxies and clusters are believed to originate from tidal interactions with local environments ( the tidal torque theory ) or the acquisition of orbital angular momentum from infalling matter ( the merging...
we employ a stochastic approach to probing the origin of the log - normal distributions of halo spin in n - body simulations . after analyzing spin evolution in halo merging trees the roles of major merging and accretion are also statistically analyzed in evolving spin distributions . several factors ( local environmen...
we employ a stochastic approach to probing the origin of the log - normal distributions of halo spin in n - body simulations . after analyzing spin evolution in halo merging trees , it was found that a spin change can be characterized by a stochastic random walk of angular momentum . also , spin distributions generated...
hep-ph0302162
r
we present in this section the results of the analytic integration of eq.([eq : ref1 ] ) and eq.([eq : ref2 ] ) as a function of @xmath40 . as already said , @xmath15 is the small photon mass " used for the parameterization of the infrared divergences . all the polylogarithms depend on @xmath9 through the variable @xm...
11.55.fv , 12.20.ds , 13.40.gp ttp03 - 05 + 3.5 cm 1.cm p. mastrolia and e. remiddi 1.0 cm _ dipartimento di fisica , universit di bologna , i-40126 bologna , italy + 0.4 cm institut fr theoretische teilchenphysik , universitt karlsruhe , d-76128 karlsruhe , germany + 0.4 cm infn , sezione di bologna , i-40...
we evaluate the on shell form factors of the electron for arbitrary momentum transfer and finite electron mass , at two loops in qed , by integrating the corresponding dispersion relations , which involve the imaginary parts known since a long time . the infrared divergences are parameterized in terms of a fictitious s...
gr-qc9803061
i
since the discovery of black holes whose event horizons have nontrivial topology @xcite there has been much research activity in this area . charged versions of these black holes were presented in @xcite , and also rotating generalizations are known @xcite . moreover , they also exist in dilaton gravity @xcite . mann @...
first , massless scalar fields and weyl spinors which propagate in the background of an anti de sitter black hole are considered in an exactly soluble two dimensional toy model . the boulware , unruh , and hartle hawking vacua are defined . the latter results to coincide with the unruh vacuum due to the boundary con...
we examine quantum properties of topological black holes which are asymptotically anti de sitter . first , massless scalar fields and weyl spinors which propagate in the background of an anti de sitter black hole are considered in an exactly soluble two dimensional toy model . the boulware , unruh , and hartle hawk...
1003.2750
i
advances in experimental techniques have led to a great number of experimental studies on electron transport through molecular junctions formed by single molecules bridged between electrodes or molecular monolayers adsorbed onto surfaces , using three - terminal set - ups or scanning tunneling microscopy ( stm ) measur...
we analyze the effects of bonding type , molecular orientation , and geometry relaxation on the electronic properties and charge and spin transport across the single - molecule junction . we consider nine interface geometries leading to five bonding mechanisms and two molecular orientations : ( i ) au - c bonding , ( i...
we examine theoretically coherent electron transport through the single - molecule magnet mn , bridged between au(111 ) electrodes , using the non - equilibrium green s function method and the density - functional theory . we analyze the effects of bonding type , molecular orientation , and geometry relaxation on the e...
1003.2750
r
we examine the nine interface geometries ( fig . [ fig : geo ] ) leading to the five bonding types and two molecular orientations that were discussed in sec . i. their molecular orientations , linker groups , bonding types , binding sites , and distances @xmath19 between the electrodes are listed in table 1 . i...
relaxation of the junction geometries mainly shifts the relevant occupied molecular levels toward the fermi energy as well as slightly reduces the broadening of the lumo level . as a result , the current slightly decreases at low bias voltage . consequently , junctions with the former orientation yield a higher current...
we examine theoretically coherent electron transport through the single - molecule magnet mn , bridged between au(111 ) electrodes , using the non - equilibrium green s function method and the density - functional theory . we analyze the effects of bonding type , molecular orientation , and geometry relaxation on the e...
1003.2750
c
we simulated a single - molecule junction based on the smm mn@xmath0 connected to au(111 ) electrodes via five different bonding mechanisms and two molecular orientations , and calculated their transport properties , using the non - equilibrium green s function method and the spin - polarized dft . geometry relaxation ...
we examine theoretically coherent electron transport through the single - molecule magnet mn , bridged between au(111 ) electrodes , using the non - equilibrium green s function method and the density - functional theory . we find that the electron transport is carried by the lowest unoccupied molecular orbital ( lumo ...
we examine theoretically coherent electron transport through the single - molecule magnet mn , bridged between au(111 ) electrodes , using the non - equilibrium green s function method and the density - functional theory . we analyze the effects of bonding type , molecular orientation , and geometry relaxation on the e...
1612.00366
i
bose - einstein condensation ( bec ) occurs in a wide variety of systems@xcite . at a sufficient density , magnons condense into a single bose quantum state . spectroscopically generated magnon condensates have been observed in ferrimagnetic insulators at room temperature@xcite . these findings imply that it is feasibl...
we explore routes to realize electrically driven bose - einstein condensation of magnons in insulating antiferromagnets . even in insulating antiferromagnets , the localized spins can strongly couple to itinerant spins in adjacent metals via spin - transfer torque and spin pumping . bose - einstein condensation can occ...
we explore routes to realize electrically driven bose - einstein condensation of magnons in insulating antiferromagnets . even in insulating antiferromagnets , the localized spins can strongly couple to itinerant spins in adjacent metals via spin - transfer torque and spin pumping . we describe the formation of steady ...
astro-ph0611799
i
the impressive recent advances in the observational studies of high redshift galaxies and quasars have brought us up to the outskirts of ` dark ages ' , when the amount of neutral intergalactic hydrogen starts becoming significant and tentative indications of the presence of metal - free population iii stars begin to s...
( 2004 ) already successfully tested against the wealth of data on later evolutionary stages . complementing the model with a simple , physically plausible , recipe for the evolution of dust attenuation in metal poor galaxies we reproduce the luminosity functions ( lfs ) of lbgs and of laes at different redshifts .
we explore the onset of star formation in the early universe , exploiting the observations of high - redshift lyman - break galaxies ( lbgs ) and ly emitters ( laes ) , in the framework of the galaxy formation scenario elaborated by granato et al . ( 2004 ) already successfully tested against the wealth of data on late...
astro-ph0611799
c
we have extended to the earliest evolutionary phases of high redshift galaxies the physical model worked out by granato et al . ( 2004 ) which proved to be capable of accounting for the wealth of data on the heavily obscured active star formation phase probed by ( sub)mm surveys and on the subsequent passive evolution ...
these objects have therefore shorter lifetimes in the lae and lbg phases , and are more easily detected in the dusty submillimeter bright ( smb ) phase . are on the average expected to be younger , with lower stellar masses , more compact , and associated to less massive halos than lbgs .
we explore the onset of star formation in the early universe , exploiting the observations of high - redshift lyman - break galaxies ( lbgs ) and ly emitters ( laes ) , in the framework of the galaxy formation scenario elaborated by granato et al . ( 2004 ) already successfully tested against the wealth of data on late...
astro-ph0509407
m
gilliland , goudfrooij , and kimble ( 1999 ) proposed to increase the photometric accuracy of very high s / n observations by using the spectroscopic mode of stis . by distributing the star light along the dispersion direction it is possible to increase the total number of photons collected before the detector reaches ...
we explore the use of integral field spectroscopy ( ifs ) for observing extrasolar planet transits . second , this type of ifs data allows to _ autocalibrate _ instrumental and background effects . third , since the star image characteristics ( i.e. seeing , spatial shifts , etc . ) as well as its photometric properti...
we explore the use of integral field spectroscopy ( ifs ) for observing extrasolar planet transits . although this technique should find its full potential in space observations ( e.g. jwst , tpf ) , we have tested its basics with ground based time series observations of hd209458b obtained with wht + integral during a...
astro-ph0509407
c
the main conclusions of the present work can be summarized as follows : 1- we have shown that integral field spectroscopy is a powerful technique for obtaining accurate relative time series photometry and , therefore , of great potential for studying transits of extrasolar planets . the three main advantages with re...
although this technique should find its full potential in space observations ( e.g. jwst , tpf ) , we have tested its basics with ground based time series observations of hd209458b obtained with wht + integral during a transit in august 17/18 , 2004 . for this analysis we have found that ifs offers three fundamental a...
we explore the use of integral field spectroscopy ( ifs ) for observing extrasolar planet transits . although this technique should find its full potential in space observations ( e.g. jwst , tpf ) , we have tested its basics with ground based time series observations of hd209458b obtained with wht + integral during a...
1612.06320
i
recent progress on atomic and optical experiments has allowed to design and manipulate many - particle quantum systems at a remarkable level of control . a key benchmark for such experiments is the generation and unambiguous detection of quantum entanglement . entangled quantum states are further required as a key reso...
we formulate a general family of entanglement criteria for multipartite systems . generalized squeezing - type criteria provide lower bounds that are less stringent but only require measurements of second moments . the discussed techniques can be readily implemented in current experiments with trapped ions in paul trap...
we formulate a general family of entanglement criteria for multipartite systems . fisher information criteria compare the sensitivity to unitary rotations with the variances of suitable local observables . generalized squeezing - type criteria provide lower bounds that are less stringent but only require measurements o...
astro-ph0006399
i
blue straggler ( bs ) stars were first identified as an unusual subclass of stars in the cluster m3 @xcite . since that time , stragglers have been identified in most , if not all , globular clusters that have accurate broad - band photometry . blue straggler candidates have also been identified in a large number of op...
we have analyzed high - resolution spectra of relatively cool blue stragglers and main sequence turnoff stars in the old open cluster m67 ( ngc 2682 ) . we attempt to identify blue stragglers whose spectra are least contaminated by binary effects ( contamination by a binary companion or absorption by circumstellar mate...
we have analyzed high - resolution spectra of relatively cool blue stragglers and main sequence turnoff stars in the old open cluster m67 ( ngc 2682 ) . we attempt to identify blue stragglers whose spectra are least contaminated by binary effects ( contamination by a binary companion or absorption by circumstellar mate...
astro-ph0006399
c
our spectroscopic analysis of 4 relatively cool blue stragglers does not provide definitive evidence of composition modifications resulting from the formation process . based on lithium abundance patterns as a function of effective temperature for main sequence stars in the hyades and m67 , we find that current upper l...
these `` best '' stragglers have metallicities ( [ fe / h ] = 0.05 ) and abundance ratios of the blue stragglers are not significantly different from those of the turnoff stars . based on arguments from hydrodynamical models of stellar collisions , we assert that the current upper limits for the lithium abundances of a...
we have analyzed high - resolution spectra of relatively cool blue stragglers and main sequence turnoff stars in the old open cluster m67 ( ngc 2682 ) . we attempt to identify blue stragglers whose spectra are least contaminated by binary effects ( contamination by a binary companion or absorption by circumstellar mate...
astro-ph9711324
i
ngc 5548 is a bright , low - redshift ( z @xmath4 0.0172 ) seyfert 1 galaxy that has received a considerable amount of attention over the past decade . in particular , ngc 5548 has been the subject of a number of intensive spectroscopic monitoring campaigns in the optical and uv ( korista et al . these efforts have yie...
all of the spectra were obtained when the broad emission line and continuum fluxes were at an historic low level , allowing us to accurately determine the contribution of the narrow - line region ( nlr ) to the emission lines . we show that the outer component may contain dust , which further reduces the mg ii flux by ...
we have combined _ hst_/fos and ground - based spectra of the seyfert 1 galaxy ngc 5548 to study the narrow emission lines over the 1200 10,000 region . all of the spectra were obtained when the broad emission line and continuum fluxes were at an historic low level , allowing us to accurately determine the contri...
astro-ph9711324
c
we have analyzed uv and optical spectra of the seyfert 1 galaxy ngc 5548 that were obtained when it was at an historical minimum . we were able to isolate the narrow emission line components ( which do not vary in flux on short time scales ) , due to the relative weakness of the more rapidly variable broad emission lin...
we have combined _ hst_/fos and ground - based spectra of the seyfert 1 galaxy ngc 5548 to study the narrow emission lines over the 1200 10,000 region . we show that the majority of the emission in the nlr of ngc 5548 must arise within about pc from the nucleus .
we have combined _ hst_/fos and ground - based spectra of the seyfert 1 galaxy ngc 5548 to study the narrow emission lines over the 1200 10,000 region . all of the spectra were obtained when the broad emission line and continuum fluxes were at an historic low level , allowing us to accurately determine the contri...
astro-ph0010526
i
the distance to the large magellanic cloud ( lmc ) is a key factor in determining the size scale of the universe . indeed , the uncertainty in the length of this `` cosmic meter stick '' is responsible for much of the current uncertainty in the value of the hubble constant , as noted by mould et al . the lmc distance i...
we have determined the distance to a second eclipsing binary system ( eb ) in the large magellanic cloud , hv 982 (b1 iv - v +b1 iv - v ) . this distance determination consists of a detailed study of well - understood objects ( b stars ) in a well - understood evolutionary phase ( core h burning ) . the results are en...
we have determined the distance to a second eclipsing binary system ( eb ) in the large magellanic cloud , hv 982 (b1 iv - v +b1 iv - v ) . the measurement of the distance among other properties of the system is based on optical photometry and spectroscopy and space - based uv / optical spectrophotometry . the analy...
astro-ph0301296
i
this is the fourth in a series of papers presenting results from detailed analyses of b - type eclipsing binary ( eb ) systems in the large magellanic cloud ( lmc ) . our primary scientific goals are : 1 ) to determine an essentially complete description of the stellar properties of each system , thus providing tests a...
we have determined the fundamental properties and distance of a fourth eclipsing binary system ( eb ) in the large magellanic cloud , hv 5936 (b0.5 v +b2 iii ) . as in our previous studies , the distance derived to the system , kpc , implies a distance of.3 to the optical center of the lmc .
we have determined the fundamental properties and distance of a fourth eclipsing binary system ( eb ) in the large magellanic cloud , hv 5936 (b0.5 v +b2 iii ) . as in our previous studies , we combine `` classical '' eb light curve and radial velocity curve analyses with modeling of the uv - through - optical spectra...
1201.2761
i
we have made an extensive survey of emission - line stars in the ic 1396 h ii region to investigate the low - mass pms population near the ob stars . a total of 639 h@xmath0 stars were detected over a 4-deg@xmath1 area and their @xmath2-photometry was performed . their spatial distribution shows several aggregates near...
we have made an extensive survey of emission - line stars in the ic 1396 h ii region to investigate the low - mass population of pre - main sequence ( pms ) stars . a total of 639 h emission - line stars were detected in an area of 4.2 deg and their-photometry was measured . their spatial distribution exhibits several ...
we have made an extensive survey of emission - line stars in the ic 1396 h ii region to investigate the low - mass population of pre - main sequence ( pms ) stars . a total of 639 h emission - line stars were detected in an area of 4.2 deg and their-photometry was measured . their spatial distribution exhibits several ...
1601.03053
i
we have spectroscopically observed a sample of 10 white dwarf candidates in the young and rich ngc 2323 . while we only found that two of these white dwarfs are consistent with membership in ngc 2323 , they are both newly discovered high - mass white dwarfs at @xmath01.07 m@xmath1 . to supplement these new white dwarfs...
we have observed a sample of 10 white dwarf candidates in the rich open cluster ngc 2323 ( m50 ) with the keck low - resolution imaging spectrometer . / n appropriate for our analysis . two of these white dwarfs are consistent with singly evolved cluster membership , and both are high mass.07 m , and give equivalent pr...
we have observed a sample of 10 white dwarf candidates in the rich open cluster ngc 2323 ( m50 ) with the keck low - resolution imaging spectrometer . the spectroscopy shows eight to be da white dwarfs , with six of these having high s / n appropriate for our analysis . two of these white dwarfs are consistent with sin...
astro-ph9702147
i
astronomers have sought for two decades for dynamical evidence for the presence of massive black holes in galaxies by studying the dynamics of gas and stars in their nuclei . rapid motions provide the main signature of a black hole . if these are indeed observed , the main difficulty is to rule out alternative interpre...
we have obtained spectra through small apertures centered on the nuclear region and major axis of m32 , with the faint object spectrograph ( fos ) on the hubble space telescope ( hst ) . a detailed analysis and reduction of the data these results significantly strengthen previous arguments for the presence of a massive...
we have obtained spectra through small apertures centered on the nuclear region and major axis of m32 , with the faint object spectrograph ( fos ) on the hubble space telescope ( hst ) . a detailed analysis and reduction of the data is presented , including : ( i ) new calibrations and modeling of the fos aperture size...
astro-ph9702147
c
hst / fos spectra were obtained through small apertures centered on the nuclear region and major axis of m32 . kinematical analysis of these data is more complicated than it is for ground - based data : the fos is a low - resolution spectrograph , and is not particularly well suited for dynamical studies of low - dispe...
is presented , including : ( i ) new calibrations and modeling of the fos aperture sizes , point - spread - function and line - spread - functions ; ( ii ) determination of the aperture positioning for each observation from the observed count rate ; and ( iii ) accurate wavelength calibration , template matching , and ...
we have obtained spectra through small apertures centered on the nuclear region and major axis of m32 , with the faint object spectrograph ( fos ) on the hubble space telescope ( hst ) . a detailed analysis and reduction of the data is presented , including : ( i ) new calibrations and modeling of the fos aperture size...
astro-ph0403462
r
using the above criteria for detecting a residual host galaxy , we find nine of the 23 host galaxies to be resolved in both bands , although some lie close to the sensitivity limit . one object formally fell above the 5% level in one band but not the other ; combo-17 33630 at @xmath64 might be marginally resolved in f...
the data are part of the gems imaging survey that provides high resolution optical images obtained with the advanced camera for surveys in two bands ( f606w and f850lp ) , sampling the rest - frame uv flux of the targets . to deblend the agn images into nuclear and resolved ( host galaxy ) components we use a psf sub...
we have performed _ hst _ imaging of a sample of 23 high - redshift ( ) active galactic nuclei , drawn from the combo-17survey . the sample contains moderately luminous quasars ( ) . the data are part of the gems imaging survey that provides high resolution optical images obtained with the advanced camera for surveys...
astro-ph0403462
c
from the corrected magnitudes we have derived @xmath92 colours for the detected host galaxies . these are listed in table [ tab : colours ] , now including also correction for galactic dust extinction . however , with @xmath93 @xcite these values of @xmath94 and @xmath95 negligibly affect the colours . at these red...
the rest - frame absolute magnitudes at 200 nm are . we find that the uv colors of all host galaxies are substantially bluer than expected from an old population of stars with formation redshift , independent of the assumed metallicities . these uv colours and luminosities range up to the values found for lyman - brea...
we have performed _ hst _ imaging of a sample of 23 high - redshift ( ) active galactic nuclei , drawn from the combo-17survey . the sample contains moderately luminous quasars ( ) . the data are part of the gems imaging survey that provides high resolution optical images obtained with the advanced camera for surveys...
astro-ph0403462
c
we performed the hitherto largest study of host galaxies properties of a complete sample of high - redshift agn . we detected the hosts and extract colour information in 9 of the 23 agn , and we also achieved a statistical detection of the host in the remaining 14 from a stack analysis . the uv luminosities can be inte...
we have performed _ hst _ imaging of a sample of 23 high - redshift ( ) active galactic nuclei , drawn from the combo-17survey . our results suggest either a recent starburst , of e.g. a few per cent of the total stellar mass and 100 myrs before observation , with mass - fraction and age strongly degenerate , or the...
we have performed _ hst _ imaging of a sample of 23 high - redshift ( ) active galactic nuclei , drawn from the combo-17survey . the sample contains moderately luminous quasars ( ) . the data are part of the gems imaging survey that provides high resolution optical images obtained with the advanced camera for surveys...
1408.0224
r
in this paper , we have derived the behavior of the accretion flows in a range of direct - impact and disk - state algol binaries with orbital periods from 1.2 to 11.1 days . these systems undergo mass transfer from a magnetically - active star onto a normal , non - magnetic main sequence star . we have applied the tec...
we have used 2d back - projection doppler tomography as a tool to examine the influence of gravitational and magnetic phenomena in interacting binaries which undergo mass transfer from a magnetically - active star onto a non - magnetic main sequence star . this multi - tiered study of over 1300 time - resolved spectra ...
we have used 2d back - projection doppler tomography as a tool to examine the influence of gravitational and magnetic phenomena in interacting binaries which undergo mass transfer from a magnetically - active star onto a non - magnetic main sequence star . this multi - tiered study of over 1300 time - resolved spectra ...
1408.0224
c
the multi - tiered analysis performed in this work involved both theoretical tools and spectroscopic observations of algol binaries from the stream state to the disk state . this analysis has provided observational evidence of the effects of gravitational forces on the accretion flows in these interacting binaries . mo...
the tomography images have revealed results that can not be explained solely by gravitational effects : chromospheric emission moving with the mass - losing star , a gas stream deflected from the gravitational trajectory , and alternating behavior between stream state and disk state . our results demonstrate that magne...
we have used 2d back - projection doppler tomography as a tool to examine the influence of gravitational and magnetic phenomena in interacting binaries which undergo mass transfer from a magnetically - active star onto a non - magnetic main sequence star . this multi - tiered study of over 1300 time - resolved spectra ...
1702.06822
c
in this paper we have performed a detailed investigation of different types of mean - field - like approximations for stochastic dynamics on graphs , within the unifying framework of a cluster - variational approach . in analogy with its equilibrium counterpart , this approach naturally opens the way to improving the a...
we investigate different mean - field - like approximations for stochastic dynamics on graphs , within the framework of a cluster - variational approach . in analogy with its equilibrium counterpart , this approach allows one to give a unified view of various ( previously known ) approximation schemes , and suggests qu...
we investigate different mean - field - like approximations for stochastic dynamics on graphs , within the framework of a cluster - variational approach . in analogy with its equilibrium counterpart , this approach allows one to give a unified view of various ( previously known ) approximation schemes , and suggests qu...
1007.0003
c
we have shown that the lack of host galaxy detections in coincidence with the bursts in _ sample 2 _ indicates either a high redshift ( @xmath12 ) origin , or substantial projected offsets of @xmath192 kpc ( @xmath193 @xmath181 ) . both scenarios can account for the lack of underlying galaxy detections and the fainter ...
the large offset scenario leads to an offset distribution that is well - matched by theoretical predictions of ns - ns / ns - bh binary kicks , or by a hybrid population with globular cluster ns - ns binaries at large offsets and primordial binaries at offsets of kpc ( indicative of negligible kicks ) .
we investigate the afterglow properties and large - scale environments of several short - duration gamma - ray bursts ( grbs ) with sub - arcsecond optical afterglow positions but no bright coincident host galaxies . the purpose of this joint study is to robustly assess the possibility of significant offsets , a hallma...
1007.0003
c
we undertook the first systematic study of short grbs with detected optical afterglows ( and hence sub - arcsecond position ) but no coincident host galaxies to limits of @xmath148 mag . we find that the optical afterglows of these bursts are fainter by about 1.4 mag compared to the optical afterglows of short grbs wit...
we investigate the afterglow properties and large - scale environments of several short - duration gamma - ray bursts ( grbs ) with sub - arcsecond optical afterglow positions but no bright coincident host galaxies . the high redshift scenario leads to a bimodal redshift distribution , with peaks at and .
we investigate the afterglow properties and large - scale environments of several short - duration gamma - ray bursts ( grbs ) with sub - arcsecond optical afterglow positions but no bright coincident host galaxies . the purpose of this joint study is to robustly assess the possibility of significant offsets , a hallma...
astro-ph0005543
i
in this section we analyse the cmb temperature and polarization spectra of our teq model . in fig.[f4 ] we plot the cmb spectra for the models discussed in the previous section ; the top panel describes temperature fluctuations ; the bottom panel shows polarization spectra . the cmb spectrum coefficients are calcula...
we give accurate analytic formulas describing the-boost , showing that the quintessence energy in this phase scales with the redshift as . similarly , the cmb acoustic peaks multipoles shift compared to ordinary tracking quintessence models by roughly an amount/8 $ ] . the turnover wavenumber in the matter power spectr...
we investigate the cosmological role of a tracking field in extended quintessence scenarios , where the dynamical vacuum energy driving the acceleration of the universe today possesses an explicit coupling with the ricci scalar , , of the form , where mimics general relativity today , . we analyse explicit non - minima...
astro-ph0005543
c
in this section we will make a self consistent summary of the results obtained in this paper , focusing on the observable features of the cosmological models here investigated . the present paper is devoted to the study of theoretical aspects and observational imprints of cosmological scenarios in which a dynamical vac...
we investigate the cosmological role of a tracking field in extended quintessence scenarios , where the dynamical vacuum energy driving the acceleration of the universe today possesses an explicit coupling with the ricci scalar , , of the form , where mimics general relativity today , . when the-boost ends , the field ...
we investigate the cosmological role of a tracking field in extended quintessence scenarios , where the dynamical vacuum energy driving the acceleration of the universe today possesses an explicit coupling with the ricci scalar , , of the form , where mimics general relativity today , . we analyse explicit non - minima...
0812.4223
i
the large hadron collider ( lhc ) will soon test the mechanism of spontaneous electroweak symmetry breaking . it is widely agreed that this phenomenon is associated to the expectation value of a scalar field which transforms as a doublet with respect to the weak su(2)-symmetry . the origin and status of this order para...
we investigate the fermions of the standard model without a higgs scalar . instead , we consider a non - local four - quark interaction in the tensor channel which is characterized by a single dimensionless coupling . the running of is asymptotically free and therefore induces a non - perturbative scale , in analogy to...
we investigate the fermions of the standard model without a higgs scalar . instead , we consider a non - local four - quark interaction in the tensor channel which is characterized by a single dimensionless coupling . quantization leads to a consistent perturbative expansion for small . the running of is asymptotically...
1401.1212
i
at first glance , star formation appears to be a localised process . the coldest gas in the galactic interstellar medium ( ism ) clumps into turbulent aggregations known as the giant molecular clouds ( gmcs ) . these stellar nurseries are on average , three orders of magnitude smaller than the galactic radii and the po...
we investigate the impact of galactic environment on the properties of simulated giant molecular clouds ( gmcs ) formed in a m83-type barred spiral galaxy . the bar clouds also show a bimodality that is not reflected in the spiral and disc clouds except in the surface density , where all three regions show two distinct...
we investigate the impact of galactic environment on the properties of simulated giant molecular clouds ( gmcs ) formed in a m83-type barred spiral galaxy . our simulation uses a rotating stellar potential to create the grand design features and resolves down to 1.5pc . from the comparison of clouds found in the bar , ...
1401.1212
r
in the initial stages of the simulation , the gas profile is smoothly exponential as described in section [ sec : numerics_disc ] . as the simulation begins and the gas feels the impact of the stellar potential , two shock waves are formed at the point of co - rotation between the stellar potential s pattern speed and...
however , the fraction of clouds in the property distribution tails varies between regions , with larger , more massive clouds with a higher velocity dispersion being found in greatest proportions in the bar , spiral and then disc . we identify these features as being due to the relative proportion of three cloud types...
we investigate the impact of galactic environment on the properties of simulated giant molecular clouds ( gmcs ) formed in a m83-type barred spiral galaxy . our simulation uses a rotating stellar potential to create the grand design features and resolves down to 1.5pc . from the comparison of clouds found in the bar , ...
1401.1212
c
we performed three - dimensional hydrodynamical simulations of a barred spiral galaxy down to a limiting resolution of 1.5pc and compared the properties of the gmcs forming in the bar , spiral and disc environments . our main results are as follows : 1 . the typical ( peak ) value of the cloud properties such as mas...
our simulation uses a rotating stellar potential to create the grand design features and resolves down to 1.5pc . from the comparison of clouds found in the bar , spiral and disc regions , we find that the typical gmc is environment independent , with a mass ofm and radius 11pc . type b _ clouds are massive giant molec...
we investigate the impact of galactic environment on the properties of simulated giant molecular clouds ( gmcs ) formed in a m83-type barred spiral galaxy . our simulation uses a rotating stellar potential to create the grand design features and resolves down to 1.5pc . from the comparison of clouds found in the bar , ...
0801.2428
m
the solutions presented in this paper are based on the formulation detailed in sw03 and sw05 . only a brief summary is given here . we write the equations of non - ideal mhd about a local keplerian frame that corotates with the disc at the keplerian frequency @xmath38 and express the velocity field as a departure from ...
solutions are obtained at representative radial locations ( and au ) from the central protostar for a minimum - mass solar nebula model and different choices of the initial magnetic field strength , configuration of the diffusivity tensor and grain sizes . in fact , mri perturbations grow at au ( 10 au ) for mg ( 13...
we investigate the linear growth and vertical structure of the magnetorotational instability ( mri ) in weakly ionised , stratified protoplanetary discs . the magnetic field is initially vertical and dust grains are assumed to be well mixed with the gas over the entire vertical dimension of the disc . for simplicity , ...
0801.2428
i
we have explored in this paper the linear growth and vertical structure of mri unstable modes at two representative radii ( @xmath3 and 10 au ) in protoplanetary discs . dust grains are assumed to be well mixed with the fluid over the entire section of the disc and , for simplicity , are taken to have the same radius (...
we investigate the linear growth and vertical structure of the magnetorotational instability ( mri ) in weakly ionised , stratified protoplanetary discs . the magnetic field is initially vertical and dust grains are assumed to be well mixed with the gas over the entire vertical dimension of the disc . for simplicity , ...
we investigate the linear growth and vertical structure of the magnetorotational instability ( mri ) in weakly ionised , stratified protoplanetary discs . the magnetic field is initially vertical and dust grains are assumed to be well mixed with the gas over the entire vertical dimension of the disc . for simplicity , ...
1207.1676
i
the @xmath2 is the only heavy meson consisting of two heavy quarks with different flavors , hence the decay properties of this meson are of special interest . the difference in heavy quark flavors forbids annihilation of this meson into gluons , so the excited @xmath2 states undergo pionic or radiative transition to th...
we investigate the radiative transition in the framework of qcd sum rules . in particular , we calculate the transition form factors responsible for this decay in both weak annihilation and electromagnetic penguin channels using the quark condensate , mixed and two - gluon condensate diagrams as well as propagation of ...
we investigate the radiative transition in the framework of qcd sum rules . in particular , we calculate the transition form factors responsible for this decay in both weak annihilation and electromagnetic penguin channels using the quark condensate , mixed and two - gluon condensate diagrams as well as propagation of ...
1012.0973
i
graphene is considered to be a promising candidate for the spintronic applications recently,@xcite partly due to the perfect two dimensionality , gate - voltage - tunable charge carrier type and density,@xcite high mobility@xcite as well as the potentially long spin relaxation time limited by the small intrinsic spin -...
we investigate the spin diffusion and transport in a graphene monolayer on sio substrate by means of the microscopic kinetic spin bloch equation approach . the substrate causes a strong rashba spin - orbit coupling field mev , which might be accounted for by the impurities initially present in the substrate or even th...
we investigate the spin diffusion and transport in a graphene monolayer on sio substrate by means of the microscopic kinetic spin bloch equation approach . the substrate causes a strong rashba spin - orbit coupling field mev , which might be accounted for by the impurities initially present in the substrate or even th...
1012.0973
c
in conclusion , we have investigated the spin diffusion and transport in graphene monolayer on sio@xmath0 substrate as presented by pi _ et al._,@xcite by means of the ksbe approach . the substrate ( including the impurities initially present ) contributes a rashba spin - orbit coupling field much stronger than the one...
lett . * 104 * , 187201 ( 2010 ) ] , the rashba spin - orbit coupling coefficient is found to increase approximately linearly from 0.15 to 0.23 mev with the increase of au density . with this strong spin - orbit coupling , this anisotropy differs from the one given by the two - component drift - diffusion model , whic...
we investigate the spin diffusion and transport in a graphene monolayer on sio substrate by means of the microscopic kinetic spin bloch equation approach . the substrate causes a strong rashba spin - orbit coupling field mev , which might be accounted for by the impurities initially present in the substrate or even th...
cond-mat0505511
i
with the advent of mesoscopic physics , it has become possible to experimentally investigate quantum phase coherent properties of electrons in solid state conductors in a controlled way . in particular , in ballistic mesoscopic samples at low temperatures , electrons can propagate up to several microns without loosing ...
we investigate the visibility of the current and shot - noise correlations of electrical analogs of the optical mach - zehnder interferometer and the hanbury brown twiss interferometer . the electrical analogs are discussed in conductors subject to high magnetic fields where electron motion is along edge states . the t...
we investigate the visibility of the current and shot - noise correlations of electrical analogs of the optical mach - zehnder interferometer and the hanbury brown twiss interferometer . the electrical analogs are discussed in conductors subject to high magnetic fields where electron motion is along edge states . the t...
cond-mat0505511
c
the mz - interferometer is an amplitude interferometer : it exhibits a visibility in the average current with period @xmath0 and exhibits a visibility in the shot noise with periods of both @xmath0 and @xmath1 . in contrast , the hbt interferometer is an intensity interferometer , it exhibits no ab - effect in the curr...
a direct comparison is only possible for the shot noise of the two interferometers . we find that the visibility of shot noise correlations of the hanbury brown twiss interferometer as function of temperature , voltage or dephasing , is qualitatively similar to the visibility of the first harmonic of the shot noise cor...
we investigate the visibility of the current and shot - noise correlations of electrical analogs of the optical mach - zehnder interferometer and the hanbury brown twiss interferometer . the electrical analogs are discussed in conductors subject to high magnetic fields where electron motion is along edge states . the t...
hep-th0703271
i
in this paper we have studied stability of the 6d braneworld solution with 4d de sitter branes from two different perspectives . one is thermodynamic stability of the braneworld solution . we have defined the de sitter entropy in the six - dimensional braneworld by one quarter of the area of the cosmological horizon...
we investigate thermodynamic and dynamical stability of a family of six - dimensional braneworld solutions with de sitter branes . we see that the family of solutions is divided into two distinct branches : the high - entropy branch and the low - entropy branch . by analogy with ordinary thermodynamics , it is found th...
we investigate thermodynamic and dynamical stability of a family of six - dimensional braneworld solutions with de sitter branes . first , we investigate thermodynamic stability in terms of de sitter entropy . we see that the family of solutions is divided into two distinct branches : the high - entropy branch and the ...
quant-ph0611151
c
a fundamental question in quantum key distribution ( qkd ) is to determine whether the legitimate users of the system can use their available measurement results to generate a secret key via two - way or one - way classical post - processing of the observed data . in this paper we have investigated single - photon qkd ...
we investigate two - way and one - way single - photon quantum key distribution ( qkd ) protocols in the presence of loss introduced by the quantum channel . our analysis is based on a simple precondition for secure qkd in each case . in particular , the legitimate users need to prove that there exists no separable sta...
we investigate two - way and one - way single - photon quantum key distribution ( qkd ) protocols in the presence of loss introduced by the quantum channel . our analysis is based on a simple precondition for secure qkd in each case . in particular , the legitimate users need to prove that there exists no separable sta...
0712.3371
i
the dirichlet laplacian in tubular domains is a simple but remarkably successful model for the quantum hamiltonian in mesoscopic waveguide systems . one of the main questions arising within the scope of electronic transport is whether or not there are geometrically induced bound states . indeed , some of the most impor...
we make an overview of spectral - geometric effects of twisting and bending in quantum waveguides modelled by the dirichlet laplacian in an unbounded three - dimensional tube of uniform cross - section . we focus on the existence of hardy - type inequalities in twisted tubes of non - circular cross - section .
we make an overview of spectral - geometric effects of twisting and bending in quantum waveguides modelled by the dirichlet laplacian in an unbounded three - dimensional tube of uniform cross - section . we focus on the existence of hardy - type inequalities in twisted tubes of non - circular cross - section .
astro-ph0211460
i
in two previous papers , we developed a model of thermal comptonization and disk thermal reprocessing to explain the data from recent multiwavelength monitoring observations of the type 1 seyfert galaxies ngc 3516 and ngc 7469 ( chiang & blaes 2001 , hereafter paper i ; chiang 2002 , hereafter paper ii ) . the esse...
we model the spectral energy distribution of the type 1 seyfert galaxy ngc 5548 , fitting data from simultaneous optical , uv , and x - ray monitoring observations . we assume a geometry consisting of a hot central comptonizing region surrounded by a thin accretion disk . the constraints imposed upon this model by the ...
we model the spectral energy distribution of the type 1 seyfert galaxy ngc 5548 , fitting data from simultaneous optical , uv , and x - ray monitoring observations . we assume a geometry consisting of a hot central comptonizing region surrounded by a thin accretion disk . the properties of the disk and the hot central ...
1102.2076
i
soft gamma - ray repeaters ( sgrs ) and anomalous x - ray pulsars ( axps ) are believed to be young neutron stars with strong magnetic fields ( @xmath7 ) . they are categorized as magnetars ( see , e.g. , @xcite ; , for review ) . their rotation period @xmath8 and its time derivative @xmath9 are @xmath10 and @xmath11 ,...
they are divided by two discontinuities . we also carried out magnetohydrodynamic ( mhd ) simulations of the evolution of magnetic loops to study the stability and the generality of our analytical solutions . [ firstpage ] relativity - stars : magnetic fields - stars : neutron - stars : flare
we obtained self - similar solutions of relativistically expanding magnetic loops by assuming axisymmetry and a purely radial flow . the stellar rotation and the magnetic fields in the ambient plasma are neglected . we include the newtonian gravity of the central star . these solutions are extended from those in our pr...
quant-ph0312071
i
when john bell , then a theoretical physicist at cern , published his now famous theorem in 1964 , it was at first hardly noticed by the scientific community . only within the subsequent decade the fundamental character of its content was truly appreciated @xcite : in a sense , it fleshed out the notion of entangled qu...
we outline the basic questions that are being studied in the theory of entanglement . following a brief review of some of the main achievements of entanglement theory for finite - dimensional quantum systems such as qubits , we will consider entanglement in infinite - dimensional systems . results of this theory are pr...
we outline the basic questions that are being studied in the theory of entanglement . following a brief review of some of the main achievements of entanglement theory for finite - dimensional quantum systems such as qubits , we will consider entanglement in infinite - dimensional systems . asking for a theory of entang...
0805.3115
i
exclusive electron scattering from the deuteron target is very interesting by itself , and also as a very relevant stepping stone towards understanding exclusive electron scattering from heavier nuclei . the @xmath0 reaction at gev energies allows us - and requires us - to carefully study the reaction mechanism . it is...
we perform a fully relativistic calculation of the reaction in the impulse approximation . we employ the gross equation to describe the deuteron ground state , and we use the said parametrization of the full nn scattering amplitude to describe the final state interactions ( fsis ) . we include both on - shell and posit...
we perform a fully relativistic calculation of the reaction in the impulse approximation . we employ the gross equation to describe the deuteron ground state , and we use the said parametrization of the full nn scattering amplitude to describe the final state interactions ( fsis ) . we include both on - shell and posit...
astro-ph9804069
c
we have numerically investigated structural and kinematical properties of remnants of galaxy mergers between late - type spirals considerably abundant in interstellar gas in order to explore the origin of the fundamental plane ( fp ) of elliptical galaxies . we particularly considered that the origin of the slope of th...
we perform numerical simulations of galaxy mergers between star - forming and gas - rich spirals in order to explore the origin of the fundamental plane ( fp ) of elliptical galaxies . we consider particularly that the origin of the slope of the fp is essentially due to the non - homology in structure and kinematics of...
we perform numerical simulations of galaxy mergers between star - forming and gas - rich spirals in order to explore the origin of the fundamental plane ( fp ) of elliptical galaxies . we consider particularly that the origin of the slope of the fp is essentially due to the non - homology in structure and kinematics of...
astro-ph0205436
c
in this paper we have demonstrated the following benefits of sampling methods for cosmological parameter estimation : * the practicality of exploring the full shape of high - dimensional posterior parameter distributions using mcmc . * the use of principle component analysis to identify well constrained non - linear...
the monte carlo method allows the rapid investigation of a large number of parameters , and we present results from 6 and 9 parameter analyses of flat models , and an 11 parameter analysis of non - flat models . our results include constraints on the neutrino mass ( ) , equation of state of the dark energy , and the te...
we present a fast markov chain monte - carlo exploration of cosmological parameter space . we perform a joint analysis of results from recent cmb experiments and provide parameter constraints , including , from the cmb independent of other data . we next combine data from the cmb , hst key project , 2df galaxy redshift...
1602.07590
i
a long standing problem in astrophysics is a result of our inability to determine the three - dimensional structure of distant objects . this limitation has often inhibited our understanding of the internal structure of even relatively well defined and isolated astronomical objects , such as molecular cloud cores . a...
. such profiles are often critical to understand the physics and chemistry of molecular cloud cores , in which star formation takes place . instead it exploits contour self - similarity in column density maps which appears to be common in data for astronomical objects . we derive the method analytically , test it numer...
we present a geometry - independent method for determining the shapes of radial volume density profiles of astronomical objects whose geometries are unknown , based on a single column density map . such profiles are often critical to understand the physics and chemistry of molecular cloud cores , in which star formatio...
1602.07590
c
this paper has presented a novel new method for determining the forms of the radial volume density profiles of objects such as molecular cloud cores without making assumptions about their geometry . while the method has been applied here only to dust extinction maps of molecular clouds , it is highly generalized and ma...
we present a geometry - independent method for determining the shapes of radial volume density profiles of astronomical objects whose geometries are unknown , based on a single column density map our method may be applied to many types of astronomical objects and observable quantities so long as they satisfy a limited ...
we present a geometry - independent method for determining the shapes of radial volume density profiles of astronomical objects whose geometries are unknown , based on a single column density map . such profiles are often critical to understand the physics and chemistry of molecular cloud cores , in which star formatio...
hep-th0611305
i
gauge theories in a slice of anti - de sitter ( ads ) space have attracted a great deal of attention in recent years primarily because they provide geometrical explanations of particle physics mysteries , including the gauge hierarchy problem @xcite , and a window into strongly coupled gauge theories via the ads / cft ...
we show that the symmetry can be restored at the nonlinear level by considering brane - localized interactions , which are added in a gauge invariant way using boundary kinetic terms . finally , we show how to localize the scalar component zero mode anywhere in the bulk which could be relevant in gauge - higgs unificat...
we present a mechanism to localize zero mode non - abelian gauge fields in a slice of ads . as in the u(1 ) case , bulk and boundary mass terms allow for a massless mode with an exponential profile that can be localized anywhere in the bulk . however in the non - abelian extension , the cubic and quartic zero mode gaug...
hep-th0611305
c
zero mode gauge fields in a compact extra dimension can be localized through the addition of bulk and brane mass terms . the inclusion of these terms modifies the bulk equation of motion and the boundary conditions such that a zero mode with an exponential wavefunction exists in the theory . in the non - abelian case ,...
we present a mechanism to localize zero mode non - abelian gauge fields in a slice of ads . as in the u(1 ) case , bulk and boundary mass terms allow for a massless mode with an exponential profile that can be localized anywhere in the bulk . however in the non - abelian extension , the cubic and quartic zero mode gaug...
we present a mechanism to localize zero mode non - abelian gauge fields in a slice of ads . as in the u(1 ) case , bulk and boundary mass terms allow for a massless mode with an exponential profile that can be localized anywhere in the bulk . however in the non - abelian extension , the cubic and quartic zero mode gaug...
0706.2394
i
currently accepted microscopic theories for superconductivity in a magnetic field include the microscopic derivation of the meissner effect in the bcs theory@xcite and the microscopic derivation of the phenomenological ginzburg - landau equations by gorkov@xcite from the bcs theory . however , the bcs derivation of the...
we expect the theory to be valid for highly - local superconductors for all temperatures and magnetic fields below the superconducting transition . in the low - field limit , the theory reduces to the local - limit result of bcs . as examples , we apply the theory to the case of a semi - infinite superconductor in an a...
we present a microscopic theory for superconductivity in a magnetic field based on a local approximation approach . we derive an expression for free energy density as a function of temperature and vector potential * a * , and two basic equations of the theory : the first is an implicit solution for energy gap parameter...
0706.2394
i
we have presented a microscopic theory for superconductivity in a magnetic field based on a local approximation approach . the theory allows microscopic description of the suppression of superconductivity by an externally applied magnetic field . in sec . [ sectheory ] , we presented the details of the theory . the ...
we present a microscopic theory for superconductivity in a magnetic field based on a local approximation approach . we derive an expression for free energy density as a function of temperature and vector potential * a * , and two basic equations of the theory : the first is an implicit solution for energy gap parameter...
we present a microscopic theory for superconductivity in a magnetic field based on a local approximation approach . we derive an expression for free energy density as a function of temperature and vector potential * a * , and two basic equations of the theory : the first is an implicit solution for energy gap parameter...
astro-ph9712108
i
standard big bang nucleosynthesis ( sbbn ; @xcite ; @xcite ; @xcite ; @xcite ; @xcite ) predicts that a measurement of the primordial ratio d / h will give the most sensitive constraint on the cosmological baryon to photon ratio , @xmath11 . using the photon density measured from the temperature of the cosmic microwav...
we present a new measurement of the deuterium - to - hydrogen ratio ( d / h ) in the lyman limit absorption system at towards q19371009 . now we present a new method to measure d / h in qso absorption systems . both this and previous analyses find contamination to be unlikely in this absorption system , a analysis in m...
we present a new measurement of the deuterium - to - hydrogen ratio ( d / h ) in the lyman limit absorption system at towards q19371009 . tytler , fan & burles ( 1996 ; hereafter tfb ) made the first extragalactic detection of deuterium in this absorption system , which remains the best location for a high accuracy mea...
1210.6841
i
supernova explosion is one of the most spectacular events in the universe . it is not only the death of massive stars but also an engine for the evolution of the galaxies . apart from the classification according to the spectroscopy , it is thought that there are two mechanisms of the explosion . while type ia supernov...
we present a new series of supernova neutrino light curves and spectra calculated by numerical simulations for a variety of progenitor stellar masses ( 13- ) and metallicities ( and 0.004 ) , which would be useful for a broad range of supernova neutrino studies , e.g. , simulations of future neutrino burst detection by...
we present a new series of supernova neutrino light curves and spectra calculated by numerical simulations for a variety of progenitor stellar masses ( 13- ) and metallicities ( and 0.004 ) , which would be useful for a broad range of supernova neutrino studies , e.g. , simulations of future neutrino burst detection by...
1606.00813
i
most standard graphical models are restricted to pairwise dependencies between variables . for example , the ising model for binary data and the multivariate gaussian for real - valued data are popular pairwise graphical models . however , real - world data often exhibits triple - wise , or more generally @xmath0-wise ...
we present a novel-way high - dimensional graphical model called the generalized root model ( grm ) that explicitly models dependencies between variable sets of sizewhere is the standard pairwise graphical model . this model is based on taking the-th root of the original sufficient statistics of any univariate exponent...
we present a novel-way high - dimensional graphical model called the generalized root model ( grm ) that explicitly models dependencies between variable sets of sizewhere is the standard pairwise graphical model . this model is based on taking the-th root of the original sufficient statistics of any univariate exponent...
gr-qc0401076
i
since many of the most interesting phenomena in astrophysics involve black holes , the modeling of black hole spacetimes is one the most important problems in numerical general relativity . it is also one of the most challenging problems . black hole evolutions present all the usual difficulties of numerical relativity...
is encountered . this excision region is introduced after the appearance of an apparent horizon , but while a significant amount of matter remains outside the hole . we test our code by evolving accurately a vacuum schwarzschild black hole , a relativistic bondi accretion flow onto a black hole , oppenheimer - snyder d...
we present a numerical code designed to study astrophysical phenomena involving dynamical spacetimes containing black holes in the presence of relativistic hydrodynamic matter . we present evolutions of the collapse of a fluid star from the onset of collapse to the settling of the resulting black hole to a final statio...
gr-qc0401076
c
we have constructed a code to study the collapse of astrophysical objects to black holes by evolving the full coupled einstein - hydrodynamics system in both 2 + 1 ( axisymmetry ) and 3 + 1 dimensions . when a black hole appears , it is treated by introducing an excision boundary well inside the horizon . our code is s...
we present a numerical code designed to study astrophysical phenomena involving dynamical spacetimes containing black holes in the presence of relativistic hydrodynamic matter . we find that a black hole forms only if , in agreement with previous simulations . when , the collapsing star forms a torus which fragments in...
we present a numerical code designed to study astrophysical phenomena involving dynamical spacetimes containing black holes in the presence of relativistic hydrodynamic matter . we present evolutions of the collapse of a fluid star from the onset of collapse to the settling of the resulting black hole to a final statio...
0901.2052
i
trying to accurately describe black holes solutions as evolving physical objects in numerical simulations is of direct interest in astrophysics . numerical simulations have made a great leap forward in the past few years , mainly with the first stable simulations of black hole mergers in full general relativity by pret...
we present a numerical work aiming at the computation of excised initial data for black hole spacetimes in full general relativity , using dirac gauge in the context of a constrained formalism for the einstein equations . introducing the isolated horizon formalism for black hole excision , we especially solve the confo...
we present a numerical work aiming at the computation of excised initial data for black hole spacetimes in full general relativity , using dirac gauge in the context of a constrained formalism for the einstein equations . introducing the isolated horizon formalism for black hole excision , we especially solve the confo...
0901.2052
c
the data we get with our simulations are interesting at several levels . they allow to make a direct comparison between the conformally flat approximation and the exact solution for axisymmetric spacetimes containing a black hole , that are both calculated _ a priori _ and in the same gauge . as we have seen in sec . [...
our method shows good concordance on physical and geometrical issues , with the particular application of the isolated horizon multipolar analysis to confirm that the solution obtained is indeed the kerr spacetime . finally , we discuss a previous suggestion in the literature for the boundary conditions for the conform...
we present a numerical work aiming at the computation of excised initial data for black hole spacetimes in full general relativity , using dirac gauge in the context of a constrained formalism for the einstein equations . introducing the isolated horizon formalism for black hole excision , we especially solve the confo...
1601.07906
r
the standard correlations between pah ratios , obtained by ` normalizing ' each pah flux by dividing by the flux of another pah band in the same spectrum , are presented in figure [ fig : rat_corr ] , where we have chosen to use the 11.2 band to normalize the data . this procedure is performed to cancel out the effec...
these include the pah emission bands , primarily at 6.2 , 7.7 , 8.6 , 11.2 and 12.7 , as well as the spectral emission lines of neon and sulfur and the absorption band caused by silicate dust at around 9.8 . in this work we describe the data in detail , including the data reduction and measurement strategies , and subs...
we present a sample of resolved galactic h ii regions and photodissociation regions ( pdrs ) observed with the _ spitzer _ infrared spectrograph ( irs ) in spectral mapping mode between the wavelengths of 515 . for each object we have spectral maps at a spatial resolution of in which we have measured all of the mid ...