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1409.3897 | r | this paper mainly treats hypothesis testing in a bipartite quantum system and its @xmath4-copies extension . for this purpose , we firstly discuss hypothesis testing in a general quantum system @xmath9 and its @xmath4-copies extension . in quantum hypothesis testing , we consider two hypotheses , the null hypothesis an... | we consider asymptotic hypothesis testing ( or state discrimination with asymmetric treatment of errors ) between an arbitrary fixed bipartite pure state and the completely mixed state under one - way locc ( local operations and classical communications ) , two - way locc , and separable povms . as a result | we consider asymptotic hypothesis testing ( or state discrimination with asymmetric treatment of errors ) between an arbitrary fixed bipartite pure state and the completely mixed state under one - way locc ( local operations and classical communications ) , two - way locc , and separable povms . as a result , we derive... |
math0105111 | i | let @xmath4 denote the space of ( ordered ) partitions of @xmath5 , that is @xmath6 by _ size - biased _ sampling according to a point @xmath7 we mean picking the @xmath8-th part @xmath9 with probability @xmath9 . the starting point for our study is the following markov chain on @xmath4 , which we call a _ coagulation ... | we consider markov chains on the space of ( countable ) partitions of the interval $ ] , obtained first by size biased sampling twice ( allowing repetitions ) and then merging the parts with probability ( if the sampled parts are distinct ) or splitting the part with probability according to a law ( if the same part wa... | we consider markov chains on the space of ( countable ) partitions of the interval $ ] , obtained first by size biased sampling twice ( allowing repetitions ) and then merging the parts with probability ( if the sampled parts are distinct ) or splitting the part with probability according to a law ( if the same part wa... |
1602.00717 | i | consider an open bounded domain @xmath1 ( @xmath2 ) . let @xmath3 be an operator defined as @xmath4 , where @xmath5 be a real @xmath6 matrix on @xmath7 that is bounded measurable and uniformly elliptic : that is , there exists a constant @xmath8 such that @xmath9 for all @xmath10 and @xmath11 . the matrix @xmath12 is n... | we consider the dirichlet boundary value problem for divergence form elliptic operators with bounded measurable coefficients . we prove that for uniform domains with ahlfors regular boundary , the bmo solvability of such problems is equivalent to a quantitative absolute continuity of the elliptic measure with respect t... | we consider the dirichlet boundary value problem for divergence form elliptic operators with bounded measurable coefficients . we prove that for uniform domains with ahlfors regular boundary , the bmo solvability of such problems is equivalent to a quantitative absolute continuity of the elliptic measure with respect t... |
1411.6284 | i | the mean field theory provides in principle a fair approximation of time evolved quantum states by many - body schrdinger dynamics in the mean field scaling ; namely when the number of particles is large and the pair interaction potential is proportionally weak . during the last decade , a strong activity around the me... | we consider the time evolution of quantum states by many - body schrdinger dynamics and study the rate of convergence of their reduced density matrices in the mean field limit . if the prepared state at initial time is of coherent or factorized type and the number of particles is large enough then it is known that is t... | we consider the time evolution of quantum states by many - body schrdinger dynamics and study the rate of convergence of their reduced density matrices in the mean field limit . if the prepared state at initial time is of coherent or factorized type and the number of particles is large enough then it is known that is t... |
0903.3108 | i | the observation @xcite of a fractional quantum hall ( fqh ) state at @xmath0 and suggestion @xcite that the moore - read pfaffian ( mr ) state @xcite might occur at this filling fraction gave the first real indication that non - abelian topological phases of matter might actually occur in nature . the striking featu... | we compare the predictions of several different models of the state of the electrons at this plateau : the moore - read , anti - pfaffian , su naf , strong pairing , and states . et al . we suggest further experiments which could help rule out some possible scenarios . | we consider the tunneling current through a double point - contact fabry - prot interferometer such as used in recent experimental studies of the fractional quantum hall plateau at filling fraction . we compare the predictions of several different models of the state of the electrons at this plateau : the moore - read ... |
0903.3108 | c | we close this discussion by assuming , for a moment , that the experiments of refs . are , in fact , performing interferometry on the @xmath0 state of the sort envisioned in refs . and are detecting non - abelian quasiparticles . what forecast would these results give for topological quantum computation @xcite ? cer... | we make the corresponding predictions for future tunneling and interference experiments at the other observed second landau level fractional quantum hall states . `` with luck , we might see a non - abelian interferometer within a year . '' attributed to kirill shtengel , april 16 , 2008 in _ quantum computation : ... | we consider the tunneling current through a double point - contact fabry - prot interferometer such as used in recent experimental studies of the fractional quantum hall plateau at filling fraction . we compare the predictions of several different models of the state of the electrons at this plateau : the moore - read ... |
1701.08367 | c | in this work we have presented a systematic study of weakly interacting bosonic gases with local and non - local multi - body interactions in the bogoliubov approximation . we considered conservative multi - body interactions for which the number of particles is conserved : of course multi - body interactions are assoc... | we consider weakly interacting bosonic gases with local and non - local multi - body interactions . by using the bogoliubov approximation , we first investigate contact interactions , studying the case in which the interparticle potential can be written as a sum of-body-interactions , and then considering general conta... | we consider weakly interacting bosonic gases with local and non - local multi - body interactions . by using the bogoliubov approximation , we first investigate contact interactions , studying the case in which the interparticle potential can be written as a sum of-body-interactions , and then considering general conta... |
1509.07116 | i | kac @xcite in 1956 to obtain a solution from a poisson of the telegraph equation @xmath3 with @xmath4 , introduced the processes @xmath5 where @xmath6 is a poisson process of intensity @xmath7 . he noticed that if in equation ( [ tele ] ) the parameters @xmath7 and @xmath8 tend to infinity with @xmath9 constant and equ... | we construct a family of processes , from a single poisson process , that converges in law to a complex brownian motion . moreover , we find realizations of these processes that converge almost surely to the complex brownian motion , uniformly on the unit time interval . finally the rate of convergence is derived . d... | we construct a family of processes , from a single poisson process , that converges in law to a complex brownian motion . moreover , we find realizations of these processes that converge almost surely to the complex brownian motion , uniformly on the unit time interval . finally the rate of convergence is derived . d... |
1607.02792 | i | the entscheidungsproblem from mathematical logic led ramsey @xcite to the following combinatorial principle that became a cornerstone of an area now called ramsey theory . [ thm : ramsey ] for any positive integers @xmath1 , @xmath0 , and @xmath2 there exists a positive integer @xmath3 with @xmath4 i.e. , such that no... | we construct a ramsey class whose objects are steiner systems . in contrast to the situation with general-uniform hypergraphs , it turns out that simply putting linear orders on their sets of vertices is not enough for this purpose : one also has to strengthen the notion of subobjects used from `` induced subsystems ''... | we construct a ramsey class whose objects are steiner systems . in contrast to the situation with general-uniform hypergraphs , it turns out that simply putting linear orders on their sets of vertices is not enough for this purpose : one also has to strengthen the notion of subobjects used from `` induced subsystems ''... |
1304.0391 | i | by mostow rigidity , a hyperbolic structure on a closed -manifold @xmath2 is unique up to isometry . while the geometry of @xmath2 is thus completely determined by its underlying topology , it can be difficult to understand the qualitative and quantitative connections between these two facets of @xmath2 . here , we sho... | we construct hyperbolic integer homology 3-spheres where the injectivity radius is arbitrarily large for nearly all points of the manifold . as a consequence , there exists a sequence of closed hyperbolic -manifolds which benjamini - schramm converge to whose normalized ray - singer analytic torsions do _ not _ converg... | we construct hyperbolic integer homology 3-spheres where the injectivity radius is arbitrarily large for nearly all points of the manifold . as a consequence , there exists a sequence of closed hyperbolic -manifolds which benjamini - schramm converge to whose normalized ray - singer analytic torsions do _ not _ converg... |
1504.03389 | i | consider a sample @xmath5 we look for substitutes @xmath6 * * and * * @xmath7 of the sample mean vector and covariance matrix , that are resistant to atypical observations . we also want estimators that have a high efficiency for normal samples@xmath8 as a measure of robustness we consider not only the breakdown point ... | the most frequently employed estimators are not quite satisfactory in this respect . the minimum volume ellipsoid ( mve ) and minimum covariance determinant ( mcd ) estimators are known to have a very low efficiency . s - estimators with a monotonic weight function like the bisquare have a low efficiency for small and ... | we deal with the equivariant estimation of scatter and location for-dimensional data , giving emphasis to scatter . it is important that the estimators possess both a high efficiency for normal data and a high resistance to outliers , that is , a low bias under contamination . the most frequently employed estimators ar... |
astro-ph0003220 | i | a number of codes were built in the past to compute the structure and the emission of photoionized media . with time , these codes became more and more sophisticated , and able to treat a larger number of situations . in the sixties they were specially designed for planetary nebulae and hii regions , i.e. for dilute an... | we describe a code designed for hot media ( t a few 10 k ) , optically thick to compton scattering . the transfer code is coupled with a monte carlo code which allows to take into account compton and inverse compton diffusions , and to compute the spectrum emitted up to mev energies , in any geometry . several applicat... | we describe a code designed for hot media ( t a few 10 k ) , optically thick to compton scattering . it computes the structure of a plane - parallel slab of gas in thermal and ionization equilibrium , illuminated on one or on both sides by a given spectrum . contrary to the other photoionization codes , it solves the t... |
astro-ph0003220 | m | it is not always clear which approximations are used in the different codes . basically the computation of the diffuse radiation field seems to be similar in all codes , except in ross & fabian ( 1993 ) and in subsequent works using this code , where it is computed using the kompaneets equation . ( ferland 1996 ) , ( k... | we stress the importance of taking into account the returning flux even for small column densities ( 10 ) , and we show that the escape probability approximation can lead to strong errors in the thermal and ionization structure , as well as in the emitted spectrum , for a thomson thickness larger than a few tenths . | we describe a code designed for hot media ( t a few 10 k ) , optically thick to compton scattering . it computes the structure of a plane - parallel slab of gas in thermal and ionization equilibrium , illuminated on one or on both sides by a given spectrum . contrary to the other photoionization codes , it solves the t... |
1211.4250 | i | partitioning a phase space into orbits is a central step in the study of any physical or formal dynamics . immediately after the introduction of graph ( /stabilizer ) states in quantum coding theory @xcite and in the context of measurement - based quantum computation @xcite , it was evident that the related task , when... | we describe a construction that maps any connected graph on three or more vertices into a larger graph , , whose independence number is strictly smaller than its lovsz number which is equal to its fractional packing number . the vertices of represent all possible events consistent with the stabilizer group of the graph... | we describe a construction that maps any connected graph on three or more vertices into a larger graph , , whose independence number is strictly smaller than its lovsz number which is equal to its fractional packing number . the vertices of represent all possible events consistent with the stabilizer group of the graph... |
1411.0641 | i | the gemini nici planet - finding campaign was a direct - imaging survey of about 250 nearby stars for substellar and planetary - mass companions conducted at gemini south observatory between 2008 and 2012 @xcite . the campaign used the near - infrared coronagraphic imager ( nici , * ? ? ? * ) , which combines adaptive ... | the campaign requires a relative astrometric accuracy of mas across multi - year timescales in order to distinguish true companions from background stars by verifying common proper motion and parallax with their parent stars . most of the campaign data in the gemini science archive are accurate to this level but we id... | we describe the astrometric calibration of the gemini nici planet - finding campaign . the campaign requires a relative astrometric accuracy of mas across multi - year timescales in order to distinguish true companions from background stars by verifying common proper motion and parallax with their parent stars . the c... |
1010.3101 | i | the study of eleven dimensional @xmath7 invariant half - bps supergravity configurations started in @xcite . they depend on a single scalar function satisfying a non - linear toda equation . when there is an extra rotational @xmath8 isometry , there exists an implicit change of variables mapping the latter to a laplace... | this allows us to identify the appropriate boundary conditions describing the most general smooth and superstar - like singular configurations . we also compute their masses , matching the expected result from their microscopic interpretation , but now at finite radius of curvature . + _ theoretical physics grou... | we describe the geometry of the invariant half - bps m - theory configurations considered in llm in terms of their electrostatic variables . we discuss both regular configurations , such as adss and adss vacua or simple excited solutions , and singular ones such as the superstar geometries . this allows us to identify ... |
cond-mat0207167 | i | an important property of most quantum phase transitions studied to date in systems with a metallic fermi surface in spatial dimensions @xmath0 is that the critical field theory for the order parameter is a free gaussian theory @xcite . this result has its origin in the fact that the order parameters considered can be e... | we describe two dimensional models with a metallic fermi surface which display quantum phase transitions controlled by strongly interacting critical field theories below their upper critical dimension . the primary examples involve transitions with a topological order parameter associated with dislocations in collinear... | we describe two dimensional models with a metallic fermi surface which display quantum phase transitions controlled by strongly interacting critical field theories below their upper critical dimension . the primary examples involve transitions with a topological order parameter associated with dislocations in collinear... |
1207.6042 | i | we have described a large ( more than 400 nights ) ground - based survey which started in 2007 and is expected to end in 20132014 , aimed at building a grid of spss for the flux calibration of gaia spectra and magnitudes . the technical complexity of gaia requires a large ( @xmath0200 ) set of spss flux tables , calibr... | we describe two ground based observing campaigns aimed at building a grid of approximately 200 spectrophotometric standard stars ( spss ) , with an internal% precision and tied to vega within% , for the absolute flux calibration of data gathered by gaia , the esa astrometric mission . in fact , all candidates are also ... | we describe two ground based observing campaigns aimed at building a grid of approximately 200 spectrophotometric standard stars ( spss ) , with an internal% precision and tied to vega within% , for the absolute flux calibration of data gathered by gaia , the esa astrometric mission . the criteria for the selection and... |
astro-ph9905295 | i | the nature of non - luminous matter that is not part of detected and catalogued galaxies remains unsolved by modern astrophysics . as mentioned in a recent thesis , low surface brightness ( lsb ) objects may prove to be the `` icebergs '' of the extragalactic world ( de blok 1997 ) . some searches for non - luminous ma... | we detected a ring - like distribution of far - infrared emission in the direction of the center of the virgo cluster . we studied this feature in the fir , radio , and optical domains , and deduced that the dust within the feature reddens the galaxies in the direction of the virgo cluster but does not affect stars wit... | we detected a ring - like distribution of far - infrared emission in the direction of the center of the virgo cluster . we studied this feature in the fir , radio , and optical domains , and deduced that the dust within the feature reddens the galaxies in the direction of the virgo cluster but does not affect stars wit... |
astro-ph9905295 | c | we identified a ring - like feature of fir emission at high galactic latitude , which is distant from the main body of the galaxy and extinguishes light from galaxies in the central part of the virgo cluster ( vc ) . there is no way to establish a distance to the extinguishing cloud with the data we presented above , e... | we propose that a highly supersonic past collision between an hi cloud and the galactic hi formed a shock that heated the interface gas to soft x - ray temperatures . hi remnants from the projectile and from the shocked galactic hi rain down onto the disk as intermediate velocity gas . our finding emphasizes that ex... | we detected a ring - like distribution of far - infrared emission in the direction of the center of the virgo cluster . we studied this feature in the fir , radio , and optical domains , and deduced that the dust within the feature reddens the galaxies in the direction of the virgo cluster but does not affect stars wit... |
1501.07442 | i | the identification of high - energy ( regge ) dynamics in qcd processes has been long since theoretically investigated . with the advent of high - energy colliders like hera , tevatron and lhc such studies have become possible at experimental level too . the processes which are expected to be more sensitive to this pec... | we determine the jet vertex for mueller - navelet jets and forward jets in the small - cone approximation for two particular choices of jet algoritms : the kt algorithm and the cone algorithm . the differences with the original calculations of the small - cone jet vertex by ivanov and papa , which is found to be equiva... | we determine the jet vertex for mueller - navelet jets and forward jets in the small - cone approximation for two particular choices of jet algoritms : the kt algorithm and the cone algorithm . these choices are motivated by the extensive use of such algorithms in the phenomenology of jets . the differences with the or... |
1302.4593 | i | the study of effective smooth torus actions on compact , smooth manifolds has a rich and long tradition in the theory of smooth transformation groups ( cf . @xcite ) . in riemannian geometry , starting with hsiang and kleiner s topological classification of compact riemannian @xmath0-manifolds of positive ( sectional )... | we also study closed singular riemannian foliations whose leaves are homeomorphic to aspherical or to bieberbach manifolds . these foliations , which we call _ a - foliations _ and _ b - foliations _ , respectively , generalize isometric torus actions on riemannian manifolds . we apply our results to the classification... | we determine the structure of the fundamental group of the regular leaves of a closed singular riemannian foliation on a compact , simply connected riemannian manifold . we also study closed singular riemannian foliations whose leaves are homeomorphic to aspherical or to bieberbach manifolds . these foliations , which ... |
1306.1999 | i | gaussian process ( gp ) models provide a flexible , probabilistic approach to regression and are widely used . however , application of gp models to large data sets is challenging as the memory and computational requirements scale as @xmath0 and @xmath1 respectively , where @xmath2 is the number of training data points... | we develop a fast variational approximation scheme for gaussian process ( gp ) regression , where the spectrum of the covariance function is subjected to a sparse approximation . our approach enables uncertainty in covariance function hyperparameters to be treated without using monte carlo methods and is robust to over... | we develop a fast variational approximation scheme for gaussian process ( gp ) regression , where the spectrum of the covariance function is subjected to a sparse approximation . our approach enables uncertainty in covariance function hyperparameters to be treated without using monte carlo methods and is robust to over... |
1306.1999 | c | in this paper , we have presented a nonconjugate variational message passing algorithm for fitting sparse spectrum gp regression models where closed form updates are possible for all variational parameters , except for the evaluation of @xmath116 . we note that @xmath116 can be evaluated very efficiently using quadratu... | second , we propose a novel adaptive neighbourhood technique for obtaining predictive inference that is effective in dealing with nonstationarity . weighting dimensions according to lengthscales , this downweights variables of little relevance , leading to automatic variable selection and improved prediction . third , ... | we develop a fast variational approximation scheme for gaussian process ( gp ) regression , where the spectrum of the covariance function is subjected to a sparse approximation . our approach enables uncertainty in covariance function hyperparameters to be treated without using monte carlo methods and is robust to over... |
1101.5805 | i | as advances in technology allow for the collection and storage of vast databases , there is a growing need for advanced machine learning techniques for speeding up the execution of queries on such large datasets . in this work we focus on the fundamental task of estimating the selectivity , or output size , of a databa... | we develop a novel method , based on the statistical concept of the _ vapnik - chervonenkis dimension _ , to evaluate the selectivity ( output cardinality ) of sql queries a crucial step in optimizing the execution of large scale database and data - mining operations . the major theoretical contribution of this work ,... | we develop a novel method , based on the statistical concept of the _ vapnik - chervonenkis dimension _ , to evaluate the selectivity ( output cardinality ) of sql queries a crucial step in optimizing the execution of large scale database and data - mining operations . the major theoretical contribution of this work ,... |
1209.3071 | i | cooling and trapping polyatomic molecules is a promising research direction within the rapidly expanding field of cold molecular gases @xcite . because of their rich internal structure and coupled vibrational degrees of freedom , polyatomic molecules offer new research opportunities at the interface between chemistry ,... | we develop a rigorous quantum mechanical theory for collisions of polyatomic molecular radicals with s - state atoms in the presence of an external magnetic field . the theory is based on a fully uncoupled space - fixed basis set representation of the multichannel scattering wavefunction . explicit expressions are pres... | we develop a rigorous quantum mechanical theory for collisions of polyatomic molecular radicals with s - state atoms in the presence of an external magnetic field . the theory is based on a fully uncoupled space - fixed basis set representation of the multichannel scattering wavefunction . explicit expressions are pres... |
0811.4768 | i | we use the term _ protodisc _ to refer to the disc region that is initially formed when wind material from a star is channelled by dipole - type magnetic fields towards the equatorial plane . the material in a protodisc region has no radial motion and rotates with the magnetic field . it is bounded above and below by s... | we develop equations and obtain solutions for the structure and evolution of a protodisc region that is initially formed with no radial motion and super - keplerian rotation speed when wind material from a hot rotating star is channelled towards its equatorial plane by a dipole - type magnetic field . | we develop equations and obtain solutions for the structure and evolution of a protodisc region that is initially formed with no radial motion and super - keplerian rotation speed when wind material from a hot rotating star is channelled towards its equatorial plane by a dipole - type magnetic field . its temperature i... |
0811.4768 | c | in this paper , we set up equations and jump conditions to study the formation , structure and evolution of protodiscs around rotating magnetic stars with winds . we obtain solutions for a variety of stellar models with different rotation rates and magnetic field strengths . when the magnetic field of a rotating hot st... | its temperature is aroundk because of shock heating and the inflow of wind material causes its equatorial density to increase with time . the centrifugal force and thermal pressure increase relative to the magnetic force and material escapes at its outer edge . the angular velocity of the protodisc region decreases rad... | we develop equations and obtain solutions for the structure and evolution of a protodisc region that is initially formed with no radial motion and super - keplerian rotation speed when wind material from a hot rotating star is channelled towards its equatorial plane by a dipole - type magnetic field . its temperature i... |
alg-geom9706004 | i | suppose we are given linear subspaces @xmath0 of @xmath1 with @xmath2 and @xmath3 . our problem is to find all @xmath4-dimensional linear subspaces of @xmath1 which meet each @xmath5 nontrivially . when the given linear subspaces are in general position , the condition @xmath6 guarantees that there is a finite number @... | we develop numerical homotopy algorithms for solving systems of polynomial equations arising from the classical schubert calculus . these homotopies are optimal in that generically no paths diverge . for problems defined by hypersurface schubert conditions we give two algorithms based on extrinsic deformations of the g... | we develop numerical homotopy algorithms for solving systems of polynomial equations arising from the classical schubert calculus . these homotopies are optimal in that generically no paths diverge . for problems defined by hypersurface schubert conditions we give two algorithms based on extrinsic deformations of the g... |
astro-ph0401356 | i | growing numbers of large - scale jets in powerful extragalactic radio sources are now being observed at optical and x - ray frequencies ( see , e.g. , * ? ? ? new , and in many ways unexpected , results call for a wide discussion of the physical conditions within these objects , and in particular of the processes respo... | we discuss morphological properties of the large - scale jets in powerful radio sources , which are now observed at radio , optical and x - ray frequencies , in order to determine the origin of their x - ray radiation and the nature of the particle acceleration responsible for their multiwavelength emission . we sugges... | we discuss morphological properties of the large - scale jets in powerful radio sources , which are now observed at radio , optical and x - ray frequencies , in order to determine the origin of their x - ray radiation and the nature of the particle acceleration responsible for their multiwavelength emission . we show t... |
astro-ph0401356 | c | we propose that the knots observed in large - scale quasar jets in radio , optical and x - rays represent portions of the jet with an excess of kinetic power due to intermittent high activity of the jet engine . the appropriate time scales for jet activity and quiescent epochs ( @xmath71 yr and @xmath125 yr , respectiv... | such problems are especially pronounced if the observed x - ray emission is due to inverse - compton scattering of the cmb radiation . the proposed model can explain some morphological properties of quasar jets like high knot - to - interknot brightness contrasts , frequency - independent knot profiles and almost univ... | we discuss morphological properties of the large - scale jets in powerful radio sources , which are now observed at radio , optical and x - ray frequencies , in order to determine the origin of their x - ray radiation and the nature of the particle acceleration responsible for their multiwavelength emission . we show t... |
1206.0969 | i | the famous no - go theorem @xcite states that lattice fermion actions with chiral symmetry , locality and other common features must produce massless degrees of freedom in multiples of two in a continuum limit . this is contradictory with a phenomenological fact that there exist only three quarks with masses below the ... | we study strong - coupling lattice qcd with the karsten - wilczek formulation , which has one relevant parameter as well as gauge coupling and a mass parameter . we find a nontrivial chiral phase structure with a second - order phase transition between chiral symmetric and broken phases . to capture the whole structure... | we discuss the chiral phase diagram in the parameter space of lattice qcd with minimal - doubling fermions , which can be seen as lattice fermions with flavored chemical potential terms . we study strong - coupling lattice qcd with the karsten - wilczek formulation , which has one relevant parameter as well as gauge co... |
1003.1744 | i | starlight produced by the first galaxies is the leading candidate for ionizing the hydrogen as well as singly ionizing the helium at @xmath10 . it takes a harder source of radiation to doubly ionize the helium , so the reionization of this species is likely deferred until @xmath11 when quasars produce a sufficient hard... | we find that this objective can be accomplished ( using coeval h i ly absorption to mask dense regions and in cross correlation ) with a spectral resolution of and a signal - to - noise ratio per resolution element of . we also discuss how he i absorption can be used to measure the hardness of the ionizing backgrou... | we discuss the potential of using the he i forest to detect and study he ii reionization . significant absorption is expected from intergalactic he ii regions , whereas there should be no detectable absorption from low density gas in he iii regions . unlike he ii ly absorption ( the subject of much recent s... |
1003.1744 | c | this paper discussed the usefulness of the he i @xmath0 forest to study he ii reionization at @xmath313 . the optical depth of the he i @xmath0 line is proportional to the optical depth in h i ly@xmath1 by the factor @xmath314 ( ignoring differences in the amount of thermal broadening between h i and he i ... | we discuss the potential of using the he i forest to detect and study he ii reionization . we estimate the requirements for a definitive detection of redshifted he i absorption from low density gas ( ) , which would indicate that he ii reionization was occurring . such specifications may be achievable on a few... | we discuss the potential of using the he i forest to detect and study he ii reionization . significant absorption is expected from intergalactic he ii regions , whereas there should be no detectable absorption from low density gas in he iii regions . unlike he ii ly absorption ( the subject of much recent s... |
hep-ph9812230 | i | the search for supersymmetry ( susy ) @xcite plays an important rle in the experimental program at the colliders lep2 and tevatron . it will be even more important at future colliders , e.g. an upgraded tevatron , lhc , an @xmath6 linear collider or a @xmath7 collider . therefore many phenomenological studies have been... | we discuss the three - body decays , , , and ( ) of the lighter top squark within the minimal supersymmetric standard model . we give the complete analytical formulas for the decay widths and present a numerical study in view of an upgraded tevatron , the cern lhc , and a future lepton collider demonstrating the import... | we discuss the three - body decays , , , and ( ) of the lighter top squark within the minimal supersymmetric standard model . we give the complete analytical formulas for the decay widths and present a numerical study in view of an upgraded tevatron , the cern lhc , and a future lepton collider demonstrating the import... |
astro-ph0307056 | i | afterglow emission , spanning from radio to x - ray , and observable from minutes to weeks after the event , appears to be a ubiquitous feature of long - duration gamma - ray burst explosions . afterglows result from radiation emitted by electrons accelerated in a relativistic shock produced by the explosion of a proge... | we employ a fireball model of the gamma - ray burst explosion to constrain intrinsic and environmental parameters of four events with good broadband afterglow data ; grb 970508 , grb 980329 , grb 980703 , and grb 000926 . using the standard assumptions of constant circumburst density and no evolution of the fractio... | we employ a fireball model of the gamma - ray burst explosion to constrain intrinsic and environmental parameters of four events with good broadband afterglow data ; grb 970508 , grb 980329 , grb 980703 , and grb 000926 . using the standard assumptions of constant circumburst density and no evolution of the fractio... |
astro-ph0307056 | c | we fit four well - studied bursts with extensive radio through x - ray afterglow datasets to a fireball model with simple assumptions concerning the microphysics and environment . we find a range of reasonable environmental and geometrical parameters . we find all four fit best with a constant density medium , one with... | we find a variety of parameters : densities that range from those of the ism to diffuse clouds , energies comparable to the total grb-ray energy , collimations from near - isotropy to 0.04 radians , substantial electron energy fractions of 10 - 30% with energy distribution indices of 2.1 - 2.9 and magnetic energy fract... | we employ a fireball model of the gamma - ray burst explosion to constrain intrinsic and environmental parameters of four events with good broadband afterglow data ; grb 970508 , grb 980329 , grb 980703 , and grb 000926 . using the standard assumptions of constant circumburst density and no evolution of the fractio... |
1406.3741 | i | dislocations are line defects in crystalline materials which play an important role in governing the deformation and failure mechanisms in solids . the energetics of dislocations and their interactions with other defects solute atoms , precipitates , grain boundaries , surfaces and interfaces significantly influence ... | we employed a real - space formulation of orbital - free density functional theory using finite - element basis to study the defect - core and energetics of an edge dislocation in aluminum . our study shows that the core - size of a perfect edge dislocation is around ten times the magnitude of the burgers vector . cons... | we employed a real - space formulation of orbital - free density functional theory using finite - element basis to study the defect - core and energetics of an edge dislocation in aluminum . our study shows that the core - size of a perfect edge dislocation is around ten times the magnitude of the burgers vector . this... |
1406.3741 | r | we now present our study of an edge dislocation in aluminum using large - scale electronic - structure calculations . in particular , we unambiguously identify the size of the dislocation core , directly compute the dislocation core - energy , study the effect of macroscopic deformations on dislocation core - energy an... | this finding is contrary to the widely accepted notion that continuum descriptions of dislocation energetics are accurate beyond burgers vector from the dislocation line . interestingly , our study revealed a significant influence of macroscopic deformations on the core - energy of shockley partials . further , we demo... | we employed a real - space formulation of orbital - free density functional theory using finite - element basis to study the defect - core and energetics of an edge dislocation in aluminum . our study shows that the core - size of a perfect edge dislocation is around ten times the magnitude of the burgers vector . this... |
0906.0286 | c | for the first time in the literature we have estimated the cross section for exclusive @xmath0 meson ( glueball candidate ) production not far from the threshold . we have included both gluon induced diffractive and triangle - double - diffractive mechanisms as well as the pion - pion exchange contributions . the qc... | , pion - pion meson exchange current ( mec ) components as well as double - diffractive mechanism with intermediate pionic loop are calculated for the first time in the literature . the pion - pion component , which can be reliably calculated , dominates close to the threshold while the diffractive component may take o... | we evaluate differential distributions for exclusive scalar meson ( glueball candidate ) production for ( fair@gsi ) and ( j - parc@tokai ) . both qcd diffractive , pion - pion meson exchange current ( mec ) components as well as double - diffractive mechanism with intermediate pionic loop are calculated for the first ... |
1603.00495 | i | we have identified on _ galex _ images the furthest out distinct @xmath0 knot in the little things sample of dirr and bcd galaxies that we are confident belong to the galaxy . these knots are found at distances from the center of the galaxies of 1 to 8 disk scale lengths and have ages of @xmath1 myrs and masses of 20 m... | we examine images of the little things sample of nearby dwarf irregular ( dirr ) and blue compact dwarf ( bcd ) galaxies to identify distinct young regions in their far outer disks . the knots are found at distances from the center of the galaxies of 1 to 8 disk scale lengths and have ages of myrs and masses of 20 m_ ... | we examine images of the little things sample of nearby dwarf irregular ( dirr ) and blue compact dwarf ( bcd ) galaxies to identify distinct young regions in their far outer disks . we use these data , obtained with the _ galaxy evolution explorer _ satellite , to determine the furthest radius at which _ in situ _ sta... |
cond-mat0206176 | i | to the best of our knowledge , the concept of the non - hermitian effective hamiltonian appeared first in feshbach s papers @xcite in connection with the general theory of resonance nuclear reactions @xcite and , independently , in livic s study of open systems @xcite . a typical atomic nucleus forms near an excitation... | the scattering amplitude is expressed in terms of the resolvent of a non - hermitian operator . we note that the simple breit - wigner approximation is as a rule valid for any individual resonance in the case of few - channel scattering on a flat billiard - like cavity , leaving no room for non - trivial to appear . we... | we examine the notion and properties of the non - hermitian effective hamiltonian of an unstable system using as an example potential resonance scattering with a fixed angular momentum . we present a consistent self - adjoint formulation of the problem of scattering on a finite - range potential , which is based on sep... |
cond-mat0206176 | c | in this paper we analyzed the relevance of the concept of the non - hermitian effective hamiltonian in finite - range potential scattering . single - channel @xmath9-wave resonance scattering is considered as an example . the scattering function @xmath13 is meromorphic in this case , i.e. , has only isolated poles in t... | we examine the notion and properties of the non - hermitian effective hamiltonian of an unstable system using as an example potential resonance scattering with a fixed angular momentum . we present a consistent self - adjoint formulation of the problem of scattering on a finite - range potential , which is based on sep... | we examine the notion and properties of the non - hermitian effective hamiltonian of an unstable system using as an example potential resonance scattering with a fixed angular momentum . we present a consistent self - adjoint formulation of the problem of scattering on a finite - range potential , which is based on sep... |
astro-ph9609051 | c | using the power ratios ( @xmath164 ) of buote & tsai ( 1995 bta ; 1996 btb ; tsai & buote 1996 tb ) we have examined the sensitivity of galaxy cluster morphologies to @xmath0 and @xmath1 using large , high - resolution n - body simulations . x - ray images are generated from the dark matter by letting the gas densit... | we examine the sensitivity of the spatial morphologies of galaxy clusters to and using high - resolution n - body simulations with large dynamic range . finally , we compared these models to a sample of clusters and find that the pr means of the scdm clusters exceed the means with a high formal level of significance . ... | we examine the sensitivity of the spatial morphologies of galaxy clusters to and using high - resolution n - body simulations with large dynamic range . variants of the standard cdm model are considered having different spatial curvatures , scdm , ocdm , lcdm , and different normalizations , . we also explore critical ... |
0810.1104 | i | neutrino oscillation experiments involving neutrinos and antineutrinos coming from astrophysical and terrestrial sources @xcite have found compelling evidence that neutrinos have mass . to accommodate this observation , the minimal standard model ( sm ) must be extended . some sensible ways to do this include : ( a ) t... | we explore how the seesaw sector in neutrino mass models may be constrained through symmetries to be completely determined in terms of low - energy mass , mixing angle and-violating phase observables . implications for leptogenesis and collider detection of heavy neutral leptons are discussed . the model where the neut... | we explore how the seesaw sector in neutrino mass models may be constrained through symmetries to be completely determined in terms of low - energy mass , mixing angle and-violating phase observables . the key ingredients are intra - family symmetries to determine the neutrino dirac mass matrix in terms of the charged ... |
nucl-th0512002 | i | the three - body problem has a long history from macroscopic celestial classical mechanics , e.g. sun - earth - moon @xcite to microscopic quantum mechanics , e.g. the helium atom @xcite , three nucleons @xcite or three quarks @xcite . the modern treatment was boosted by the formulation of the faddeev equations @xcite ... | we expose the relation between the properties of the three - body continuum states and their two - body subsystems . these properties refer to their bound and virtual states and resonances , all defined as poles of the-matrix . for one infinitely heavy core and two non - interacting light particles , these generic rela... | we expose the relation between the properties of the three - body continuum states and their two - body subsystems . these properties refer to their bound and virtual states and resonances , all defined as poles of the-matrix . for one infinitely heavy core and two non - interacting light particles , the complex energi... |
1101.0365 | i | cosmology tells us that about 25% of the total mass density in the universe is dark matter that can not be accounted for by conventional baryons @xcite . alongside observation , intense theoretical efforts are made in order to elucidate the nature and properties of this unknown form of matter . in this context , electr... | we extend the standard model by adding two gauge - singlet-symmetric scalar fields that interact with visible matter only through the higgs particle . one is a stable dark matter wimp , and the other one undergoes a spontaneous breaking of the symmetry that opens new channels for the dark matter annihilation , hence lo... | we extend the standard model by adding two gauge - singlet-symmetric scalar fields that interact with visible matter only through the higgs particle . one is a stable dark matter wimp , and the other one undergoes a spontaneous breaking of the symmetry that opens new channels for the dark matter annihilation , hence lo... |
0910.3132 | i | in the absence of flavor symmetries , the yukawa couplings between the standard model ( sm ) fermions and the higgs field are in general complex arbitrary matrices which , after electroweak symmetry breaking ( ewsb ) , become the mass matrices of the quarks and charged leptons . in the case of neutrinos , the mass matr... | we then study a special class of fermion mass matrices , defined by the requirement that all of the diagonalizing unitary matrices ( in the up , down , charged lepton and neutrino sectors ) contain at least one mixing angle much smaller than the other two . our new parametrization allows us to quickly extract informati... | we first obtain the most general and compact parametrization of the unitary transformation diagonalizing any hermitian matrix , as a function of its elements and eigenvalues . we then study a special class of fermion mass matrices , defined by the requirement that all of the diagonalizing unitary matrices ( in the up ,... |
0910.3132 | c | in this work , we started by obtaining the simplest parametrization for the diagonalization of a @xmath222 hermitian matrix , as a function of both its matrix elements and its eigenvalues . since the masses of fermions in the sm are well known , the problem to attack is not an eigenvalue problem , but an eigenvector pr... | we first obtain the most general and compact parametrization of the unitary transformation diagonalizing any hermitian matrix , as a function of its elements and eigenvalues . in particular we find that the phase difference between two elements of the two mass matrices ( of the sector in question ) controls the generic... | we first obtain the most general and compact parametrization of the unitary transformation diagonalizing any hermitian matrix , as a function of its elements and eigenvalues . we then study a special class of fermion mass matrices , defined by the requirement that all of the diagonalizing unitary matrices ( in the up ,... |
cond-mat0211001 | i | issues of quantum measurement in mesoscopic systems have recently garnered considerable interest , both because of their relevance to attempts at quantum computation @xcite and quantum - limited amplifiers @xcite . a general consequence of any quantum measurement is that it must induce decoherence in the system variabl... | we formulate general conditions necessary for a linear - response detector to reach the quantum limit of measurement efficiency , where the measurement - induced dephasing rate takes on its minimum possible value . these conditions are applicable to both non - interacting and interacting systems . we assess the status ... | we formulate general conditions necessary for a linear - response detector to reach the quantum limit of measurement efficiency , where the measurement - induced dephasing rate takes on its minimum possible value . these conditions are applicable to both non - interacting and interacting systems . we assess the status ... |
1012.0591 | i | a _ crossing - free straight - edge graph _ @xmath9 is an embedding of a planar graph in the plane such that the vertices are mapped to a set @xmath0 of points in the plane and the edges are pairwise non - crossing line segments between pairs of points in @xmath0 . ( segments are allowed to share endpoints . ) by fry s... | we prove a worst - case tight lower bound for the number of pseudo - simultaneously flippable edges in a triangulation in terms of the number of vertices . we use this bound for deriving new upper bounds for the maximal number of crossing - free straight - edge graphs that can be embedded on any fixed set of points in ... | we generalize the notions of flippable and simultaneously flippable edges in a triangulation of a set of points in the plane to so - called _ pseudo - simultaneously flippable edges_. such edges are related to the notion of convex decompositions spanned by . we prove a worst - case tight lower bound for the number o... |
1012.3729 | i | a quandle , which was introduced by joyce @xcite , is an algebraic object whose axioms are motivated by knot theory and conjugation in a group . in @xcite , carter , jelsovsky , kamada , langford and saito introduced a quandle homology theory , and they defined the quandle cocycle invariants for classical knots and sur... | we give a construction of quandle cocycles from group cocycles , especially , for any integer , quandle cocycles of the dihedral quandle from group cocycles of the cyclic group . we will show that a group 3-cocycle of gives rise to a non - trivial quandle 3-cocycle of . when is an odd prime , since , our 3-cocycle is a... | we give a construction of quandle cocycles from group cocycles , especially , for any integer , quandle cocycles of the dihedral quandle from group cocycles of the cyclic group . we will show that a group 3-cocycle of gives rise to a non - trivial quandle 3-cocycle of . when is an odd prime , since , our 3-cocycle is a... |
0704.2133 | i | adiabatic pair creation ( apc ) has been called unfortunately misleading spontaneous pair creation ( @xcite,@xcite - @xcite,@xcite ) . the creation of electron positron pairs in very strong external classical electromagnetic fields arises straight forwardly from the dirac sea interpretation of negative energy states ... | we give here the proof that pair creation arises from the dirac equation with an external time dependent potential . pair creation happens with probability one if the potential changes adiabatically in time and becomes overcritical , that is when an eigenvalue curve ( as function of time ) bridges the gap between the n... | we give here the proof that pair creation arises from the dirac equation with an external time dependent potential . pair creation happens with probability one if the potential changes adiabatically in time and becomes overcritical , that is when an eigenvalue curve ( as function of time ) bridges the gap between the n... |
cond-mat0306532 | i | half - doped perovskite manganites re@xmath3a@xmath3mno@xmath4 ( re - rare earth , a - alkaline earth ) exhibit very specific properties quite different from manganites with other @xmath5 electron concentrations.@xcite generally , for large size re and a cations or when external pressure is applied@xcite these compound... | we have analyzed different correlation functions in a realistic spin - orbital model for half - doped manganites . using a finite - temperature diagonalization technique the ce phase was found in the charge - ordered phase in the case of small antiferromagnetic interactions between electrons . it is shown that a key in... | we have analyzed different correlation functions in a realistic spin - orbital model for half - doped manganites . using a finite - temperature diagonalization technique the ce phase was found in the charge - ordered phase in the case of small antiferromagnetic interactions between electrons . it is shown that a key in... |
astro-ph0311281 | c | we have analysed all the available rxte data of between 1997 february and 2002 may and investigated its spectral and timing properties in correlation . this work has been motivated by recent reports that show that if large data sets are used , the atoll sources displaying the largest ampitude variations in intensity s... | these states are respectively identified with the extreme island , island and banana states that characterize the atoll sources . the very - low frequency noise that characterizes the banana - state power spectra below 1 hz can not be described in terms of a single power law but a two - component model is required . in... | we have analyzed five x - ray outbursts of the neutron - star soft x - ray transient and investigated the timing properties of the source in correlation with its spectral states as defined by different positions in the color - color and hardness - intensity diagrams . the hard color and the source count rate serve as ... |
astro-ph0509182 | i | a great deal of progress has been made in the last decade in the studies of distant galaxies . the average star formation history of the universe has also been estimated from emission properties of galaxies detected in deep imaging and redshift surveys such as the canada - france redshift survey and the hubble deep fie... | we compare our results with those from other emission - line studies of absorber fields and with predictions for global average sfr based on the models of cosmic chemical evolution . , these studies suggest that sfrs in a large fraction of objects in the absorber fields may lie below the global mean sfr . however , it ... | we have carried out a deep narrow - band imaging survey of six fields with heavy - element quasar absorption lines , using the goddard fabry - perot ( fp ) system at the apache point observatory ( apo ) 3.5-meter telescope . the aim of these observations was to search for redshifted ly- emission from the galaxies under... |
astro-ph0509182 | r | figures 1(a)-6(a ) show @xmath38 sections of the reduced broad - band ( b ) images of the quasar absorber fields of q0216 + 080 , q0636 + 680 , q0956 + 123 , q1209 + 093 , q1442 + 101 , and q2233 + 131 , respectively . the corresponding panels ( b ) show the narrow - band images of the same fields obtained with the blu... | the 3 sensitivity levels ranged between and erg s in observed - frame ly- flux . no significant ly- emitters were detected at level . the absence of significant ly- emission implies limits on the star formation rate ( sfr ) of 0.9 - 2.7 yr per 2-pixel x 2-pixel region , if no dust attenuation is assumed . our limits ar... | we have carried out a deep narrow - band imaging survey of six fields with heavy - element quasar absorption lines , using the goddard fabry - perot ( fp ) system at the apache point observatory ( apo ) 3.5-meter telescope . the aim of these observations was to search for redshifted ly- emission from the galaxies under... |
astro-ph0509182 | c | for most of our targets , no other imaging information exists in any waveband on a scale comparable to our fields of view . for q0216 + 080 and q2233 + 131 , hst nicmos h - band images are available ( warren et al . the nicmos images of q0216 + 080 show two objects with @xmath58 and 24.34 , located 1.4@xmath28 and 3.8@... | we have carried out a deep narrow - band imaging survey of six fields with heavy - element quasar absorption lines , using the goddard fabry - perot ( fp ) system at the apache point observatory ( apo ) 3.5-meter telescope . the aim of these observations was to search for redshifted ly- emission from the galaxies under... | we have carried out a deep narrow - band imaging survey of six fields with heavy - element quasar absorption lines , using the goddard fabry - perot ( fp ) system at the apache point observatory ( apo ) 3.5-meter telescope . the aim of these observations was to search for redshifted ly- emission from the galaxies under... |
astro-ph0012341 | r | figure 1 shows the distribution of the integrated intensity of co j=21 emission . the velocity range is between @xmath17 and @xmath18 , which covers most of the emission . the overlaied contour map shows the 1420 mhz brightness distribution of hb 21 ( t90 ) . the overall distribution of co gas in figure 1 is not ... | molecular gas appears to be distributed mainly along the boundary of the snr , but the overall distribution has little correlation either with the distortion of the snr boundary or with the distribution of radio brightness . along the eastern boundary , where the snr was considered to be interacting with molecular clou... | we have carried outco j=21 line observations of the supernova remnant ( snr ) hb 21 in order to search for evidence of interaction with molecular clouds . we mapped the eastern half ( ) of the snr almost completely . molecular gas appears to be distributed mainly along the boundary of the snr , but the overall distrib... |
astro-ph0012341 | i | we have mapped the eastern half ( @xmath192 ) of the snr hb 21 in @xmath0co j=21 line emission almost completely . our map , which has been completely sampled with @xmath193 resolution , shows the detailed structure of molecular clouds in this area . we have detected broad co lines with large @xmath57 in the northern ... | we have carried outco j=21 line observations of the supernova remnant ( snr ) hb 21 in order to search for evidence of interaction with molecular clouds . instead we detected broad ( 2040 ) co emission lines in the northern and southern parts of the snr . in the northern area , the broad - line emitting cloud is comp... | we have carried outco j=21 line observations of the supernova remnant ( snr ) hb 21 in order to search for evidence of interaction with molecular clouds . we mapped the eastern half ( ) of the snr almost completely . molecular gas appears to be distributed mainly along the boundary of the snr , but the overall distrib... |
1006.5932 | c | we have derived an x - ray luminosity function for 12 dwarf novae using archival _ suzaku _ , _ xmm - newton _ , and _ asca _ observations , and obtained new observations for bz uma , sw uma , vy aqr , ss aur , v893 sco and asas j0025 with _ suzaku _ as originally , they were not available in the archive . our re... | we have derived an x - ray luminosity function using parallax - based distance measurements of a set of 12 dwarf novae , consisting of _ suzaku _ , _ xmm - newton _ and _ asca _ observations . the total integrated luminosity within a radius of 200 pc is 1.48 10 erg s over the luminosity range of 1 10 erg s and the max... | we have derived an x - ray luminosity function using parallax - based distance measurements of a set of 12 dwarf novae , consisting of _ suzaku _ , _ xmm - newton _ and _ asca _ observations . the shape of the x - ray luminosity function obtained is the most accurate to date , and the luminosities of our sample are con... |
1006.5932 | c | we have analysed the x - ray spectra of 13 dwarf novae with accurate parallax - based distance estimates , and derived the most accurate shape for the x - ray luminosity function of dne in the 210 kev band to date due to accurate distance measurements and due to the fact that we did not use an x - ray selected sample ... | the shape of the x - ray luminosity function obtained is the most accurate to date , and the luminosities of our sample are concentrated between 10 erg s , lower than previous measurements of x - ray luminosity functions of dwarf novae . based on the integrated x - ray luminosity function , the sample becomes more inco... | we have derived an x - ray luminosity function using parallax - based distance measurements of a set of 12 dwarf novae , consisting of _ suzaku _ , _ xmm - newton _ and _ asca _ observations . the shape of the x - ray luminosity function obtained is the most accurate to date , and the luminosities of our sample are con... |
0811.1616 | i | quantum phase transitions originating from quantum fluctuations have been extensively studied as a hot issue in condensed - matter physics . several interesting characteristics of the transitions appear in the low - energy behavior of the systems . two types of approach can capture the phase transitions and critical ph... | we have developed a numerical procedure to clarify the critical behavior near a quantum phase transition by analyzing a multi - point correlation function characterizing the ground state . this work presents a successful application of this procedure to the string order parameter of the chain with uniaxial single - ion... | we have developed a numerical procedure to clarify the critical behavior near a quantum phase transition by analyzing a multi - point correlation function characterizing the ground state . this work presents a successful application of this procedure to the string order parameter of the chain with uniaxial single - ion... |
0811.1616 | r | let us first review the behavior of the four order parameters under consideration in a finite - size system and summarize some important relations between them . in a moderately large system , we can see indications of asymptotic behavior in each order parameter , although slow convergence prevents a full description .... | this quantity shows that the finite - size scaling sensitively changes at the critical point . our estimates of the transition point and the critical exponents , which are determined only by the ground - state quantities , are consistent with results obtained from the analysis of the energy - level structure . this wor... | we have developed a numerical procedure to clarify the critical behavior near a quantum phase transition by analyzing a multi - point correlation function characterizing the ground state . this work presents a successful application of this procedure to the string order parameter of the chain with uniaxial single - ion... |
0712.2979 | i | rich groups and clusters of galaxies are immersed in hot ( @xmath0@xmath4@xmath5 k ) x - ray - emitting gas that constitutes a large fraction of their baryonic mass @xcite . radiative cooling of this gas , by virtue of its x - ray emission , should result in an inflow of relatively cool gas to the cluster center ; i.e... | we have imaged in co(2 - 1 ) the molecular gas in ngc 1275 ( perseus a ) , the cd galaxy at the center of the perseus cluster , at a spatial resolution of kpc over a central region of radius kpc . per a is known to contain of molecular gas , which has been proposed to be captured from mergers with or ram - pressure... | we have imaged in co(2 - 1 ) the molecular gas in ngc 1275 ( perseus a ) , the cd galaxy at the center of the perseus cluster , at a spatial resolution of kpc over a central region of radius kpc . per a is known to contain of molecular gas , which has been proposed to be captured from mergers with or ram - pressure... |
0712.2979 | i | to better understand the origin of the molecular gas in per a , we have imaged this galaxy in co(2 - 1 ) at an angular resolution of 3 ( spatial resolution of 1 kpc ) with the submillimeter array ( sma ) . single - dish maps with angular resolutions as high as 12 ( 4 kpc ) have previously shown that the molecular ... | the molecular gas detected in our image has a total mass of , and for the first time can be seen to be concentrated in three radial filaments with lengths ranging from at least 1.12.4 kpc all lying in the east - west directions spanning the center of the galaxy to radii of kpc . the eastern and outer western filament... | we have imaged in co(2 - 1 ) the molecular gas in ngc 1275 ( perseus a ) , the cd galaxy at the center of the perseus cluster , at a spatial resolution of kpc over a central region of radius kpc . per a is known to contain of molecular gas , which has been proposed to be captured from mergers with or ram - pressure... |
1607.07907 | i | recently we have proposed @xcite that the 750gev - resonance@xcite - which now turned out to be only a statistcal fluctuation@xcite - were our long speculated and waited for bound state@xcite of 6 top + 6 anti top quarks . the very suggestive existence of the bound state as well as the in the present article to be pres... | it is crucial to assume , that our since long speculated principle `` multiple point principle '' is true . this principle says : _ there are several vacua all having almost zero energy density_. further we make an approximation of the higgs yukawa potential essentially replacing the exponential in it by a step - funct... | we have long speculated , that 6 top + 6 anti - top quarks due to the realtively large size of the top - yukawa coupling would bind exceptionaly strongly by mainly higgs exchange . here we present a surprisingly simple `` calculation '' of the mass of this speculated bound state . even a possible resonance in scatterin... |
1607.07907 | c | we have presented an overly simple `` calculation '' leading to there being due to the strong top - yukawa coupling and under the assumtion of a finetuning ensuring a with the normal vacuum degenerate one with a condensate of bound states s = f of six top + six anti top , two `` resonances '' with masses respectively @... | we have long speculated , that 6 top + 6 anti - top quarks due to the realtively large size of the top - yukawa coupling would bind exceptionaly strongly by mainly higgs exchange . here we present a surprisingly simple `` calculation '' of the mass of this speculated bound state . the new result means that there are no... | we have long speculated , that 6 top + 6 anti - top quarks due to the realtively large size of the top - yukawa coupling would bind exceptionaly strongly by mainly higgs exchange . here we present a surprisingly simple `` calculation '' of the mass of this speculated bound state . even a possible resonance in scatterin... |
0808.3393 | c | four of the sb2 solutions shown in figures [ fig : sb2plots1 ] and [ fig : sb2plots2 ] depend on a single measurement of the secondary velocity , and another nine on only two measurements . consequently , many of the derived @xmath48 s , and the resulting @xmath6 s , have large uncertainties . figure [ fig : qvsqmin ... | we combine our double - lined infrared measurements with well constrained orbital parameters from visible light single - lined observations to derive dynamical mass ratios . using these results , along with photometry and theoretical mass - luminosity relationships , our emphasis is on measuring these distributions , n... | we have observed a large sample of spectroscopic binary stars in the hyades cluster , using high resolution infrared spectroscopy to detect low mass companions . we combine our double - lined infrared measurements with well constrained orbital parameters from visible light single - lined observations to derive dynamica... |
0808.3393 | i | we have obtained high resolution infrared spectroscopy of 32 sbs in the hyades , whose sb1 orbital parameters have been measured by rps and dwl at the cfa , in order to detect their companions and thereby study the binary mass ratio distribution in this young cluster . we detected the companion in 25 of these systems .... | we have observed a large sample of spectroscopic binary stars in the hyades cluster , using high resolution infrared spectroscopy to detect low mass companions . this corresponds to secondary masses as small as . this paper is an initial step in a program to produce distributions of mass ratio and secondary mass for hy... | we have observed a large sample of spectroscopic binary stars in the hyades cluster , using high resolution infrared spectroscopy to detect low mass companions . we combine our double - lined infrared measurements with well constrained orbital parameters from visible light single - lined observations to derive dynamica... |
0907.4004 | i | the interstellar medium is known to be inhomogeneous , consisting of various gaseous phases , from cool molecular clouds to tenuous million degree gas @xcite . a study of the interaction of a supersonic wind with a dense cloud is a problem with many astronomical applications , such as galactic winds , supernova remnant... | these simulations are motivated by our recent three - dimensional model of a starburst - driven galactic wind interacting with an inhomogeneous disk , which show that an optically emitting filament can be formed by the break - up and acceleration of a cloud into a supersonic wind . in this study we confirm the mechanis... | we have performed a series of three - dimensional simulations of the interaction of a supersonic wind with a non - spherical radiative cloud . these simulations are motivated by our recent three - dimensional model of a starburst - driven galactic wind interacting with an inhomogeneous disk , which show that an optical... |
0907.4004 | i | we have performed a series of three - dimensional simulations of the interaction of a supersonic wind with a radiative cloud . we consider two different cloud geometries ( i.e. fractal and spherical ) , which enable us to investigate the impact of the initial shape and structure of the cloud on its subsequent evolution... | we have performed a series of three - dimensional simulations of the interaction of a supersonic wind with a non - spherical radiative cloud . we consider the evolution of a cloud with two different geometries ( fractal and spherical ) and investigate the importance of radiative cooling on the cloud s survival . we fin... | we have performed a series of three - dimensional simulations of the interaction of a supersonic wind with a non - spherical radiative cloud . these simulations are motivated by our recent three - dimensional model of a starburst - driven galactic wind interacting with an inhomogeneous disk , which show that an optical... |
1008.1058 | i | the size distribution is one of the most fundamental properties of a planetesimal population . as the size of an object is primarily determined from its accretion and collisional disruption histories , the size distribution can reveal important information on the accretion and collisional history of that population ( f... | we have performed an ecliptic survey of the kuiper belt , with an areal coverage of 8.9 square degrees to a 50% limiting magnitude of , and have detected 88 kuiper belt objects , roughly half of which received follow - up one to two months after detection . using this survey data alone , we have measured the luminosity... | we have performed an ecliptic survey of the kuiper belt , with an areal coverage of 8.9 square degrees to a 50% limiting magnitude of , and have detected 88 kuiper belt objects , roughly half of which received follow - up one to two months after detection . using this survey data alone , we have measured the luminosity... |
1008.1058 | c | the observed luminosity functions imply size distribution slopes @xmath110 , @xmath111 , and @xmath112 for the _ cold _ , _ hot _ , and _ close _ populations . the consistency of the _ hot _ and _ close _ populations leaves us to consider the two populations together , implying a slope for the combined population of @x... | this suggests that the dynamically excited population underwent a different accretion history and achieved a more evolved state of accretion than the cold population . we find that while the jupiter family comets and the scattered disk exhibit similar size distributions , a power - law extrapolation to small sizes for ... | we have performed an ecliptic survey of the kuiper belt , with an areal coverage of 8.9 square degrees to a 50% limiting magnitude of , and have detected 88 kuiper belt objects , roughly half of which received follow - up one to two months after detection . using this survey data alone , we have measured the luminosity... |
1008.1058 | c | we have performed an ecliptic survey , and have detected 88 kuiper belt objects with magnitudes @xmath142 . a subset of these objects have received additional follow - up observations allowing us to accurately determine their inclinations and distances . using these data , we have measured the size distribution of the ... | we have found that the _ cold _ population defined as having inclinations less than has a luminosity function slope , and is different from the _ hot _ population , which has inclinations greater than and a luminosity function slope . as well , we have found that those objects closer than 38 au have virtually the same ... | we have performed an ecliptic survey of the kuiper belt , with an areal coverage of 8.9 square degrees to a 50% limiting magnitude of , and have detected 88 kuiper belt objects , roughly half of which received follow - up one to two months after detection . using this survey data alone , we have measured the luminosity... |
1106.1927 | r | optical cmds provide a powerful means of selecting likely _ chandra _ source counterparts and investigating their properties . for each of the 79 _ chandra _ sources within the half - mass radius , we checked the locations of all objects within the x - ray error circle in the cmds shown in figures [ f : cmd_cv ] and... | we have searched for optical identifications for 79 _ chandra _ x - ray sources that lie within the half - mass radius of the nearby , core - collapsed globular cluster ngc 6397 , using deep hubble space telescope advanced camera for surveys wide field channel imaging in , , and . photometry of these images allows us ... | we have searched for optical identifications for 79 _ chandra _ x - ray sources that lie within the half - mass radius of the nearby , core - collapsed globular cluster ngc 6397 , using deep hubble space telescope advanced camera for surveys wide field channel imaging in , , and . photometry of these images allows us ... |
1106.1927 | i | we have shown that with moderately deep @xmath1 , @xmath0 , and _ hst_-acs / wfc imaging , it is possible to identify and classify nearly all of the 79 currently detected _ chandra _ sources within the half - mass radius of ngc 6397 . our classifications are based on cmd location and are tested for consistency with e... | in addition to recovering nine previously detected cataclysmic variables ( cvs ) , we have identified six additional faint cv candidates , a total of 42 active binaries ( abs ) , two millisecond pulsars ( msps ) , one candidate active galactic nucleus , and one candidate interacting galaxy pair . of the 79 sources , 69... | we have searched for optical identifications for 79 _ chandra _ x - ray sources that lie within the half - mass radius of the nearby , core - collapsed globular cluster ngc 6397 , using deep hubble space telescope advanced camera for surveys wide field channel imaging in , , and . photometry of these images allows us ... |
astro-ph0511571 | i | deep multiwavelength surveys are progressively sheding light on the history of galaxy evolution since very high redshifts . from new surveys in the ultraviolet regime ( e.g. martin et al . 2005 ) to the latest ir , sub - millimetre and radio campaigns ( e.g. werner et al . 2004 ; dunlop 2005 ; condon et al . 2003 ) , t... | we have selected and analysed the properties of a sample of 2905 galaxies in of the great observatories origins deep survey ( goods ) chandra deep field south ( cdfs ) , to obtain further constraints on the evolution of-selected galaxies with respect to the results already obtained in previous studies . | we have selected and analysed the properties of a sample of 2905 galaxies in of the great observatories origins deep survey ( goods ) chandra deep field south ( cdfs ) , to obtain further constraints on the evolution of-selected galaxies with respect to the results already obtained in previous studies . we made use of ... |
astro-ph0511571 | i | with the goods project close to completion , in this work we have been able to set tighter constraints on the evolution of near - ir - selected galaxies in the goods / cdfs field . we took advantage of the latest available very deep and homogeneous multiwavelength photometry , in conjunction with the information provid... | we made use of the public deep multiwavelength imaging from the optical through the infrared ( ir ) bands , in conjunction with available spectroscopic and combo17 data in the cdfs , to construct an optimised redshift catalogue for our galaxy sample . we computed the-band lf and determined that its characteristic magni... | we have selected and analysed the properties of a sample of 2905 galaxies in of the great observatories origins deep survey ( goods ) chandra deep field south ( cdfs ) , to obtain further constraints on the evolution of-selected galaxies with respect to the results already obtained in previous studies . we made use of ... |
0908.2678 | r | the rmf+bcs minimizations with nl - sv1 give rise to a prolate and an oblate solution for most of the nuclei . we show the quadrupole deformation @xmath64 for the lowest energy state ( ground state ) for all the isotopic chains in figures [ fig : fig1](a)- [ fig : fig1](j ) . a large number of nuclei in these chains ... | the region of study spans nuclides with neutron numbers . it is shown that a large number of nuclides exhibit the phenomenon of shape - coexistence over a significant region of the superheavy elements . shape coexistence of a prolate and an oblate shape is prevalent in nuclides far below , whilst nuclei in the vicinity... | we have studied properties and shell structure of the superheavy elements from to within the framework of the rmf theory . the region of study spans nuclides with neutron numbers . the lagrangian model nl - sv1 with the inclusion of the vector self - coupling of the-meson has been employed in this work . we have perfor... |
0908.2678 | i | we have studied the structure of superheavy nuclei within the framework of the relativistic mean - field theory . the region of superheavy elements from @xmath0 to @xmath1 has been explored . the isotopic chains of the superheavy elements encompassing the neutron number from @xmath26 to @xmath27 have been investigated ... | the lagrangian model nl - sv1 with the inclusion of the vector self - coupling of the-meson has been employed in this work . the ground - state binding energies , single - particle properties and quadrupole deformation of nuclei have been obtained from the mean - field minimizations . the shell structure and 2-neutron ... | we have studied properties and shell structure of the superheavy elements from to within the framework of the rmf theory . the region of study spans nuclides with neutron numbers . the lagrangian model nl - sv1 with the inclusion of the vector self - coupling of the-meson has been employed in this work . we have perfor... |
0911.2212 | i | this is a continuing study of the narrow - line region ( hereafter nlr ) of the seyfert galaxy ngc4151 using data obtained with the gemini near - infrared integral field spectrograph ( nifs ) . the data comprise spectra of the inner@xmath12pc@xmath13 , at a spatial resolution of@xmath14pc at the galaxy , covering the w... | we have used the gemini near - infrared integral field spectrograph ( nifs ) to map the gas kinematics of the inner 200pc of the seyfert galaxy ngc4151 in the z , j , h and k bands at a resolving power and spatial resolution ofpc . the ionised gas emission is most extended along the known ionisation bi - cone at positi... | we have used the gemini near - infrared integral field spectrograph ( nifs ) to map the gas kinematics of the inner 200pc of the seyfert galaxy ngc4151 in the z , j , h and k bands at a resolving power and spatial resolution ofpc . the ionised gas emission is most extended along the known ionisation bi - cone at positi... |
0911.2212 | c | in the centroid velocity maps for the ionised gas emission ( fig.[f - doublevel ] ) , the lowest velocities are observed at the nucleus , while the highest are observed away from the nucleus . this is the case for ngc4151 and also for 6 other seyfert galaxies for which we have recently obtained kinematic data with the ... | this indicates that the agn ionizes gas beyond the borders of the bi - cone , within a sphere with radius around the nucleus . the ionised gas has three kinematic components : ( 1 ) one observed at the systemic velocity and interpreted as originating in the galaxy disk ; ( 2 ) one outflowing along the bi - cone , with... | we have used the gemini near - infrared integral field spectrograph ( nifs ) to map the gas kinematics of the inner 200pc of the seyfert galaxy ngc4151 in the z , j , h and k bands at a resolving power and spatial resolution ofpc . the ionised gas emission is most extended along the known ionisation bi - cone at positi... |
0806.4635 | c | in this paper , we have presented the results of our multi - epoch phase - referencing observations with vera over 18 months of an h@xmath0o maser source in the galactic star - forming region ngc 281 west , associated with a fragmenting superbubble @xmath196 pc above the perseus spiral arm . the primary results are ... | we have used the japanese vlbi array vera to perform high - precision astrometry of an ho maser source in the galactic star - forming region ngc 281 west , which has been considered to be part of a 300-pc superbubble . we successfully detected a trigonometric parallax of 0.355.030 mas , corresponding to a source dis... | we have used the japanese vlbi array vera to perform high - precision astrometry of an ho maser source in the galactic star - forming region ngc 281 west , which has been considered to be part of a 300-pc superbubble . we successfully detected a trigonometric parallax of 0.355.030 mas , corresponding to a source dis... |
astro-ph0412097 | c | objects were identified to be m ( or early l ) dwarf main - sequence stars . two objects were found to be best fit by early l dwarf templates @xcite . both of these objects are red enough to be outside of the color range shown in figures [ vibv ] and [ izvi ] with @xmath48 and @xmath49 . deep infrared observations of t... | the local white dwarf density is computed to be as high as . based on observations taken 73 days apart no high velocity white dwarfs were identified in the hudf , and all four candidates appear more likely to be part of the galactic thick disk . the lack of detected halo white dwarfs implies that , if the dark matter h... | we identified unresolved source candidates in the hubble ultra deep field , down to . unresolved objects were identified using a parameter , which measures the deviation from the curve - of - growth of a point source . extensive testing of this parameter was carried out , including the effects of decreasing signal - to... |
astro-ph0412097 | c | a systematic search for unresolved objects in the hudf identified objects with @xmath110 mag . using the grapes spectra of these objects , objects with @xmath28 mag were spectroscopically identified , including m and later dwarfs ( including 2 unconfirmed l dwarf candidates ) , and qsos . the m dwarf luminosity functio... | we identified unresolved source candidates in the hubble ultra deep field , down to . low resolution grism spectra of the objects brighter than identify m and later stellar type dwarfs , 2 candidate l - dwarfs , qsos , and 4 white dwarfs . using the observed population of dwarfs with spectral type m4 or later , we deri... | we identified unresolved source candidates in the hubble ultra deep field , down to . unresolved objects were identified using a parameter , which measures the deviation from the curve - of - growth of a point source . extensive testing of this parameter was carried out , including the effects of decreasing signal - to... |
1301.1135 | c | from our knowledge , the model we developed in this paper is the first model that accounts for both stylized facts of market prices microstructure ( including random time arrival of price moves , discrete price grid , high frequency mean reversion , correlation functions behavior at various time scales ) and the styliz... | we introduce a multivariate hawkes process that accounts for the dynamics of market prices through the impact of market order arrivals at microstructural level . it allows one to account for both stylized facts of market prices microstructure ( including random time arrival of price moves , discrete price grid , high f... | we introduce a multivariate hawkes process that accounts for the dynamics of market prices through the impact of market order arrivals at microstructural level . our model is a point process mainly characterized by 4 kernels associated with respectively the trade arrival self - excitation , the price changes mean rever... |
cond-mat0203232 | r | evolving random graphs have recently attracted attention , see e.g. refs @xcite and references therein . this interest is mainly motivated by concrete problems related to the structure of communication or biological networks . experimental data are now available in many contexts @xcite . in these examples , the asym... | we introduce a new oriented evolving graph model inspired by biological networks . a node is added at each time step and is connected to the rest of the graph by random oriented edges emerging from older nodes . the distribution of component sizes decreases algebraically with a continuously varying exponent depending o... | we introduce a new oriented evolving graph model inspired by biological networks . a node is added at each time step and is connected to the rest of the graph by random oriented edges emerging from older nodes . this leads to a statistical asymmetry between incoming and outgoing edges . we show that the model exhibits ... |
1605.03462 | i | hydrodynamical simulations of structure formation have convincingly demonstrated that the forest is an excellent probe of the underlying dark matter distribution , tracing the cosmic web of large scale structure on scales @xmath9@xmath10 comoving mpc ( cmpc ) along the line of sight @xcite . detailed comparison of inte... | these are performed in volumes comoving , span almost four orders of magnitude in mass resolution with up to 17.2 billion particles , and employ a variety of physics variations including warm dark matter and galactic outflows . an uncertain correction for continuum placement bias is required to match the distribution a... | we introduce a new set of large scale , high resolution hydrodynamical simulations of the intergalactic medium : the sherwood simulation suite . these are performed in volumes comoving , span almost four orders of magnitude in mass resolution with up to 17.2 billion particles , and employ a variety of physics variation... |
1605.03462 | c | in this work we introduce a new set of large scale , high resolution hydrodynamical simulations of the igm the sherwood simulation suite . we perform a detailed comparison to high resolution ( @xmath196 ) , high signal - to - noise ( @xmath197 ) observations of the forest over the redshift range @xmath3 . our conclusi... | we introduce a new set of large scale , high resolution hydrodynamical simulations of the intergalactic medium : the sherwood simulation suite . we undertake a detailed comparison of the simulations to high resolution , high signal - to - noise observations of the forest over the redshift range . the simulations are in... | we introduce a new set of large scale , high resolution hydrodynamical simulations of the intergalactic medium : the sherwood simulation suite . these are performed in volumes comoving , span almost four orders of magnitude in mass resolution with up to 17.2 billion particles , and employ a variety of physics variation... |
0904.0505 | i | experiments on , where @xmath7 is na , rb , or k , show a wide range of strongly correlated phases.@xcite , in particular , has attracted much attention following the discovery of superconductivity when water is intercalated into the system.@xcite the phase diagram , with doping @xmath8 , shows many interesting phases,... | we study the paramagnetic phases of this theory at three quarters filling , where it is a model of , , and . we compare our results with exact diagonalisation calculations and experiments on , and discuss the relevance of our results to and . we propose a resolution of seemingly contradictory experimental results on . ... | we introduce a strongly correlated mean - field theory of the ionic hubbard model on the triangular lattice with alternating stripes of site energy using barnes - coleman slave bosons . we study the paramagnetic phases of this theory at three quarters filling , where it is a model of , , and . this theory has two bands... |
0904.0505 | i | we have presented a mean - field slave boson theory of the ionic hubbard model on the triangular lattice with alternating stripes of site energy . this model has two bands : one of which is weakly correlated and nearly filled or filled , the other is nearly half - filled or half - filled and hence strongly correlated .... | we introduce a strongly correlated mean - field theory of the ionic hubbard model on the triangular lattice with alternating stripes of site energy using barnes - coleman slave bosons . this theory has two bands of fermionic quasi - particles : one of which is filled or nearly filled and hence weakly correlated ; the o... | we introduce a strongly correlated mean - field theory of the ionic hubbard model on the triangular lattice with alternating stripes of site energy using barnes - coleman slave bosons . we study the paramagnetic phases of this theory at three quarters filling , where it is a model of , , and . this theory has two bands... |
1105.3388 | i | in the today s world full of crypto algorithms , one may wonder what makes a block cipher attractive . in the authors opinion , the answer to the question is one word : elegance . if something looks nice , then there is a big chance that it is also good . an elegant specification makes it easier to memorize . memora... | the skipjack s internal 4-round feistel structure is replaced with a-bit , 2-round cascade of a binary operation that permutes a text word under control of a key word . the operation , similarly to the multiplication in idea , bases on an algebraic group over-bit words , so it is also capable of decrypting by means of ... | we introduce nsabc/ nice - structured algebraic block cipher using-bit word arithmetic , a-bit analogous of skipjack with-bit key . the skipjack s internal 4-round feistel structure is replaced with a-bit , 2-round cascade of a binary operation that permutes a text word under control of a key word . the operation , sim... |
1112.1469 | i | quantum theory is generally formulated relative to a given causal structure . this is the case both in quantum field theory , where the spacetime metric is given from the beginning , and in the operational framework of quantum information , where protocols and computations consist in sequences of operations performed a... | we introduce the study of quantum protocols that probabilistically simulate quantum channels from a sender in the future to a receiver in the past . we illustrate this dependence in several examples , including ideal classical and quantum channels , measure - and - prepare channels , partial trace channels , and univer... | we introduce the study of quantum protocols that probabilistically simulate quantum channels from a sender in the future to a receiver in the past . the maximum probability of simulation is determined by causality and depends on the amount and type ( classical or quantum ) of information that the channel can transmit .... |
1406.0767 | i | consider the following situation . alice writes a message to bob consisting of the numbers of several bank accounts to which bob has to send some money . she writes in a hurry ( she just got to know that the transfers are urgent if they do not want to pay delay punishment , but currently she has little time ) . therefo... | this scenario leads to the definition of a digraph parameter that generalizes witsenhausen s zero - error rate for directed graphs . we investigate this new parameter for some specific directed graphs and explore its relations to other digraph parameters like sperner capacity and dichromatic number . keywords : zero... | we investigate a communication setup where a source output is sent through a free noisy channel first and an additional codeword is sent through a noiseless but expensive channel later . with the help of the second message the decoder should be able to decide with zero - error whether its decoding of the first message ... |
1401.4702 | i | dispersive coupling of a quantum system to a mechanical or electromagnetic cavity mode has been attracting much attention recently . the coupling provides a means for quantum nondemolition measurement of the occupation number of the mode or of the populations in the energy levels of the system @xcite . the underlying r... | we focus on the regime where the relaxation rate of the system greatly exceeds that of the mode , and develop a quantum adiabatic approach for analyzing the dynamics . semiclassically , the dispersive coupling leads to a mutual tuning of the mode and system into and out of resonance with their modulating fields , leadi... | we investigate a resonantly modulated harmonic mode , dispersively coupled to a nonequilibrium few - level quantum system . we focus on the regime where the relaxation rate of the system greatly exceeds that of the mode , and develop a quantum adiabatic approach for analyzing the dynamics . semiclassically , the disper... |
0706.0211 | m | the context for our study is the model of the spatial distribution of massive halos and the galaxies that inhabit them provided by the millennium simulation @xcite . this is a collisionless dark matter simulation performed in a periodic cube @xmath20mpc ( comoving ) on a side , using @xmath21 particles for a cosmology ... | we investigate halo mass selection properties of red - sequence cluster finders using galaxy populations of the millennium simulation ( ms ) . a clear red sequence exists for ms galaxies in massive halos at redshifts , and we use this knowledge to inform a cluster - finding algorithm applied to projections of the simul... | we investigate halo mass selection properties of red - sequence cluster finders using galaxy populations of the millennium simulation ( ms ) . a clear red sequence exists for ms galaxies in massive halos at redshifts , and we use this knowledge to inform a cluster - finding algorithm applied to projections of the simul... |
0706.0211 | r | an ideal cluster catalog would be _ pure _ , _ complete _ and _ unbiased _ with respect to halos . a perfectly _ pure _ sample would have no accidental projections ; all the galaxies of any chosen cluster would be common members of a single , dark matter halo . a perfectly _ complete _ sample would be one for which eac... | the fraction of blends increases to , as weaker redshift evolution in observed color extends the comoving length probed by a fixed range of color . other factors contributing to the increased blending at high- include broadening of the red sequence and confusion from a larger number of intermediate mass halos hosting b... | we investigate halo mass selection properties of red - sequence cluster finders using galaxy populations of the millennium simulation ( ms ) . a clear red sequence exists for ms galaxies in massive halos at redshifts , and we use this knowledge to inform a cluster - finding algorithm applied to projections of the simul... |
0706.0211 | c | with the advent of wide field imagers , optical searches have become a powerful way to compile large samples of high redshift clusters . key to these techniques is the use of multi - color information to reduce the line - of - sight contamination that plagued earlier , single filter , observations @xcite . two - filter... | our method produces catalogs of cluster candidates whose halo mass selection function , , is characterized by a bimodal log - normal model with a dominant component that reproduces well the real - space distribution , and a redshift - dependent tail that is broader and displaced by a factor lower in mass . we discuss i... | we investigate halo mass selection properties of red - sequence cluster finders using galaxy populations of the millennium simulation ( ms ) . a clear red sequence exists for ms galaxies in massive halos at redshifts , and we use this knowledge to inform a cluster - finding algorithm applied to projections of the simul... |
cond-mat0604238 | c | we summarize our key results concerning the stability of stripe phases in the nickelates . we investigated this problem using two hubbard models the realistic model for @xmath0 electrons , and the ddh model which frequently serves as the simplest approach to the orbital degeneracy . @xcite it is quite encouraging that... | in contrast , for the doubly degenerate hubbard model the most stable stripes are somewhat reminiscent of the cuprates , with half - filled atoms at the domain wall sites . this difference elucidates the crucial role of the off - diagonal hopping terms for the stripe formation in lasrnio . | we investigate the electron density distribution and the stability of stripe phases in the realistic two - band model with hopping elements between orbitals at ni sites on the square lattice , and compare these results with those obtained for the doubly degenerate hubbard model with two equivalent orbitals and diagonal... |
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