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1411.3054 | c | we have described the theory of a previously unstudied form of the josephson interference effect that can occur in nanoscale @xmath0 junctions due to the coupling of the orbital angular momentum of transverse electronic subbands with an axial magnetic flux . we found in section [ sec : effect_of_length ] the regimes in... | numerical calculations of the critical current versus axial field reveal flux - aperiodic oscillations that we identify as a novel form of josephson interference due to this orbital subband effect . this behavior is studied as a function of junction length and chemical potential . finally , we discuss extensions to the... | a semiconductor nanowire based superconductor - normal - superconductor ( ) junction is modeled theoretically . a magnetic field is applied along the nanowire axis , parallel to the current . the bogoliubov - de gennes equations for andreev bound states are solved while considering the electronic subbands due to radial... |
astro-ph9705057 | i | when galaxies formed and how they evolved are among the central issues of cosmology today . the traditional clue to this problem has been provided by the number count of galaxies as a function of apparent magnitude . early observations in the blue band showed that the number of galaxies per unit angular area increases ... | a simple quantitative model is presented for the history of galaxies to explain galaxy number counts , redshift distributions and some other related observations . we first infer that irregular galaxies and the disks of spiral galaxies are young , probably formed at from a simultaneous consideration of colours and gas ... | a simple quantitative model is presented for the history of galaxies to explain galaxy number counts , redshift distributions and some other related observations . we first infer that irregular galaxies and the disks of spiral galaxies are young , probably formed at from a simultaneous consideration of colours and gas ... |
0705.2707 | i | since tubules were fabricated successfully from chiral lipid molecules , chiral lipid structures have attracted much experimental attention @xcite . most of chiral structures in experiments are self - assembled from dc@xmath3 which is a typical chiral molecule . et al . _ have observed that the spherical vesicles in so... | a theory of chiral lipid membranes is proposed on the basis of a concise free energy density which includes the contributions of the bending and the surface tension of membranes , as well as the chirality and orientational variation of tilting molecules . this theory is consistent with the previous experiments [ j.m . ... | a theory of chiral lipid membranes is proposed on the basis of a concise free energy density which includes the contributions of the bending and the surface tension of membranes , as well as the chirality and orientational variation of tilting molecules . this theory is consistent with the previous experiments [ j.m . ... |
0705.2707 | c | in this paper , we have focused on a concise free energy from which the euler - lagrange equations of clms without free edges and euler - lagrange equations as well as boundary conditions of clms with free edges can be derived analytically . their implications for extant and future experiments can be summarized as foll... | the pitch angles of helical ripples are theoretically estimated to be about 0 and 35 , which are close to the most frequent values 5 and 28 observed in the experiment [ n. mahajan _ the ratio between the width and pitch of twisted ribbons is predicted to be proportional to the relative concentration difference of left-... | a theory of chiral lipid membranes is proposed on the basis of a concise free energy density which includes the contributions of the bending and the surface tension of membranes , as well as the chirality and orientational variation of tilting molecules . this theory is consistent with the previous experiments [ j.m . ... |
1303.0944 | i | a possible approach for dealing with the intractability of a given decision or optimization problem is to identify restrictions on input instances under which the problem can still be solved efficiently . one generic framework for describing a kind of such restrictions in case of graph problems is the following : given... | a total dominating set in a graph is a set of vertices such that every vertex of the graph has a neighbor in the set . we introduce and study graphs that admit non - negative real weights associated to their vertices such that a set of vertices is a total dominating set if and only if the sum of the corresponding weigh... | a total dominating set in a graph is a set of vertices such that every vertex of the graph has a neighbor in the set . we introduce and study graphs that admit non - negative real weights associated to their vertices such that a set of vertices is a total dominating set if and only if the sum of the corresponding weigh... |
1612.03355 | i | no - slip billiard systems have received so far very little attention despite some interesting features that distinguish them from the much more widely studied standard billiards . these non - standard types of billiards are discrete time systems in dimension @xmath2 ( after taking the natural poincar section of a flow... | _ this leads to the study of _ no - slip billiards_planar billiard systems in which the moving particle is a disc ( with rotationally symmetric mass distribution ) whose translational and rotational velocities can both change at each collision with the boundary of the billiard domain . in this paper we greatly exten... | abstract rigid bodies collision maps in dimension two , under a natural set of physical requirements , can be classified into two types : the standard specular reflection map and a second which we call , after broomhead and gutkin , _ no - slip . _ this leads to the study of _ no - slip billiards_planar billiard sys... |
0910.4172 | i | a _ convex body _ is a compact convex set in @xmath3 with nonempty interior . let @xmath1 be a family of convex bodies . the _ packing number _ @xmath7 is the maximum cardinality of a set of pairwise - disjoint convex bodies in @xmath1 , and the _ transversal number _ @xmath0 is the minimum cardinality of a set of poin... | according to a classical result of grnbaum , the transversal number of any family of pairwise - intersecting translates or homothets of a convex body in is bounded by a function of . denote by ( resp . ) the supremum of the ratio of the transversal number to the packing number over all families of translates ( resp .... | according to a classical result of grnbaum , the transversal number of any family of pairwise - intersecting translates or homothets of a convex body in is bounded by a function of . denote by ( resp . ) the supremum of the ratio of the transversal number to the packing number over all families of translates ( resp .... |
0910.3085 | c | we have presented several methods to encode sets of finite vertices as single vertices . in the first part , we used depth - first spanning trees to encode edges by vertices . as an application we were able to extend courcelle s result on the collapse of @xmath1 to @xmath2 on sparse hypergraphs from countable hypergrap... | according to a theorem of courcelle monadic second - order logic and guarded second - order logic ( where one can also quantify over sets of edges ) have the same expressive power over the class of all countable-sparse hypergraphs . in the first part of the present paper we extend this result to hypergraphs of arbitrar... | according to a theorem of courcelle monadic second - order logic and guarded second - order logic ( where one can also quantify over sets of edges ) have the same expressive power over the class of all countable-sparse hypergraphs . in the first part of the present paper we extend this result to hypergraphs of arbitrar... |
1508.05240 | c | in this paper , we have presented new alma observations of the four brightest stars in the globular cluster 47 tucanae , examining the co @xmath97 transitions . no source was detected . having modelled the interaction between the isrf and the circumstellar enviroment , we expect that the co line fluxes from the giant s... | alma observations show a non - detection of carbon monoxide around the four most luminous asymptotic giant branch ( agb ) stars in the globular cluster 47 tucanae . we estimate that the co envelopes will be truncated at a few hundred stellar radii from their host stars and that the line intensities are about two orders... | alma observations show a non - detection of carbon monoxide around the four most luminous asymptotic giant branch ( agb ) stars in the globular cluster 47 tucanae . stellar evolution models and star counts show that the mass - loss rates from these stars should be.23.5 10 m yr . we would navely expect such stars to be ... |
1302.0983 | i | silicon is at the heart of all modern microelectronics . its properties have allowed the semiconductor industry to follow moore s law for nearly half a century , delivering nowadays billions of nanometre - scale transistors per chip . remarkably , silicon is also an ideal material to manipulate quantum information enco... | here we demonstrate that valley separation can be accurately tuned via electrostatic gate control in a metal - oxide - semiconductor quantum dot , providing splittings spanning 0.3 - 0.8 mev . the splitting varies linearly with applied electric field , with a ratio in agreement with atomistic tight - binding prediction... | although silicon is a promising material for quantum computation , the degeneracy of the conduction band minima ( valleys ) must be lifted with a splitting sufficient to ensure formation of well - defined and long - lived spin qubits . here we demonstrate that valley separation can be accurately tuned via electrostatic... |
1610.04741 | i | in a _ geometric drawing of a graph @xmath0 _ , the vertices of @xmath0 are represented by distinct points in the plane and each edge @xmath10 of @xmath0 is represented by the line segment between the pair of points that represent the vertices of @xmath10 . as usual , we identify the vertices and their images , as well... | an _ obstacle representation _ of a graph is a set of points in the plane representing the vertices of , together with a set of polygonal obstacles such that two vertices of are connected by an edge in if and only if the line segment between the corresponding points avoids all the obstacles . the _ obstacle number of ... | an _ obstacle representation _ of a graph is a set of points in the plane representing the vertices of , together with a set of polygonal obstacles such that two vertices of are connected by an edge in if and only if the line segment between the corresponding points avoids all the obstacles . the _ obstacle number of ... |
1609.00094 | i | a fundamental challenge in studying complex networked systems is to reveal the interplay between network topology and functionality@xcite . here we tackle this challenge by investigating a classical notion in graph theory , i.e. articulation points . a node in a network is an articulation point ( ap ) if its removal di... | an articulation point in a network is a node whose removal disconnects the network . those nodes play key roles in ensuring connectivity of many real - world networks , from infrastructure networks to protein interaction networks and terrorist communication networks . despite their fundamental importance , a general fr... | an articulation point in a network is a node whose removal disconnects the network . those nodes play key roles in ensuring connectivity of many real - world networks , from infrastructure networks to protein interaction networks and terrorist communication networks . despite their fundamental importance , a general fr... |
1412.1958 | i | it has long been known that general relativity and electrodynamics exhibit certain formal similarities , see matte @xcite and bel @xcite , or for a more recent overview costa and natrio @xcite . on the other hand , petrov type d spacetimes can be thought of as spacetimes with coulomb - like sources , as already point... | robinson 3-form , from which the bel we also determine the kummer tensor , a tensor cubic in curvature , for a general type d solution for the first time , and calculate the pieces of its irreducible decomposition . the calculations are carried out in two coordinate systems : in the original polynomial pd coordinat... | analogies between gravitation and electromagnetism have been known since the 1950s . here , we examine a fairly general type d solution the exact seven parameter solution of plebaski demiaski ( pd)to demonstrate these analogies for a physically meaningful spacetime : the two quadratic curvature invariants and are ... |
1412.1958 | c | in this paper , we have used the plebaski demiaski solution of general relativity to show that the formal analogy of invariants in general relativity and electrodynamics can be understood in a physical sense : the electric field @xmath202 ( charges ) corresponds to the mass parameter @xmath116 ( gravitational charge )... | analogies between gravitation and electromagnetism have been known since the 1950s . here , we examine a fairly general type d solution the exact seven parameter solution of plebaski demiaski ( pd)to demonstrate these analogies for a physically meaningful spacetime : the two quadratic curvature invariants and are ... | analogies between gravitation and electromagnetism have been known since the 1950s . here , we examine a fairly general type d solution the exact seven parameter solution of plebaski demiaski ( pd)to demonstrate these analogies for a physically meaningful spacetime : the two quadratic curvature invariants and are ... |
1611.08349 | i | we continue a study ( @xcite ; article i ) on the 26 december 2001 event ( sol2001 - 12 - 26 ) . this solar eruptive - flare event produced a strong flux of solar energetic particles ( seps , mainly protons ) near earth and a 63rd ground - level enhancement of cosmic - ray intensity ( gle63 ) . gles represent the high... | analysis of the observations of the sol2001 - 12 - 26 event related to ground - level - event gle63 , including microwave spectra and images from the _ nobeyama radioheliograph _ at 17 and 34ghz , _ siberian solar radio telescope _ at 5.7ghz , and _ transition region and coronal explorer _ in 1600 has led to the follo... | analysis of the observations of the sol2001 - 12 - 26 event related to ground - level - event gle63 , including microwave spectra and images from the _ nobeyama radioheliograph _ at 17 and 34ghz , _ siberian solar radio telescope _ at 5.7ghz , and _ transition region and coronal explorer _ in 1600 has led to the follo... |
1611.08349 | c | analysis of the microwave and uv images has shown that each of the two microwave sources observed at 5.7 , 17 , and 34ghz was associated with one of the two ribbons located in opposite - polarity magnetic fields . the appearance of each microwave source corresponds to the whole related ribbon , as if it had been viewed... | atypical were : i ) long duration of the flare of more than one hour ; ii ) moderate intensity of a microwave burst , aboutsfu ; iii ) low peak frequency of the gyrosynchrotron spectrum , around 6ghz ; and its insensitivity to the flux increase by more than one order of magnitude . comparison of the 17ghz and 1600 ... | analysis of the observations of the sol2001 - 12 - 26 event related to ground - level - event gle63 , including microwave spectra and images from the _ nobeyama radioheliograph _ at 17 and 34ghz , _ siberian solar radio telescope _ at 5.7ghz , and _ transition region and coronal explorer _ in 1600 has led to the follo... |
1008.0554 | i | there are more and more astrophysical observations justifying the existence of extremely compact massive objects with size close to their schwarzschild radius @xcite . it is widely accepted that these observations also provide indirect justifications of the existence of black holes ( bhs ) . nevertheless , there are al... | as a preparation for the dynamical investigations , this paper begins with a short review of the three - layer gravastar model with distinguished attention to the structure of the pertinent parameter space of gravastars in equilibrium . then the radial stability of these types of gravastars is studied by determining th... | as a preparation for the dynamical investigations , this paper begins with a short review of the three - layer gravastar model with distinguished attention to the structure of the pertinent parameter space of gravastars in equilibrium . then the radial stability of these types of gravastars is studied by determining th... |
1008.0554 | r | by inspection of the new effective potential the dynamics of the gravastar can be determined . if the new potential possesses the form of graph 2 of figure [ figure1 ] the motion of the gravastar surface remains bounded and we can determine the minimum and maximum value of the radius . in particular , the maximum mass ... | while in the analytic setup the equation of state is kept to be generic , in the numerical investigations three functionally distinct classes of equations of states are applied . in the corresponding particular cases the maximal mass of the dust shell that may fall onto a gravastar without converting it into a black ho... | as a preparation for the dynamical investigations , this paper begins with a short review of the three - layer gravastar model with distinguished attention to the structure of the pertinent parameter space of gravastars in equilibrium . then the radial stability of these types of gravastars is studied by determining th... |
1103.4003 | i | we start the introduction by considering the following views of great men : @xmath0``although nobody is in doubt today of the validity of the remarkable interpretation of thermodynamics with which statistical mechanics , following the efforts of boltzmann and gibbs , has recently provided us , it still remains extremel... | as the title says we want to answer the question ; how and why does statistical mechanics work ? as we know from the most used prescription of gibbs we calculate the phase space averages of dynamical quantities and we find that these phase averages agree very well with experiments . clearly actual experiments are not d... | as the title says we want to answer the question ; how and why does statistical mechanics work ? as we know from the most used prescription of gibbs we calculate the phase space averages of dynamical quantities and we find that these phase averages agree very well with experiments . clearly actual experiments are not d... |
cond-mat0612361 | i | most of the current experiments involving trapped atomic fermi gases focus on the bec - bcs crossover . by changing the magnetic field around a feshbach resonance , the scattering length @xmath0 of the atoms can be varied from small positive values through very large values near the resonance to small negative values .... | at finite temperature , the hydrodynamic collective modes of superfluid trapped fermi gases are coupled to the motion of the normal component , which in the bcs limit behaves like a collisionless normal fermi gas . the coupling between the superfluid and the normal components is treated in the framework of a semiclassi... | at finite temperature , the hydrodynamic collective modes of superfluid trapped fermi gases are coupled to the motion of the normal component , which in the bcs limit behaves like a collisionless normal fermi gas . the coupling between the superfluid and the normal components is treated in the framework of a semiclassi... |
1312.6925 | i | the scissors mode , which is a rotational mode of isovector character in deformed nuclei@xcite , is usually visualized by an out of phase orbital motion of protons against neutrons . this intuitive picture lead to the prediction of the scissors mode both in terms of nucleonic@xcite and bosonic@xcite degrees of freedom ... | background : : : the scissors mode is a rotational mode of isovector character in deformed nuclei . together with the isoscalar rotation , it is the prominent collective mode at low excitation energies . special emphasis is put on the coupling of the spin part of the m1 operator to the scissors mode . metho... | background : : : the scissors mode is a rotational mode of isovector character in deformed nuclei . together with the isoscalar rotation , it is the prominent collective mode at low excitation energies . purpose : : : we use a simple field theory model to investigate the role of the nucleon spin for the ... |
hep-ph9604416 | i | even though qcd yields a remarkably good description of the strong interaction , the low energy hadron physics has to be modelled phenomenologically . this is due to the fact that the usual perturbative approach in the coupling constant can not be applied to qcd below energies of the order of 1 gev . most of the phenom... | numerically , we find that this unitarization technique yields the correct complex analytic structure in terms of cuts and poles . indeed , using the chiral parameter estimates obtained from low energy experiments we obtain the poles associated with the and resonances . we have obtained the chiral parameters and scatte... | based on a dispersive approach , we apply the inverse amplitude method to unitarize one - loop and chiral perturbation theory . numerically , we find that this unitarization technique yields the correct complex analytic structure in terms of cuts and poles . indeed , using the chiral parameter estimates obtained from l... |
hep-ph9604416 | m | let us briefly review the standard derivation @xcite of the inverse amplitude method , since we will use it later in order to understand the applicability of the method . any partial wave obtained from a relativistic quantum field theory should present a characteristic analytic structure in the complex @xmath42 plane .... | based on a dispersive approach , we apply the inverse amplitude method to unitarize one - loop and chiral perturbation theory . pacs : 14.40.aq , 14.40.cs,11.80.et,13.75.lb 6.5 in 8.5 in epsf lbl-38645 ucm - ft 3/96 april 1996 revised nov96 to appear in : prd 1-sept-97 * the inverse amplitude me... | based on a dispersive approach , we apply the inverse amplitude method to unitarize one - loop and chiral perturbation theory . numerically , we find that this unitarization technique yields the correct complex analytic structure in terms of cuts and poles . indeed , using the chiral parameter estimates obtained from l... |
cond-mat0211615 | i | the pyrochlores with the chemical formula @xmath0mo@xmath1o@xmath2 ( @xmath3 being the divalent element ) exhibit a number of interesting and not completely understood phenomena,@xcite which present the main motivation for the analysis of electronic and magnetic structure of these compounds , which we undertake in this... | the coulomb repulsion plays a very important role in the problem , and the semi - empirical value- ev accounts simultaneously for the metal - insulator ( m - i ) transition , the ferromagnetic ( fm ) - spin - glass ( sg ) transition , and for the observed enhancement of the anomalous hall effect ( ahe ) . the m - i tra... | being motivated by recent experimental studies , we investigate magnetic structures of the mo pyrochloresmoo ( y , nd , and gd ) and their impact on the electronic properties . the latter are closely related with the behavior of twelve mo( ) bands , located near the fermi level and well separated from the rest of the s... |
cond-mat0211615 | i | we have presented results of model hf calculations for pyrochlores @xmath0mo@xmath1o@xmath2 ( @xmath3@xmath4 y , gd , and nd ) . the model combines details of lda electronic structure for the mo(@xmath5 ) bands located near the fermi level , the spin - orbit interaction , and the on - site coulomb interactions amongst ... | we use a mean - field hartree - fock approach , which combines fine details of the electronic structure for these bands , extracted from the conventional calculations in the local - density approximation , the spin - orbit interaction , and the on - site coulomb interactions amongst the mo( ) electrons , treated in the... | being motivated by recent experimental studies , we investigate magnetic structures of the mo pyrochloresmoo ( y , nd , and gd ) and their impact on the electronic properties . the latter are closely related with the behavior of twelve mo( ) bands , located near the fermi level and well separated from the rest of the s... |
1005.1312 | i | the principal results of this paper are as follows . assuming only a _ large scale _ anisotropic distribution of crs ( generated , for example by a nearby accelerator , such as a snr ) and a @xcite ( gs ) cascade of alfvenic turbulence originating from some scale @xmath1 , which is the longest scale relevant for the wa... | both the acceleration of cosmic rays ( cr ) in supernova remnant shocks and their subsequent propagation through the random magnetic field of the galaxy deem to result in an almost isotropic cr spectrum . the key assumption is that crs are scattered by a strongly anisotropic alfven wave spectrum formed by the turbulent... | both the acceleration of cosmic rays ( cr ) in supernova remnant shocks and their subsequent propagation through the random magnetic field of the galaxy deem to result in an almost isotropic cr spectrum . yet the milagro tev observatory discovered a sharp ( arrival anisotropy of cr nuclei . we suggest a mechanism for p... |
gr-qc0002092 | i | this article presents the calculation , using continuum and lattice methods , of boundary terms in 3-dimensional gravity . the gravity theory is presented in first order palatini form , this being a particular example of the general class of bf models @xcite as this is the most convenient presentation for deriving the ... | boundary actions for three - dimensional quantum gravity in the discretized formalism of ponzano - regge are studied with a view towards understanding the boundary degrees of freedom . these degrees of freedom postulated in the holography hypothesis are supposed to be characteristic of quantum gravity theories . in par... | boundary actions for three - dimensional quantum gravity in the discretized formalism of ponzano - regge are studied with a view towards understanding the boundary degrees of freedom . these degrees of freedom postulated in the holography hypothesis are supposed to be characteristic of quantum gravity theories . in par... |
1211.5799 | i | during last decades , the interest in diffusive processes has grown tremendously because of their universality in diverse physical areas ; ranging from condensed matter to elementary particle physics and gravitation @xcite . in particular , it has emerged an intense activity in the study of brownian motion in curved ma... | brownian motion of free particles on curved surfaces is studied by means of the langevin equation written in riemann normal coordinates . in the diffusive regime we find the same physical behavior as the one described by the diffusion equation on curved manifolds [ j. stat . our findings are corroborated by means of br... | brownian motion of free particles on curved surfaces is studied by means of the langevin equation written in riemann normal coordinates . in the diffusive regime we find the same physical behavior as the one described by the diffusion equation on curved manifolds [ j. stat . mech . ( 2010 ) p08006 ] . therefore , we us... |
1403.7007 | i | the demand for high - definition video streaming services such as youtube and netflix is driving the rapid growth of internet traffic . in order to mitigate the effect of this increased load on the underlying communication infrastructure , content delivery networks deploy storage memories or caches throughout the netwo... | caching of popular content during off - peak hours is a strategy to reduce network loads during peak hours . recent work has shown significant benefits of designing such caching strategies not only to deliver part of the content locally , but also to provide coded multicasting opportunities even among users with differ... | caching of popular content during off - peak hours is a strategy to reduce network loads during peak hours . recent work has shown significant benefits of designing such caching strategies not only to deliver part of the content locally , but also to provide coded multicasting opportunities even among users with differ... |
1305.4685 | i | this account of physics starts by considering _ configuration space _ @xmath1 , i.e. the space of all possible configurations @xmath2 that a physical system can take . in ordinary mechanics , the configurations are particle positions @xcite . in field theories they are the values taken by the field on a fixed spatial s... | i provide perturbative schemes for these in which the timefunction is to be determined rather than assumed . this paper is useful modelling as regards the halliwell hawking arena for the quantum origin of the inhomogeneous cosmological fluctuations . * edward anderson * pacs : 04.60kz , 04.20.cv . ea212@cam.... | classical and semiclassical schemes are presented that are timeless at the primary level and recover time from mach s ` time is to be abstracted from change ' principle at the emergent secondary level . the semiclassical scheme is a machian variant of the semiclassical approach to the problem of time in quantum gravity... |
1305.4685 | c | classical and semiclassical schemes are presented that are timeless at the primary level and recover time from mach s ` time is to be abstracted form change ' principle at the emergent secondary level . this paper considers this for relational particle mechanics ( rpm ) model arenas . see @xcite for the minisuperspace ... | classical and semiclassical schemes are presented that are timeless at the primary level and recover time from mach s ` time is to be abstracted from change ' principle at the emergent secondary level . the semiclassical scheme is a machian variant of the semiclassical approach to the problem of time in quantum gravity... | classical and semiclassical schemes are presented that are timeless at the primary level and recover time from mach s ` time is to be abstracted from change ' principle at the emergent secondary level . the semiclassical scheme is a machian variant of the semiclassical approach to the problem of time in quantum gravity... |
1702.08234 | i | * the rise of cloud apps : * + the popularity of consumer cloud storage providers ( csps ) over the previous decade has been on a roll . dropbox , google drive , and one drive have each amassed hundreds of millions of users . in order to further appeal to their users , the csps have been transitioning from being pure _... | such apps often request full access to users files , including files shared with collaborators . hence , whenever a user grants access to a new vendor , she is inflicting a privacy loss on herself and on her collaborators too . based on analyzing a real dataset of 183 google drive users and 131 third party apps , we di... | cloud storage services , like dropbox and google drive , have growing ecosystems of 3rd party apps that are designed to work with users cloud files . such apps often request full access to users files , including files shared with collaborators . hence , whenever a user grants access to a new vendor , she is inflicting... |
0902.2881 | i | the most popular model for the central engines of long gamma - ray - burst ( grb ) jets is based on the `` failed supernova '' scenario of stellar collapse , or `` collapsar '' , where the iron core of progenitor star forms a bh @xcite . if the specific angular momentum in the equatorial part of progenitor exceeds that... | we explore whether this process can explain the stellar explosions and relativistic jets associated with long gamma - ray - bursts . in however , this energy deficit can be recovered via additional power provided by the disk . black hole physics supernovae : general gamma - rays : bursts methods : numerical mhd ... | collapse of massive stars may result in formation of accreting black holes in their interior . the accreting stellar matter may advect substantial magnetic flux onto the black hole and promote release of its rotational energy via magnetic stresses ( the blandford - znajek mechanism ) . in this paper we explore whether ... |
0902.2881 | c | in this paper we continued our study into the potential of the blandford - znajek mechanism as main driver in the central engines of gamma ray bursts . in particularly , we analysed the conditions for activation of the mechanism in the collapsar model where accumulation of magnetic flux by the central black hole is lik... | particularly , we show that the blandford - znajek mechanism is activated when the rest mass - energy density of matter drops below the energy density of magnetic field in the very vicinity of the black hole ( within its ergosphere ) . we also discuss whether such a strong magnetic field is in conflict with the rapid r... | collapse of massive stars may result in formation of accreting black holes in their interior . the accreting stellar matter may advect substantial magnetic flux onto the black hole and promote release of its rotational energy via magnetic stresses ( the blandford - znajek mechanism ) . in this paper we explore whether ... |
1604.06244 | i | the casimir effect ( for reviews see @xcite ) is among the most interesting boundary - induced effects in quantum field theory . nearly seventy years after its discovery , the effect continues to be area of active theoretical and experimental research today . this is due to of fundamental and practical importance of th... | complete set of cylindrical modes is constructed for the electromagnetic field inside and outside a cylindrical shell in the background of-dimensional ds spacetime . on the shell , the field obeys the generalized perfect conductor boundary condition . for the bunch - davies vacuum state the vacuum energy - momentum ten... | complete set of cylindrical modes is constructed for the electromagnetic field inside and outside a cylindrical shell in the background of-dimensional ds spacetime . on the shell , the field obeys the generalized perfect conductor boundary condition . for the bunch - davies vacuum state , we evaluate the expectation va... |
1604.06244 | c | in the investigations of the casimir effect the cylindrically symmetric boundaries are among the most popular geometries . in the present paper we have investigated the local casimir densities for the electromagnetic field inside and outside a cylindrical shell in background of @xmath0-dimensional ds spacetime . on the... | , we evaluate the expectation values ( vevs ) of the electric field squared and of the energy - momentum tensor . , the renormalization is reduced to the one for the vevs in the boundary - free ds bulk . as a special case , this flux is directed from the shell in both the exterior and interior regions . for points near... | complete set of cylindrical modes is constructed for the electromagnetic field inside and outside a cylindrical shell in the background of-dimensional ds spacetime . on the shell , the field obeys the generalized perfect conductor boundary condition . for the bunch - davies vacuum state , we evaluate the expectation va... |
0911.1777 | i | a bayesian data analysis specifies joint probability distributions to describe the relationship between the prior information , the model or hypotheses , and the data . using bayes theorem , the posterior distribution is uniquely determined from the conditional probability distribution of the unknowns given the observe... | computation of the marginal likelihood from a simulated posterior distribution is central to bayesian model selection but is computationally difficult . the often - used harmonic mean approximation uses the posterior directly but is unstably sensitive to samples with anomalously small values of the likelihood . the lap... | computation of the marginal likelihood from a simulated posterior distribution is central to bayesian model selection but is computationally difficult . the often - used harmonic mean approximation uses the posterior directly but is unstably sensitive to samples with anomalously small values of the likelihood . the lap... |
cond-mat0004182 | i | theoretical research on electronic properties in mesoscopic condensed matter systems has focussed primarily on the charge degrees of freedom of the electron , while its spin degrees of freedom have not yet received the same attention . however , an increasing number of spin - related experiments @xcite show that the s... | control over electron - spin states , such as coherent manipulation , filtering and measurement promises access to new technologies in conventional as well as in quantum computation and quantum communication . we review our proposal of using electron spins in quantum confined structures as qubits and discuss the requir... | control over electron - spin states , such as coherent manipulation , filtering and measurement promises access to new technologies in conventional as well as in quantum computation and quantum communication . we review our proposal of using electron spins in quantum confined structures as qubits and discuss the requir... |
1405.5311 | i | in recent years there has been a huge explosion in the variety of sensors and the dimensionality of the data produced by these sensors and this has been in a large number of applications ranging from imaging to other scientific applications.the total amount of data produced by the sensors is much more than the availabl... | conventional approaches of sampling signals follow the celebrated theorem of nyquist and shannon . compressive sampling , introduced by donoho , romberg and tao , is a new paradigm that goes against the conventional methods in data acquisition and provides a way of recovering signals using fewer samples than the tradit... | conventional approaches of sampling signals follow the celebrated theorem of nyquist and shannon . compressive sampling , introduced by donoho , romberg and tao , is a new paradigm that goes against the conventional methods in data acquisition and provides a way of recovering signals using fewer samples than the tradit... |
1011.3041 | i | weak gravitational lensing is a powerful technique for studying the distribution of matter in the universe due to its ability to model the matter distribution in foreground structures , independent of the nature of the matter present . as the light from background sources is bent around foreground lenses , the galaxy i... | current theories of structure formation predict specific density profiles of galaxy dark matter haloes , and with weak gravitational lensing we can probe these profiles on several scales . on small scales , higher - order shape distortions known as flexion add significant detail to the weak lensing measurements . [ fir... | current theories of structure formation predict specific density profiles of galaxy dark matter haloes , and with weak gravitational lensing we can probe these profiles on several scales . on small scales , higher - order shape distortions known as flexion add significant detail to the weak lensing measurements . we pr... |
1011.3041 | c | we have shown a significant detection of galaxy - galaxy f flexion for the first time with shapelets using the space - based cosmos data set . we used this flexion signal in conjunction with the shear to constrain the average density profile of the galaxy haloes in our lens sample . we found a power - law profile consi... | we present here the first detection of a galaxy - galaxy flexion signal in space - based data , obtained using a new shapelets pipeline introduced here . we combine this higher - order lensing signal with shear to constrain the average density profile of the galaxy lenses in the hubble space telescope cosmos survey . w... | current theories of structure formation predict specific density profiles of galaxy dark matter haloes , and with weak gravitational lensing we can probe these profiles on several scales . on small scales , higher - order shape distortions known as flexion add significant detail to the weak lensing measurements . we pr... |
astro-ph0512261 | i | in the sections above , we have shown that curves derived as powers of ellipse functions , called p - ellipses , provide simple , yet surprisingly accurate approximations to orbits in a range of power - law potentials , including the well - known logarithmic potential , and softened power - law potentials . for a given... | curves in a family derived from powers of the polar coordinate formula for ellipses are found to provide good fits to bound orbits in a range of power - law potentials . this range includes the well - known ( keplerian ) and logarithmic potentials . the p - ellipses make very useful tools for studying trends among powe... | curves in a family derived from powers of the polar coordinate formula for ellipses are found to provide good fits to bound orbits in a range of power - law potentials . this range includes the well - known ( keplerian ) and logarithmic potentials . these approximate orbits , called p - ellipses , retain some of the ba... |
1508.05245 | c | by exploiting adiabatic elimination techniques , semi - classical methods , and c - mop theory , we have provided a theoretical analysis of the dompo which works even at the critical point . we have focused on the region where the optical field is fully quantum , showing that such a quantum - correlated field with no c... | we introduce a theoretical approach that is capable of describing this regime , even at the critical point itself . we find that the down - converted field can induce significant mechanical cooling and identify the process responsible of this as a cooling - by - heating mechanism . our approach opens the possibility fo... | degenerate optomechanical parametric oscillators are optical resonators in which a mechanical degree of freedom is coupled to a cavity mode that is nonlinearly amplified via parametric down - conversion of an external pumping laser . below a critical pumping power the down - converted field is purely quantum - mechanic... |
1202.6037 | i | diagnostic sonography allows visualization of body tissues , by radiating them with acoustic energy pulses , which are transmitted from an array of transducer elements . the image typically comprises multiple scanlines , each constructed by integrating data collected by the transducers , following the transmission of a... | emerging sonography techniques often require increasing the number of transducer elements involved in the imaging process . consequently , larger amounts of data must be acquired and processed . the significant growth in the amounts of data affects both machinery size and power consumption . within the classical sampli... | emerging sonography techniques often require increasing the number of transducer elements involved in the imaging process . consequently , larger amounts of data must be acquired and processed . the significant growth in the amounts of data affects both machinery size and power consumption . within the classical sampli... |
gr-qc9701059 | i | understanding the origin of the black - hole entropy is one of the most fascinating problems in black - hole physics @xcite . the concept of the black - hole entropy traces back to the work by bekenstein , who pointed out that the behavior of the basic physical quantities describing stationary black holes has an analo... | entanglement entropy is often speculated as a strong candidate for the origin of the black - hole entropy . to judge whether this speculation is true or not , it is effective to investigate the whole structure of thermodynamics obtained from the entanglement entropy , rather than just to examine the apparent structure ... | entanglement entropy is often speculated as a strong candidate for the origin of the black - hole entropy . to judge whether this speculation is true or not , it is effective to investigate the whole structure of thermodynamics obtained from the entanglement entropy , rather than just to examine the apparent structure ... |
1311.3975 | c | through a combination of analytical calculations and quantum monte carlo simulations , we have investigated the behavior of valence bond probability distributions and correlations in ground states of the antiferromagnetic heisenberg model on chain , square and cubic lattices . our analytic results provide a clear groun... | , we study the bipartite valence bond distributions and their correlations within the ground state of the heisenberg antiferromagnet on bipartite lattices . in terms of field theory , a non - linear model analysis reveals that at long distances the probability distribution of valence bond lengths decays as and that val... | every singlet state of a quantum spin- system can be decomposed into a linear combination of valence bond basis states . the range of valence bonds within this linear combination as well as the correlations between them can reveal the nature of the singlet state , and are key ingredients in variational calculations . i... |
1310.1360 | i | the discovery of many extrasolar planets ( exoplanets ) by radial velocity , transit , and imaging techniques has stimulated observational and theoretical studies to characterize their atmospheric chemistry and physical properties and to investigate whether these exoplanets could sustain life forms ( e.g. , * ? ? ? * ;... | since stellar euv fluxes can not now be measured and interstellar neutral hydrogen completely obscures stellar radiation between 40 and 91.2 nm , even for the nearest stars , we must estimate the unobservable euv flux by indirect methods . we provide formulae for predicting euv flux ratios based on the _ euve _ and _ ... | extreme ultraviolet ( euv ) radiations ( 10117 nm ) from host stars play important roles in the ionization , heating , and mass loss from exoplanet atmospheres . together with the host star s ly and far - uv ( 117170 nm ) radiation , euv radiation photodissociates important molecules , thereby changing the chemistry ... |
1310.1360 | c | euv fluxes from host stars control the photochemistry , heating , and mass loss from the outer atmospheres of exoplanets , especially for those exoplanets located close to their host stars . the objective of this study is to develop a useful technique for predicting the euv fluxes of f5m5 dwarf stars , since there are ... | extreme ultraviolet ( euv ) radiations ( 10117 nm ) from host stars play important roles in the ionization , heating , and mass loss from exoplanet atmospheres . together with the host star s ly and far - uv ( 117170 nm ) radiation , euv radiation photodissociates important molecules , thereby changing the chemistry ... | extreme ultraviolet ( euv ) radiations ( 10117 nm ) from host stars play important roles in the ionization , heating , and mass loss from exoplanet atmospheres . together with the host star s ly and far - uv ( 117170 nm ) radiation , euv radiation photodissociates important molecules , thereby changing the chemistry ... |
nucl-th9603008 | c | quasi - potential equations ( qpes ) , despite their success as a basis for hadronic phenomenology , can not be improved upon systematically . this is because whenever they are used beyond first - order they predict amplitudes with unphysical singularities . these singularities also appear whenever attempts are made to... | firstly , a systematic procedure is derived for obtaining three - dimensional bound - state equations from four - dimensional ones . unlike `` quasi - potential approaches '' this procedure does not involve the use of delta - function constraints on the relative four - momentum . in the absence of negative - energy sta... | firstly , a systematic procedure is derived for obtaining three - dimensional bound - state equations from four - dimensional ones . unlike `` quasi - potential approaches '' this procedure does not involve the use of delta - function constraints on the relative four - momentum . in the absence of negative - energy sta... |
1205.5408 | c | in this article we have studied the novel scenario proposed by refs . @xcite where the vacuum expectation values of susy flat directions generate a large mass for gauge bosons and gauginos . due to the large gauge boson masses thermalization is delayed after the end of inflation . in the non - thermal universe gravitin... | flat directions in generic supersymmetric theories can change the thermal history of the universe . a novel scenario was proposed earlier where the vacuum expectation value of the flat directions induces large masses for all the gauge bosons and gauginos . we find that the total gravitino abundance generated is consist... | flat directions in generic supersymmetric theories can change the thermal history of the universe . a novel scenario was proposed earlier where the vacuum expectation value of the flat directions induces large masses for all the gauge bosons and gauginos . this delays the thermalization of the universe after inflation ... |
0905.2215 | c | we expect not only the drinfeld double @xmath2 but also the pair @xmath5 , with @xmath1 being a @xmath2-module algebra , to play a fundamental role on the quantum group side of the logarithmic kazhdan lusztig duality . based on the general recipe in sec . [ sec : thm ] , the contents of sec . [ sec : sl2 ] must have a... | , we work out the case where is the taft hopf algebra related to the quantum group that is kazhdan lusztig - dual to logarithmic conformal models . the corresponding pair is `` truncated '' to , where is a module algebra that turns out to have the form{\otimes}{\mathbb{c}}[\lambda]/(\lambda^{2p}-1)$ ] , where $ ] is t... | for a hopf algebra , we endow the heisenberg double with the structure of a module algebra over the drinfeld double . based on this property , we propose that is to be the counterpart of the algebra of fields on the quantum - group side of the kazhdan lusztig duality between logarithmic conformal field theories and qu... |
quant-ph0309021 | i | in classical mechanics , ensembles , such as the microcanonical and canonical ensembles , are represented by probability distributions on the phase space . in quantum mechanics , ensembles are usually represented by density matrices . it is natural to regard these density matrices as arising from probability distributi... | for a quantum system , a density matrix that is not pure can arise , via averaging , from a distribution of its wave function , a normalized vector belonging to its hilbert space . while itself does not determine a unique , additional facts , such as that the system has come to thermal equilibrium , might . it is thus ... | for a quantum system , a density matrix that is not pure can arise , via averaging , from a distribution of its wave function , a normalized vector belonging to its hilbert space . while itself does not determine a unique , additional facts , such as that the system has come to thermal equilibrium , might . it is thus ... |
1007.3662 | i | for an r.v . @xmath0 with density @xmath2 , mean @xmath3 and finite variance @xmath4 , goldstein and reinert @xcite showed the identity ( see also @xcite ) @xmath5,\ ] ] which holds for any absolutely continuous function @xmath6 with a.s . derivative @xmath7 such that the right - hand side is finite . in ( [ eq1.1 ] ) ... | for an absolutely continuous ( integer - valued ) r.v . of the pearson ( ord ) family , we show that , under natural moment conditions , a stein - type covariance identity of order holds ( cf . [ goldstein and reinert , _ j. theoret . this identity is closely related to the corresponding sequence of orthogonal polynom... | for an absolutely continuous ( integer - valued ) r.v . of the pearson ( ord ) family , we show that , under natural moment conditions , a stein - type covariance identity of order holds ( cf . [ goldstein and reinert , _ j. theoret . probab . _ * 18 * ( 2005 ) 237260 ] ) . this identity is closely related to the cor... |
1604.00019 | c | in order to quantitatively interpret the radio light curves and spectra of isne , one needs to understand the evolution of the shocked gas . one popular model for shock evolution is the ( * ? ? ? * c82 ) one - dimensional self - similar interaction model , which assumes a continuous csm . here we explored moving beyo... | however , while such models have been successfully applied to core - collapse sne , the assumption of continuity may not be accurate for sne ia , as shells of csm could be formed by pre - supernova eruptions ( novae ) . in this work , we model the interaction of sne with a spherical , low density , finite - extent csm ... | for decades , a wide variety of observations spanning the radio through optical and on to the x - ray have attempted to uncover signs of type ia supernovae ( sne ia ) interacting with a circumstellar medium ( csm ) . the goal of these studies is to constrain the nature of the hypothesized sn ia mass - donor companion .... |
1611.08503 | i | many mathematical models of physical phenomena deal with systems of volterra integral equations with singular kernels ( e.g. @xcite ) . in this paper , motivated by some nonlinear volterra integral equations arising in quantum mechanics , we investigate the properties of convolution operators with kernels possibly more... | for kernels which are positive and integrable we show that the operator on a finite time interval enjoys a regularizing effect when applied to hlder continuous and lebesgue functions and a `` contractive '' effect when applied to sobolev functions . for hlder continuous functions , we establish that the improvement of ... | for kernels which are positive and integrable we show that the operator on a finite time interval enjoys a regularizing effect when applied to hlder continuous and lebesgue functions and a `` contractive '' effect when applied to sobolev functions . for hlder continuous functions , we establish that the improvement of ... |
1503.03936 | r | in this section , we report numerical experiments to illustrate the regularizing effects of minres and mr - ii and make a number of comparisons . we justify our theory : ( i ) minres has only the partial regularization , independent of the degree of ill - posedness , and a hybrid minres is generally needed ; ( ii ) the... | we call a regularized solution best possible if it is at least as accurate as the best regularized solution obtained by the truncated singular value decomposition ( tsvd ) method . in this paper , we analyze their regularizing effects and establish the following results : ( i ) the filtered svd expression are derived f... | for large scale symmetric discrete ill - posed problems , minres and mr - ii are often used iterative regularization solvers . we call a regularized solution best possible if it is at least as accurate as the best regularized solution obtained by the truncated singular value decomposition ( tsvd ) method . in this pape... |
cond-mat0204325 | i | the understanding of spin dephasing is of paramount interest in all fields of nuclear magnetic resonance ( nmr ) sciences . in nmr spectroscopy it determines the line shape , in nmr imaging it is besides longitudinal relaxation the major mechanism determining the contrast and contains morphological as well as functio... | rev . lett . 83 ( 1999 ) 4215 ) into a systematic framework . our new approach provides expressions for the free induction and spin echo magnetization decays that may be solved analytically or at least numerically . it is tested for the generic cases of dephasing due to an anderson - weiss process and due to restricted... | for markovian dynamics of field fluctuations we present here an extended strong collision approximation , thereby putting our previous strong collision approach ( phys . rev . lett . 83 ( 1999 ) 4215 ) into a systematic framework . our new approach provides expressions for the free induction and spin echo magnetization... |
cond-mat0107553 | c | by considering the gfe for a system , this paper proposed a vpa scheme for the generalized statistical mechanics based on the tsallis entropy . for approximating the gfe , we derived the truncated expressions for @xmath57 up to the third order in the variational perturbation expansion , and the classical harmonic oscil... | for the generalized statistical mechanics based on the tsallis entropy , a variational perturbation approximation method with the principle of minimal sensitivity is developed by calculating the generalized free energy up to the third order in variational perturbation expansion . the approximation up to the first order... | for the generalized statistical mechanics based on the tsallis entropy , a variational perturbation approximation method with the principle of minimal sensitivity is developed by calculating the generalized free energy up to the third order in variational perturbation expansion . the approximation up to the first order... |
1101.4890 | i | in summary , einstein s field equation is extended to include the quantum effect of gravity , from the general assumption that gravity force originates from the coupling and thermal equilibrium between matter and vacuum background . with this new field equation and physical mechanism of gravity force , without any fitt... | from the general assumption that gravity originates from the coupling and thermal equilibrium between matter and vacuum , after a derivation of newton s law of gravitation and an interpretation of the attractive gravity force between two classical objects , we consider the macroscopic quantum gravity effect for particl... | from the general assumption that gravity originates from the coupling and thermal equilibrium between matter and vacuum , after a derivation of newton s law of gravitation and an interpretation of the attractive gravity force between two classical objects , we consider the macroscopic quantum gravity effect for particl... |
astro-ph0612517 | i | in the favored cold dark matter cosmology , present - day galaxies were assembled hierarchically from smaller building blocks at earlier cosmic times . since all nearby galaxies with stellar spheroids are observed to host nuclear smbhs @xcite , hierarchical merging leads inevitably to the formation of smbh binaries @xc... | galaxies with stellar bulges are generically observed to host supermassive black holes ( smbhs ) . the hierarchical merging of galaxies should therefore lead to the formation of smbh binaries . if the binary lifetime exceeds the typical time between mergers , then triple black hole ( bh ) systems may form . we study th... | galaxies with stellar bulges are generically observed to host supermassive black holes ( smbhs ) . the hierarchical merging of galaxies should therefore lead to the formation of smbh binaries . merging of old massive galaxies with little gas promotes the formation of low - density nuclei where smbh binaries are expecte... |
astro-ph0612517 | m | to get a physically motivated distribution of bh mass ratios , we associate the formation of the inner and outer binaries with the last two major mergers in the history of the galactic halo hosting the triple system . we use extended press - schechter theory @xcite to calculate the probability distributions of the halo... | merging of old massive galaxies with little gas promotes the formation of low - density nuclei where smbh binaries are expected to survive over long times . our simulations include a smooth background potential consisting of a stellar bulge plus a dark matter halo , drag forces due to gravitational radiation and dynami... | galaxies with stellar bulges are generically observed to host supermassive black holes ( smbhs ) . the hierarchical merging of galaxies should therefore lead to the formation of smbh binaries . merging of old massive galaxies with little gas promotes the formation of low - density nuclei where smbh binaries are expecte... |
1608.08462 | i | in @xcite , we constructed a perturbative invariant of 3-manifolds with @xmath8 by modifying fukaya s morse homotopy theoretic invariant ( @xcite ) . in this paper , we extend the invariant of @xcite to 3-manifolds with higher first betti numbers and see that it is effectively utilized in the study of finite type invar... | garoufalidis and levine defined a filtration for 3-manifolds equipped with some degree 1 map (-homology equivalence ) to a fixed 3-manifold and showed that there is a natural surjection from a space of-decorated graphs to the graded quotient of the filtration over $ ] . in this paper , we show that in the case of the s... | garoufalidis and levine defined a filtration for 3-manifolds equipped with some degree 1 map (-homology equivalence ) to a fixed 3-manifold and showed that there is a natural surjection from a space of-decorated graphs to the graded quotient of the filtration over $ ] . in this paper , we show that in the case of the s... |
q-bio0702003 | i | genetic switch systems with mutual repression of two transcription factors , have been studied using a combination of deterministic and stochastic methods . these system exhibit bistability , namely two stable states such that spontaneous transitions between them are rare . induced transitions take place as a result of... | genetic switch systems with mutual repression of two transcription factors are studied using deterministic methods ( rate equations ) and stochastic methods ( the master equation and monte carlo simulations ) . these systems exhibit bistability , namely two stable states such that spontaneous transitions between them a... | genetic switch systems with mutual repression of two transcription factors are studied using deterministic methods ( rate equations ) and stochastic methods ( the master equation and monte carlo simulations ) . these systems exhibit bistability , namely two stable states such that spontaneous transitions between them a... |
1408.1653 | i | hexagonal boron nitride ( hbn ) , a wide - bandgap insulator , has recently emerged as a sort of `` magic '' substrate for exfoliated graphene sheets . early on , it was demonstrated @xcite that hbn is a much better substrate than @xmath2the ordinary substrate @xcite for much of the early work in graphene physics and... | we focus on scattering of these modes against graphene s acoustic phonons and hbn optical phonons , two sources of scattering that are expected to play a key role in hbn / g / hbn stacks . we confirm that the plasmon lifetime is not directly correlated with the mobility : in fact , it can be anti - correlated . | graphene sheets encapsulated between hexagonal boron nitride ( hbn ) slabs display superb electronic properties due to very limited scattering from extrinsic disorder sources such as coulomb impurities and corrugations . such samples are therefore expected to be ideal platforms for highly - tunable low - loss plasmonic... |
1408.1653 | i | we have presented a theory of hybrid plasmon - phonon modes in a graphene sheet encapsulated between two hexagonal boron nitride ( hbn ) semi - infinite slabs ( hbn / g / hbn ) . by using linear response theory and the random phase approximation , we have calculated the dispersion relation of hybrid plasmon - phonon mo... | graphene sheets encapsulated between hexagonal boron nitride ( hbn ) slabs display superb electronic properties due to very limited scattering from extrinsic disorder sources such as coulomb impurities and corrugations . such samples are therefore expected to be ideal platforms for highly - tunable low - loss plasmonic... | graphene sheets encapsulated between hexagonal boron nitride ( hbn ) slabs display superb electronic properties due to very limited scattering from extrinsic disorder sources such as coulomb impurities and corrugations . such samples are therefore expected to be ideal platforms for highly - tunable low - loss plasmonic... |
astro-ph0612256 | c | the extreme interest in grb050904 has motivated several groups to analyze the burst data and suggest interpretations . these works fall into two categories : ( 1 ) comparing the properties of grb050904 with other bursts ; and ( 2 ) making fits to the grb050904 data either in the framework of internal shock or external ... | we suggest that the period of accelerated decay in the nir may be due to suppression of synchrotron radiation by inverse compton interaction of flare photons with electrons in the forward shock ; a subsequent interval of slow decay would then be due to a progressive decline in this suppression . | grb050904 at redshift , discovered and observed by _ swift_and with spectroscopic redshift from the subaru telescope , is the first gamma - ray burst to be identified from beyond the epoch of reionization . since the progenitors of long gamma - ray bursts have been identified as massive stars , this event offers a uniq... |
astro-ph0612256 | c | in this paper we have performed the most extensive multiband analysis so far of the grb050904 afterglow . we have considered two scenarios : ( a ) only forward shock emission is considered , and the flares peaking at @xmath263 after the burst are assumed to be due to internal shocks ( or are otherwise independent of th... | apart from its record redshift , the burst is remarkable in two respects : first , it exhibits fast - evolving and optical flares that peak simultaneously ats in the observer frame , and may thus originate in the same emission region ; and second , its afterglow exhibits an accelerated decay in the near - infrared ( n... | grb050904 at redshift , discovered and observed by _ swift_and with spectroscopic redshift from the subaru telescope , is the first gamma - ray burst to be identified from beyond the epoch of reionization . since the progenitors of long gamma - ray bursts have been identified as massive stars , this event offers a uniq... |
1606.05507 | i | all graphs in this paper are finite and simple . a graph @xmath15 is a of a graph @xmath16 if @xmath15 can be obtained from a subgraph of @xmath16 by contracting edges . we write @xmath17 if @xmath15 is a minor of @xmath16 . in those circumstances we also say that @xmath16 has an @xmath15 . our work is motivated by the... | hadwiger s conjecture from 1943 states that for every integer , every graph either can be-colored or has a subgraph that can be contracted to the complete graph on vertices . as pointed out by paul seymour in his recent survey on hadwiger s conjecture , proving that graphs with no minor are-colorable is the first case ... | hadwiger s conjecture from 1943 states that for every integer , every graph either can be-colored or has a subgraph that can be contracted to the complete graph on vertices . as pointed out by paul seymour in his recent survey on hadwiger s conjecture , proving that graphs with no minor are-colorable is the first case ... |
astro-ph0009157 | c | as discussed in sections[ls5130_dis][ls5127_dis ] , all four stars have relatively normal oxygen abundances . if the oxygen abundance gradients derived in the solar neighbourhood and outer disk are extrapolated inwards ( smartt & rolleston 1997 , rsdr ; @xmath10.07 dexkpc@xmath7 ) their o abundances would be 0.3@xmath1... | the stars appear to be rich in all the well sampled chemical elements ( c , n , si , mg , s , al ) , _ except for oxygen_. oxygen abundances derived in the atmospheres of these four stars are very similar to that in the solar neighbourhood . if the photospheric composition of these young stars is reflective of the gase... | high - resolution , high signal - to - noise spectral data are presented for four young b - type stars lying towards the galactic centre . determination of their atmospheric parameters from their absorption line profiles , and photometric measurement of the continua indicate that they are massive objects lying slightly... |
astro-ph0009157 | c | the analysis of high - quality data for four blue stars lying towards the galactic centre , and a comparison with young stars throughout the galactic disk , leads to the following conclusions 1 . the four stars appear to be normal , young , massive , early b - type stars . they lie slightly out of the galactic plane... | high - resolution , high signal - to - noise spectral data are presented for four young b - type stars lying towards the galactic centre . determination of their atmospheric parameters from their absorption line profiles , and photometric measurement of the continua indicate that they are massive objects lying slightly... | high - resolution , high signal - to - noise spectral data are presented for four young b - type stars lying towards the galactic centre . determination of their atmospheric parameters from their absorption line profiles , and photometric measurement of the continua indicate that they are massive objects lying slightly... |
astro-ph0409268 | i | classical t tauri stars ( cttss ) appear to be roughly solar mass pre - main sequence stars still surrounded by disks of material which actively accrete onto the central star . their properties have been recently reviewed by mnard and bertout ( 1999 ) . it is within the disks surrounding cttss that solar systems form .... | high resolution optical and infrared ( ir ) echelle spectra of the naked ( diskless ) t tauri star hubble 4 are presented . the k band ir spectra include 4 zeeman sensitive lines along with several magnetically insensitive co lines . these stellar parameters are used to synthesize k band spectra to compare with the obs... | high resolution optical and infrared ( ir ) echelle spectra of the naked ( diskless ) t tauri star hubble 4 are presented . the k band ir spectra include 4 zeeman sensitive lines along with several magnetically insensitive co lines . detailed spectrum synthesis combined with modern atmospheric models is used to fit the... |
0811.3149 | c | in this paper we have studied conformal perturbation theory beyond the leading order . we have shown that , at least up to quadratic order , the combined bulk boundary perturbation problem is renormalisable , using the minimal subtraction scheme . we also discussed the more commonly used ` wilsonian ' ope scheme , and ... | we identify systematically the universal quantities in the beta function equations , and we give explicit formulae for the universal coefficients at next - to - leading order in terms of integrated correlation functions . as an example , we analyse the radius - dependence of the conformal dimension of some boundary ope... | higher order conformal perturbation theory is studied for theories with and without boundaries . we identify systematically the universal quantities in the beta function equations , and we give explicit formulae for the universal coefficients at next - to - leading order in terms of integrated correlation functions . a... |
astro-ph9907082 | c | our main goal here is to use observed properties of the blue compact dwarf galaxy i zw 18 to put constraints on its age : the high ionization state of the gas and the presence of wr stars in the main body , the existence of ionized gas in the c component , and the colour - magnitude diagrams from hst images . we were m... | hubble space telescope ( hst ) colour - magnitude diagrams in , and along with long - slit multiple mirror telescope ( mmt ) spectrophotometric data are used to investigate the evolutionary status of the nearby blue compact dwarf ( bcd ) galaxy i zw 18 . we find that the distance to i zw 18 should be as high as 20 mp... | hubble space telescope ( hst ) colour - magnitude diagrams in , and along with long - slit multiple mirror telescope ( mmt ) spectrophotometric data are used to investigate the evolutionary status of the nearby blue compact dwarf ( bcd ) galaxy i zw 18 . we find that the distance to i zw 18 should be as high as 20 mp... |
1303.1906 | i | in this paper i have studied the rest - frame uv / optical / near - ir ( @xmath14 $ \sim$}}~}3 \ , \rm \mu m$ ] ) seds of 174 @xmath4-selected galaxies with secure spectroscopic redshifts @xmath2 , analysing explicitly the presence and significance of a hot - dust , power - law component . i modelled the residual light... | i derive this diagnostic from the analysis of 174 galaxies with and spectroscopic redshifts in the chandra deep field south , for which i study the rest - frame uv / optical / near - ir spectral energy distributions ( seds ) , after subtracting a hot - dust , power - law component with three possible spectral indices ,... | i present a generalized power - law diagnostic that allows to identify the presence of active galactic nuclei ( agn ) in infrared ( ir ) galaxies at , down to flux densities at which the extragalactic ir background is mostly resolved . i derive this diagnostic from the analysis of 174 galaxies with and spectroscopic re... |
1501.07888 | i | the study of the intersection theory on the moduli space of riemann surfaces with boundary ( often viewed , with the boundary removed , as open riemann surfaces ) was recently initiated in @xcite . the authors constructed a descendent theory in genus @xmath0 and obtained a complete description of it . in all genera ,... | in a recent work , r. pandharipande , j. p. solomon and the second author have initiated a study of the intersection theory on the moduli space of riemann surfaces with boundary . they conjectured that the generating series of the intersection numbers satisfies the open kdv equations . in this paper we prove this co... | in a recent work , r. pandharipande , j. p. solomon and the second author have initiated a study of the intersection theory on the moduli space of riemann surfaces with boundary . they conjectured that the generating series of the intersection numbers satisfies the open kdv equations . in this paper we prove this co... |
0907.4392 | i | the values of the fundamental constants determine the nature of the physical universe , from the size of mountains on earth to the eventual fate of the universe as a whole . historically we have assumed that these constants are invariant in space and time . speculation on the possibility of a time variation of the cons... | in an effort to resolve the discrepancy between two measurements of the fundamental constant , the proton to electron mass ratio , at early times in the universe we reanalyze the same data used in the earlier studies . both of the previous studies and this study are based on the same data but with differing analysis me... | in an effort to resolve the discrepancy between two measurements of the fundamental constant , the proton to electron mass ratio , at early times in the universe we reanalyze the same data used in the earlier studies . our analysis of the molecular hydrogen absorption lines in archival vlt / uves spectra of the damped ... |
0907.4392 | c | our basic conclusion , based on the combination of data from q0347 - 383 and q0405 - 443 , is that there has been no change in the value of @xmath0 to 1 part in @xmath78 over a time span of 11.5 gigayears . this is approximately @xmath9 of the age of the universe . the accuracy of the limit on @xmath1 is set by both th... | our analysis of the molecular hydrogen absorption lines in archival vlt / uves spectra of the damped lyman alpha systems in the qsos q0347 - 383 and q0405 - 443 yields a combined measurement of a value of , consistent with no change in the value of over a time span of 11.5 gigayears . here improvements in the wavelengt... | in an effort to resolve the discrepancy between two measurements of the fundamental constant , the proton to electron mass ratio , at early times in the universe we reanalyze the same data used in the earlier studies . our analysis of the molecular hydrogen absorption lines in archival vlt / uves spectra of the damped ... |
1701.05316 | i | in fluid dynamical simulations in astrophysics , large deformations are common and surface tracking is sometimes necessary . mesh - free methods , in which particles move following the motion of fluid , are very useful for such simulations . in particular , smoothed particle hydrodynamics ( sph ; @xcite , @xcite ) has ... | in fluid dynamical simulations in astrophysics , large deformations are common and surface tracking is sometimes necessary . smoothed particle hydrodynamics ( sph ) method has been used in many of such simulations . recently , however , it has been shown that sph can not handle contact discontinuities or free surfaces ... | in fluid dynamical simulations in astrophysics , large deformations are common and surface tracking is sometimes necessary . smoothed particle hydrodynamics ( sph ) method has been used in many of such simulations . recently , however , it has been shown that sph can not handle contact discontinuities or free surfaces ... |
1401.1154 | i | there are many situations in which it is necessary to distinguish the topological properties of ring - shaped quasi one - dimensional objects . this is for instance the case of polymers @xcite , vortex structures in nematic liquid crystals @xcite , @xmath2 superfluid @xcite and disclination lines in chiral nematic coll... | in mathematics there is a wide class of knot invariants that may be expressed in the form of multiple line integrals computed along the trajectory describing the spatial conformation of the knot . in this work it is addressed the problem of evaluating invariants of this kind in the case in which the knot is discrete , ... | in mathematics there is a wide class of knot invariants that may be expressed in the form of multiple line integrals computed along the trajectory describing the spatial conformation of the knot . in this work it is addressed the problem of evaluating invariants of this kind in the case in which the knot is discrete , ... |
1401.1154 | c | in this work an algorithm to compute the vassiliev invariant of degree 2 @xmath1 for any knot @xmath0 has been provided . particular attention has been devoted to discrete knots whose trajectories consist of segments connected together at their ends forming @xmath4curves in the space . this case is relevant in numerica... | such discrete knots appear almost everywhere in numerical simulations of systems containing one dimensional ring - shaped objects . the procedure is quite general and can be applied to any discrete knot defined off or on lattice . this is the simplest knot invariant that admits a definition in terms of multiple line in... | in mathematics there is a wide class of knot invariants that may be expressed in the form of multiple line integrals computed along the trajectory describing the spatial conformation of the knot . in this work it is addressed the problem of evaluating invariants of this kind in the case in which the knot is discrete , ... |
1312.0003 | i | there are several ways to test the geometry of a cosmological model and its expansion , i.e. , that redshifts of the galaxies are cosmological and not due to an alternative mechanism ( narlikar 1989 ; lpez - corredoira 2003 , section 2.1 ; lpez - corredoira 2006 ) . however , almost all of the cosmological tests are en... | in order to test the expansion of the universe and its geometry , we carry out an alcock & paczyski cosmological test , that is , an evaluation of the ratio of observed angular size to radial / redshift size . the main advantage of this test is that it does not depend on the evolution of the galaxies , but only on the ... | in order to test the expansion of the universe and its geometry , we carry out an alcock & paczyski cosmological test , that is , an evaluation of the ratio of observed angular size to radial / redshift size . the main advantage of this test is that it does not depend on the evolution of the galaxies , but only on the ... |
1312.0003 | c | the application of the alcock paczyski test using the anisotropic two - point correlation function was shown here to be a useful tool for discriminating among different cosmological models without any a priori assumptions . we have seen that the major caveat is the disentanglement with the redshift distortions produce... | we derive the anisotropic correlation function of sources in three surveys within the sloan digital sky survey ( sdss ) : galaxies from sdss - iii / baryon oscillation spectroscopy survey data release 10 ( boss - dr10 ) , and qsos from sdss - ii and sdss - iii / boss - dr10 . from these , we are able to disentangle th... | in order to test the expansion of the universe and its geometry , we carry out an alcock & paczyski cosmological test , that is , an evaluation of the ratio of observed angular size to radial / redshift size . the main advantage of this test is that it does not depend on the evolution of the galaxies , but only on the ... |
quant-ph0507010 | i | quantum adiabatic algorithms , first conceived in ref . @xcite , have been developed as an alternative to the traditional circuit model of quantum computation . an important aspect of the adiabatic approach is its expected resilience to various kinds of open system effects , which makes it a promising candidate for rob... | in phys . rev . a * 71 * , 060312(r ) ( 2005 ) the robustness of the local adiabatic quantum search to decoherence in the instantaneous eigenbasis of the search hamiltonian was examined . as in the case of the local search the asymptotic time complexity for the global search is the same as for the ideal closed case , a... | in phys . rev . a * 71 * , 060312(r ) ( 2005 ) the robustness of the local adiabatic quantum search to decoherence in the instantaneous eigenbasis of the search hamiltonian was examined . we expand this analysis to include the case of the global adiabatic quantum search . as in the case of the local search the asymptot... |
1609.07930 | c | in this section we apply the stability criteria and growth rate estimates of the two - fluid model to reasonable models of protoplanetary disks . because of uncertainties in the parameters and deficiencies in the model itself , we do not attempt to be comprehensive or to hold fast to the quantitative results we obtain ... | in protoplanetary disks the aerodynamical friction between particles and gas induces a variety of instabilities that facilitate planet formation . of these in contrast to a single - fluid treatment , the sgi is quenched within a critical disk radius , as large as 10 au and 30 au for cm and mm sized particles respective... | in protoplanetary disks the aerodynamical friction between particles and gas induces a variety of instabilities that facilitate planet formation . of these we examine the so called ` secular gravitational instability ' ( sgi ) in the two - fluid approximation , deriving analytical expressions for its stability criteria... |
1210.8304 | i | the constraints of causality for two - body scattering with finite - range interactions were first derived by wigner @xcite . the causality bound can be understood as a lower bound on the time delay between the incoming and outgoing wave packets , @xmath4 . when @xmath4 is negative , the outgoing wave packet departs e... | the main result is an upper bound for the coulomb - modified effective range parameter . we discuss the implications of this bound to the effective field theory for nuclear halo systems . for the bound - state regime , we find relations for the asymptotic normalization coefficients ( ancs ) of nuclear halo states . as ... | in quantum systems with short - range interactions , causality imposes nontrivial constraints on low - energy scattering parameters . we investigate these causality constraints for systems where a long - range coulomb potential is present in addition to a short - range interaction . the main result is an upper bound fo... |
astro-ph0601336 | i | the determination of water abundance in space is a long standing problem in astronomy . theoretical models predict that water can be the most abundant species in _ warm _ molecular clouds after h@xmath0 and co @xcite . therefore , the determination of its spatial distribution and abundance contributes to a better knowl... | in the region of sgr b2 there are several condensations heated externally by nearby hot stars . therefore ho far we have conducted a study combining ho lines in both spectral regions . first , observations of several ho thermal lines seen in absorption toward sgr b2(m ) at a spectral resolution of km s have been an... | in the region of sgr b2 there are several condensations heated externally by nearby hot stars . therefore ho far ir lines are expected to probe only an external low density and high temperature section of these condensations , whereas millimeter - wave lines can penetrate deeper into them where the density is higher ... |
astro-ph0601336 | c | the warm gas present in the outer layers of sgr b2(m ) might be expected to radiate in high@xmath6 co lines . the co @xmath6=1413 transition at 185.999 @xmath28 m is the one with the lowest energy level ( e@xmath53@xmath14581 k ) within the range of iso / lws detectors . however , we have not detected any emission / ... | ir lines are expected to probe only an external low density and high temperature section of these condensations , whereas millimeter - wave lines can penetrate deeper into them where the density is higher and t lower . ho line at 183.31 ghz , seen in emission , has also been obtained and analyzed . the ho lines seen ... | in the region of sgr b2 there are several condensations heated externally by nearby hot stars . therefore ho far ir lines are expected to probe only an external low density and high temperature section of these condensations , whereas millimeter - wave lines can penetrate deeper into them where the density is higher ... |
astro-ph0601336 | i | we have carried out far ir observations of several thermal absorption lines of water vapor toward sgr b2(m ) and have mapped the 183.31 ghz water line around the main dust condensations of the complex . the main conclusions of this work are the following : 1 . the detected water absorption lines are very opaque a... | we conclude , based on the observed co=76 line at 806.65 ghz with the _ caltech submillimeter observatory _ , and the lack of emission from the far ir co lines , that the gas density has to be lower than . using the values obtained for the kinetic temperature and gas density from oh , co , and other molecular spec... | in the region of sgr b2 there are several condensations heated externally by nearby hot stars . therefore ho far ir lines are expected to probe only an external low density and high temperature section of these condensations , whereas millimeter - wave lines can penetrate deeper into them where the density is higher ... |
1109.1515 | c | much as the fwhm of h@xmath70 , strength of ( relative to h@xmath70 ) , and soft x - ray properties can be used to divide low-@xmath34 quasars into extrema in the `` eigenvector 1 '' context @xcite , so can the properties of the emission line at high redshift . in @xcite , we showed that the extrema of large ( small )... | we explore the connection between these emission - line properties and the uv through x - ray spectral energy distribution ( sed ) for radio - quiet ( rq ) quasars . we find that rq quasars with both strong emission and small blueshifts can be classified as `` hard - spectrum '' sources that are ( relatively ) strong... | in the restframe ultra - violet ( uv ) , two of the parameters that best characterize the range of emission - line properties in quasar broad emission - line regions are the equivalent width and the blueshift of the line relative to the quasar rest frame . we explore the connection between these emission - line proper... |
1302.5386 | i | let us consider a bounded domain @xmath0 in @xmath1 containing the closed unit ball @xmath2 ( see figure 1 ) . let @xmath3 $ ] be a hlder continuous function which is periodic with respect to the orthonomal basis @xmath4 of @xmath1 . more precisely , @xmath5 satisfies @xmath6 with @xmath7 and @xmath5 as given above ... | in this article we investigate averaging properties of fully nonlinear pdes in bounded domains with oscillatory neumann boundary data . the oscillation is periodic and is present both in the operator and in the neumann data . our main result states that , when the domain does not have flat boundary parts and when the h... | in this article we investigate averaging properties of fully nonlinear pdes in bounded domains with oscillatory neumann boundary data . the oscillation is periodic and is present both in the operator and in the neumann data . our main result states that , when the domain does not have flat boundary parts and when the h... |
1112.1978 | c | in this article we have provided a formal framework for reidentification in general . we have defined @xmath0-confusion as a concept for modelling the anonymity of a database table and we have proved that @xmath0-confusion is a generalization of @xmath1-anonymity . then after a short survey on the different available d... | in this article we provide a formal framework for reidentification in general . we define-confusion as a concept for modelling the anonymity of a database table and we prove that-confusion is a generalization of-anonymity . after a short survey on the different available definitions of-anonymity for graphs we provide a... | in this article we provide a formal framework for reidentification in general . we define-confusion as a concept for modelling the anonymity of a database table and we prove that-confusion is a generalization of-anonymity . after a short survey on the different available definitions of-anonymity for graphs we provide a... |
1610.06790 | i | the strong numerical approximation of an it stochastic partial differential equation defined in the bounded domain @xmath1 is analyzed . the domain @xmath2 is assumed to be a convex polygon , or has smooth boundary . boundary conditions on the domain @xmath2 are typically neumann , dirichlet or robin conditions . more ... | in this paper , we consider the numerical approximation of a general second order semilinear stochastic partial differential equation ( spde ) driven by multiplicative and additive noise . our main interest is on such spdes where the nonlinear part is stronger than the linear part also called stochastic reactive domina... | in this paper , we consider the numerical approximation of a general second order semilinear stochastic partial differential equation ( spde ) driven by multiplicative and additive noise . our main interest is on such spdes where the nonlinear part is stronger than the linear part also called stochastic reactive domina... |
1610.06790 | r | before we state the well posedness result , let us define keys functional spaces , norms and notations that we will be use in the rest of the paper . let @xmath23 be a separable hilbert space . for all @xmath24 and for a banach space @xmath25 , we denote by @xmath26 the banach space of all equivalence classes of @xmath... | we consider noise that is in a trace class and give a strong convergence proof of the new scheme toward the exact solution in the root - mean - square norm . example.eps gsave newpath 20 20 moveto 20 220 lineto 220 220 lineto 220 20 lineto closepath 2 setlinewidth gsave .4 setgray fill grestore stroke grestore | in this paper , we consider the numerical approximation of a general second order semilinear stochastic partial differential equation ( spde ) driven by multiplicative and additive noise . our main interest is on such spdes where the nonlinear part is stronger than the linear part also called stochastic reactive domina... |
1702.02694 | i | the _ nariai spacetime _ was discovered by nariai in 1950 ( see the reprints of the original works in @xcite ) . it is the solution of einstein s vacuum equations for spacetime metrics and the sign convention for curvature tensors in @xcite . in this convention the de - sitter spacetime is a solution of eq . with @xm... | in this paper , we construct and study solutions of einstein s equations in vacuum with a positive cosmological constant which can be considered as inhomogeneous generalizations of the nariai cosmological model . similar to this nariai spacetime , our solutions are at the borderline between gravitational collapse and d... | in this paper , we construct and study solutions of einstein s equations in vacuum with a positive cosmological constant which can be considered as inhomogeneous generalizations of the nariai cosmological model . similar to this nariai spacetime , our solutions are at the borderline between gravitational collapse and d... |
1301.5298 | i | optimization appears in many areas of scientific computing , since the solution of a problem can often be described as the minimum of an optimization problem . local methods such as gradient descent are often employed to handle global minimization problems . they can be very efficient to compute a local minimum , but t... | in this paper , we describe a new method to compute the minimum of a real polynomial function and the ideal defining the points which minimize this polynomial function , assuming that the minimizer ideal is zero - dimensional . the proposed algorithm combines border basis , moment matrices and semidefinite programming ... | in this paper , we describe a new method to compute the minimum of a real polynomial function and the ideal defining the points which minimize this polynomial function , assuming that the minimizer ideal is zero - dimensional . our method is a generalization of lasserre relaxation method and stops in a finite number of... |
1310.1272 | i | the topological he - mckellar - wilkens ( hmw ) phase introduced in 1993 by x.g . he and b.h.j . mckellar @xcite and in 1994 by m. wilkens @xcite was never tested since its theoretical discovery . we have recently published such a test @xcite using our lithium atom interferometer . in a companion paper @xcite quoted h... | we start by describing our setup and we characterize the effects of the electric and magnetic fields needed to observe the hmw effect . then , we develop a model of our interferometer signals including all the defects we have identified . after various tests of this model , we use it to suppress the largest part of the... | in this paper , we describe an experimental test of the he - mckellar - wilkens ( hmw ) topological phase with our lithium atom interferometer . the expected value of the hmw phase shift in our experiment is small and its measurement was difficult because of stray phase shifts due to small experimental defects . we sta... |
1310.1272 | c | we have described a measurement of the he - mckellar - wilkens topological phase by atom interferometry . this experiment was feasible with our atom interferometer because the interferometer arms are well separated in space and the interferometer signal is intense , with a large fringe visibility , near @xmath300% . th... | in this paper , we describe an experimental test of the he - mckellar - wilkens ( hmw ) topological phase with our lithium atom interferometer . we thus obtain a series of measurements of the hmw phase : the results are% larger than expected and this discrepancy is probably due to some limitations of our model . | in this paper , we describe an experimental test of the he - mckellar - wilkens ( hmw ) topological phase with our lithium atom interferometer . the expected value of the hmw phase shift in our experiment is small and its measurement was difficult because of stray phase shifts due to small experimental defects . we sta... |
astro-ph0211159 | i | the one - point probability distribution function ( pdf ) of a random mass density field @xmath3 , or the counts - in - cells ( cic ) statistics of a discrete random distribution such as galaxies , is probably the first statistics used to reveal the clustering feature of galaxy distribution . in the famous work by edwi... | we also establish the mapping between the dwt one - point statistics in redshift space and real space , i.e. the algorithm for recovering the dwt one - point statistics from the redshift distortion of bulk velocity , velocity dispersion , and selection function . the dwt estimators , however , do not need such extra in... | in this paper , we develop a method of performing the one - point statistics of a perturbed density field with a multiresolutional decomposition based on the discrete wavelet transform ( dwt ) . we establish the algorithm of the one - point variable and its moments in considering the effects of poisson sampling and sel... |
astro-ph0211159 | c | we have developed the one - point statistics of a perturbed density field with the multiresolutional decomposition based on discrete wavelet transform . since the scale and shape of the dwt bases are well defined , this frame work is very effective to deal with problems of how the one - point distribution and its momen... | in this paper , we develop a method of performing the one - point statistics of a perturbed density field with a multiresolutional decomposition based on the discrete wavelet transform ( dwt ) . we establish the algorithm of the one - point variable and its moments in considering the effects of poisson sampling and sel... | in this paper , we develop a method of performing the one - point statistics of a perturbed density field with a multiresolutional decomposition based on the discrete wavelet transform ( dwt ) . we establish the algorithm of the one - point variable and its moments in considering the effects of poisson sampling and sel... |
1208.6419 | i | star clusters are considered as important tracers for understanding the formation and evolution of their host galaxies @xcite . star cluster systems have been traditionally separated into two populations globular clusters and open clusters ( gcs and ocs)on their ages , masses , metallicities , and positions . however ... | in this paper , we present photometry for young star clusters in m31 , which are selected from caldwell et al . these star clusters have been observed as part of the beijing arizona taiwan connecticut ( batc ) multicolor sky survey from 1995 february to 2008 march . | in this paper , we present photometry for young star clusters in m31 , which are selected from caldwell et al . these star clusters have been observed as part of the beijing arizona taiwan connecticut ( batc ) multicolor sky survey from 1995 february to 2008 march . the batc images including these star clusters are ... |
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