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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...