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1110.3870	i	present study deals with the model calculations of co cameron band and @xmath4doublet ultraviolet emissions in martian dayglow and the impact of solar euv flux on the calculated intensities . photoelectrons generated due to photoionization in the martian atmosphere have been degraded in the atmosphere using monte carlo...	calculated limb intensities profiles are compared with spicam / mars express and mariner observations . analytical yield spectrum densities of prominent ions and co molecule in excited triplet a state are calculated using major ion - neutral reactions . volume emission rates of co cameron and co uv doublet bands have b...	this study is aimed at making a calculation about the impact of the two most commonly used solar euv flux models solar2000 ( s2k ) of and euvac model of on photoelectron fluxes , volume emission rates , ion densities and co cameron and co uv doublet band dayglow emissions on mars in three solar activity conditions : ...
1702.08003	i	one of the most elementary system configuation models in multi - user information theory is the broadcast channel ( bc ) . it has been introduced in the early seventies of the twentieth century by cover @xcite , and since then , a vast amount of papers and books , studying different topics of the broadcast problem , ha...	this work contains two main contributions concerning the asymmetric broadcast channel . the first is an analysis of the exact random coding error exponents for both users , and the second is the derivation of universal decoders for both users . these universal decoders are certain variants of the maximum mutual informa...	this work contains two main contributions concerning the asymmetric broadcast channel . the first is an analysis of the exact random coding error exponents for both users , and the second is the derivation of universal decoders for both users . these universal decoders are certain variants of the maximum mutual informa...
0805.3731	i	new @xmath9-dimensional @xmath0- and @xmath1- and @xmath2-transforms were recently described in @xcite . each transform is based on a compact semisimple lie group of rank @xmath9 and comes in three versions : analogs of fourier series , fourier integrals , and fourier transforms on an @xmath9-dimensional lattice . the...	three dimensional continuous and discrete fourier - like transforms , based on the three simple and four semisimple compact lie groups of rank 3 , are presented . for each simple lie group , pertinent properties of the functions are described in detail , such as their orthogonality within each family , when integrated ...	three dimensional continuous and discrete fourier - like transforms , based on the three simple and four semisimple compact lie groups of rank 3 , are presented . for each simple lie group , there are three families of special functions (- ,- , and-functions ) on which the transforms are built . pertinent properties of...
1003.2341	i	tio@xmath0 has been one of the most studied oxides over the past few years . this is due to the broad range of applications it offers in strategic fields of scientific , technological , environmental , and commercial relevance . in particular , tio@xmath0 surfaces and nanocrystals provide a rich variety of suitably tun...	titanium dioxide is one of the most widely investigated oxides . this is due to its broad range of applications , from catalysis to photocatalysis to photovoltaics . despite this large interest , many of its bulk properties further , some of tio s most important properties , such as its electronic band gap , the locali...	titanium dioxide is one of the most widely investigated oxides . this is due to its broad range of applications , from catalysis to photocatalysis to photovoltaics . despite this large interest , many of its bulk properties have been sparsely investigated using either experimental techniques or _ ab initio _ theory . f...
0905.4683	i	determining the physical parameters of large samples of galaxies is crucial to constrain our knowledge of the complicated physical processes that govern the formation and evolution of these systems . ultimately , we seek methods that quickly and effectively map observed data from @xmath0 galaxies to sets of parameters ...	to further our knowledge of the complex physical process of galaxy formation , it is essential that we characterize the formation and evolution of large databases of galaxies . the spectral synthesis starlight code of cid fernandes et al . ( 2004 ) was designed for this purpose . results of starlight are highly depende...	to further our knowledge of the complex physical process of galaxy formation , it is essential that we characterize the formation and evolution of large databases of galaxies . the spectral synthesis starlight code of cid fernandes et al . ( 2004 ) was designed for this purpose . results of starlight are highly depende...
0905.4683	m	we adopt the model of galaxy spectra as a mixture of simple systems introduced in @xcite : @xmath3 where @xmath4 is the model flux in wavelength bin @xmath5 . the component @xmath6 is the @xmath7th basis spectrum normalized at wavelength @xmath8 . the basis of ssp spectra @xmath9 is chosen before performing the analysi...	speed of the code , which uses random walks through the parameter space , scales as the square of the number of basis spectra , making it computationally necessary to choose a small number of ssps that are coarsely sampled in age and metallicity . in this paper , we develop methods based on diffusion map ( lafon & lee ...	to further our knowledge of the complex physical process of galaxy formation , it is essential that we characterize the formation and evolution of large databases of galaxies . the spectral synthesis starlight code of cid fernandes et al . ( 2004 ) was designed for this purpose . results of starlight are highly depende...
astro-ph0003109	i	galaxies do not live isolated lives , but exist in the tidal fields of their environment . arp ( 1966 ) , in his atlas of peculiar galaxies , lay the observational groundwork for the modern study of interacting galaxy systems by identifying many `` peculiar '' systems , later interpreted as various stages of major gala...	to investigate the link between weak tidal interactions in disk galaxies and the boosting of their recent star formation , we obtain images and spatially integrated spectra ( ) for 40 late - type spiral galaxies ( sab - sbc ) with varying degrees of lopsidedness ( a dynamical indicator of weak interactions ) . we quant...	to investigate the link between weak tidal interactions in disk galaxies and the boosting of their recent star formation , we obtain images and spatially integrated spectra ( ) for 40 late - type spiral galaxies ( sab - sbc ) with varying degrees of lopsidedness ( a dynamical indicator of weak interactions ) . we quant...
astro-ph0003109	i	to quantify the correlation between the recent sf histories of present - day spiral galaxies and their global asymmetry , we compare the integrated spectral properties of late - type spirals of varying lopsidedness . we find that the recent ( @xmath159 gyr ) sfh and current ( @xmath160 years ) sfr are both strongly cor...	the median spectrum of the most lopsided galaxies shows strong evidence for a more prominent young stellar population ( i.e. strong balmer absorption , strong nebular emission , a weak break and a blue continuum ) when compared to the median spectrum of the most symmetric galaxies . using the evolutionary population sy...	to investigate the link between weak tidal interactions in disk galaxies and the boosting of their recent star formation , we obtain images and spatially integrated spectra ( ) for 40 late - type spiral galaxies ( sab - sbc ) with varying degrees of lopsidedness ( a dynamical indicator of weak interactions ) . we quant...
1105.1482	i	the relationship between the transmitted symbol and the received signal vector in many communication systems can be expressed in the form @xmath1 where @xmath2 is the @xmath3 transmitted vector whose entries are chosen from a finite symbol alphabet , @xmath4 and @xmath5 are the @xmath6 received signal and noise vectors...	tree detection techniques are often used to reduce the complexity of _ a posteriori probability _ ( app ) detection in high dimensional multi - antenna wireless communication systems . in this paper , we introduce an efficient soft - input soft - output tree detection algorithm that employs a new type of look - ahead p...	tree detection techniques are often used to reduce the complexity of _ a posteriori probability _ ( app ) detection in high dimensional multi - antenna wireless communication systems . in this paper , we introduce an efficient soft - input soft - output tree detection algorithm that employs a new type of look - ahead p...
1312.6129	i	turbulence is a common phenomenon in astrophysical fluids ( see , for example , elmegreen & scalo 2004 ) and it is obvious that most astrophysical fluids are permeated by magnetic fields ( brandenburg & subramanian 2005 ) . such magnetized fluids can be investigated by numerical simulations of driven magnetohydrodynami...	turbulence is ubiquitous in astrophysical fluids such as the interstellar medium ( ism ) and the intracluster medium ( icm ) . in turbulence studies , it is customary to assume that fluid is driven on a single scale . however , in astrophysical fluids , there can be many different driving mechanisms that act on differe...	turbulence is ubiquitous in astrophysical fluids such as the interstellar medium ( ism ) and the intracluster medium ( icm ) . in turbulence studies , it is customary to assume that fluid is driven on a single scale . however , in astrophysical fluids , there can be many different driving mechanisms that act on differe...
0704.3889	c	we have compared the predictions for the liquid - vapour coexistence curve of a long - range yukawa fluid obtained from advanced theoretical approaches with gibbs ensemble monte carlo simulations . concerning the simulations care has to be taken when the range of the potential exceeds the length of the simulation box ....	two liquid state theories , the self - consistent ornstein - zernike equation ( scoza ) and the hierarchical reference theory ( hrt ) are shown , by comparison with monte carlo simulations , to perform extremely well in predicting the liquid - vapour coexistence of the hard core yukawa ( hcy ) fluid when the interactio...	two liquid state theories , the self - consistent ornstein - zernike equation ( scoza ) and the hierarchical reference theory ( hrt ) are shown , by comparison with monte carlo simulations , to perform extremely well in predicting the liquid - vapour coexistence of the hard core yukawa ( hcy ) fluid when the interactio...
0709.1114	i	in the past several years h@xmath0 has been detected in diffuse interstellar clouds @xcite where it had been expected to exist in abundances below observable limits . this surprising result raised various questions about the diffuse cloud environment . the rather simple chemistry of h@xmath0 allows for only three var...	h is detected in eight diffuse cloud sightlines with column densities varying from to . because of the simple chemistry associated with h production and destruction , these column density measurements can be used in concert with various other data to infer the primary cosmic - ray ionization rate , .	using high resolution infrared spectroscopy we have surveyed twenty sightlines for h absorption . h is detected in eight diffuse cloud sightlines with column densities varying from to . this brings to fourteen the total number of diffuse cloud sightlines where h has been detected . these detections are mostly alo...
0709.1114	c	values of the cosmic - ray ionization rate for diffuse clouds observed here as well as those determined for other diffuse clouds observed previously by us are given in the right hand column of table [ tbl4 ] . the detected values in the lines of sight to fourteen sources cover the range 0.53.2@xmath71 s@xmath6 . upper...	these detections are mostly along sightlines concentrated in the galactic plane , but well dispersed in galactic longitude . values range from s to s with an average of s . where h is not detected the upper limits on the ionization rate are consistent with this range . the average value of is about an order of magn...	using high resolution infrared spectroscopy we have surveyed twenty sightlines for h absorption . h is detected in eight diffuse cloud sightlines with column densities varying from to . this brings to fourteen the total number of diffuse cloud sightlines where h has been detected . these detections are mostly alo...
1210.6353	i	both theoretically and observationally , core - collapse supernova ( ccsn ) explosions are linked with the death of massive stars . however , because precise measurements of ccsn progenitor masses are scarce , the mapping between explosion scenario and the progenitor mass distribution is less clear . the most common me...	application of stellar evolution models allows us to infer thefrom this age . because our technique is not contingent on identification or precise location of the progenitor star , it can be applied to the location of any known snr . if we assume a single power law distribution , , we find a distribution that is steepe...	using hubble space telescope ( hst ) photometry , we age - date 59 supernova remnants ( snrs ) in the spiral galaxy m31 and use these ages to estimate zero - age main sequence masses ( ) for their progenitors . to accomplish this , we create color - magnitude diagrams ( cmds ) and employ cmd fitting to measure the rece...
1210.6353	m	the basic procedure for deriving a mass estimate for each progenitor is as follows . we first use coordinates from three snr catalogs as explained in 2.2 , which we assume are accurate to within a few arcseconds and unbiased to any one type of sn . we then search for any appropriate hst fields that contain the snr in ...	, we create color - magnitude diagrams ( cmds ) and employ cmd fitting to measure the recent star formation history ( sfh ) of the regions surrounding cataloged snr sites . we identify any young coeval population that likely produced the progenitor star , then assign an age and uncertainty to that population . we ident...	using hubble space telescope ( hst ) photometry , we age - date 59 supernova remnants ( snrs ) in the spiral galaxy m31 and use these ages to estimate zero - age main sequence masses ( ) for their progenitors . to accomplish this , we create color - magnitude diagrams ( cmds ) and employ cmd fitting to measure the rece...
1210.6353	c	our method measures the prominence of a burst as a fraction of the total recent sf . this approach requires that we define the period of time that we consider as `` recent '' sf . specifically , we must identify the age range where star formation can produce stars massive enough to result in ccsne . theoretical argumen...	using hubble space telescope ( hst ) photometry , we age - date 59 supernova remnants ( snrs ) in the spiral galaxy m31 and use these ages to estimate zero - age main sequence masses ( ) for their progenitors . to accomplish this we consider the remaining 6 snrs as either probable type ia candidates or the result of co...	using hubble space telescope ( hst ) photometry , we age - date 59 supernova remnants ( snrs ) in the spiral galaxy m31 and use these ages to estimate zero - age main sequence masses ( ) for their progenitors . to accomplish this , we create color - magnitude diagrams ( cmds ) and employ cmd fitting to measure the rece...
1502.03583	r	in bulk a fluid of hard rectangles of aspect ratio @xmath1 undergoes a phase transition from an isotropic to a nematic phase upon increasing the density @xcite . the bulk transition is continuous , presumably of the kosterlitz - thouless type @xcite . the aim of the present work is to study confinement properties , and...	we present results for the state diagram as a function of the packing fraction and the degree of confinement . under extreme confinement , unexpected states appear with lower symmetries than those of the corresponding stable states in bulk , such as the formation of states that break the anchoring constraints or the sy...	using monte carlo simulation , we analyse the behaviour of two - dimensional hard rods in four different types of geometric confinement : ( i ) a slit pore where the particles are confined between two parallel walls with homeotropic anchoring ; ( ii ) a hybrid slit pore formed by a planar and a homeotropic wall ; squar...
1502.03583	c	in summary , we have performed a systematic analysis of the behaviour of two - dimensional hard rods confined in slit pores and in square cavities . in the case of slit pores we have shown that our simple hard core model contains much of the phenomenology observed in corresponding confined three dimensional systems . e...	using monte carlo simulation , we analyse the behaviour of two - dimensional hard rods in four different types of geometric confinement : ( i ) a slit pore where the particles are confined between two parallel walls with homeotropic anchoring ; ( ii ) a hybrid slit pore formed by a planar and a homeotropic wall ; squar...	using monte carlo simulation , we analyse the behaviour of two - dimensional hard rods in four different types of geometric confinement : ( i ) a slit pore where the particles are confined between two parallel walls with homeotropic anchoring ; ( ii ) a hybrid slit pore formed by a planar and a homeotropic wall ; squar...
1009.2140	i	the magnetic field is an essential ingredient in present - day star formation . observations have shown that molecular cloud cores have magnetic energy comparable to gravitational energy @xcite . the cloud cores also have angular momentum @xcite . stars are born in such cloud cores . as the cloud collapses , the centra...	, however , the circumstellar disk grows rapidly and exceedsau by the end of the main accretion phase . this rapid growth of the circumstellar disk is caused by the depletion of the infalling envelope , while magnetic braking is effective when the infalling envelope is more massive than the circumstellar disk . the inf...	using resistive magnetohydrodynamics simulation , we investigate circumstellar disk formation in a strongly magnetized cloud . as the initial state , an isolated cloud core embedded in a low - density interstellar medium with a uniform magnetic field is adopted . the cloud evolution is calculated until almost all gas i...
1009.2140	c	in this paper , to investigate the formation of the circumstellar disk in a realistic setting , we set a dense molecular cloud core embedded in a low - density interstellar medium in a large simulation box with size 16 times the radius of the molecular cloud core , in which a uniform magnetic field parallel to the rota...	using resistive magnetohydrodynamics simulation , we investigate circumstellar disk formation in a strongly magnetized cloud . as the initial state , an isolated cloud core embedded in a low - density interstellar medium with a uniform magnetic field the cloud evolution is calculated until almost all gas inside the ini...	using resistive magnetohydrodynamics simulation , we investigate circumstellar disk formation in a strongly magnetized cloud . as the initial state , an isolated cloud core embedded in a low - density interstellar medium with a uniform magnetic field is adopted . the cloud evolution is calculated until almost all gas i...
0706.2473	c	we use the simple population synthesis to model the stellar contributions in double - peaked sdss agns . the reliable stellar velocity dispersions are obtained for 52 medium - luminous double - peaked sdss agns with obvious stellar features . we find that : 1 ) the black hole mass is from @xmath173 to @xmath174 and the...	the stellar velocity dispersions ( ) are obtained for 52 double - peaked agns with obvious stellar absorption features , ranging from 106 to 284 ^-1 km s . the black hole masses are calculated to range from to , and the eddington ratio from about 0.01 to about 1 . we find that far deviates from 0.75 , suggesting the n...	using the stellar population synthesis , we model the stellar contribution for a sample of 110 double - peaked broad - lines agns from the sloan digital sky survey ( sdss ) . the stellar velocity dispersions ( ) are obtained for 52 double - peaked agns with obvious stellar absorption features , ranging from 106 to 284 ...
1511.04705	c	we have investigated , by means of numerical transfer - matrix approach in the angular - momentum space , the effects of the skew - interlayer hopping integrals ( the trigonal warping ) on selected transport characteristics of bilayer - graphene ( blg ) corbino disks . additionally , the analytical mode - matching for ...	using the transfer matrix in the angular - momentum space we investigate the impact of trigonal warping on magnetotransport and scaling properties of a ballistic bilayer graphene in the corbino geometry . although the conductivity at the charge - neutrality point and zero magnetic field exhibits a one - parameter scal...	using the transfer matrix in the angular - momentum space we investigate the impact of trigonal warping on magnetotransport and scaling properties of a ballistic bilayer graphene in the corbino geometry . although the conductivity at the charge - neutrality point and zero magnetic field exhibits a one - parameter scal...
1010.4673	i	this article is about the properties of a quantum statistical ensemble , which is , in a sense , opposite to the conventional micro - canonical ensemble . it is an extension of the previous work of one of us@xcite . the present work contains a discussion of underlying conceptual issues and detailed analytical and numer...	usual approach to the foundations of quantum statistical physics is based on conventional micro - canonical ensemble as a starting point for deriving boltzmann - gibbs ( bg ) equilibrium . it leaves , however , a number of conceptual and practical questions unanswered . here we discuss these questions , thereby motivat...	usual approach to the foundations of quantum statistical physics is based on conventional micro - canonical ensemble as a starting point for deriving boltzmann - gibbs ( bg ) equilibrium . it leaves , however , a number of conceptual and practical questions unanswered . here we discuss these questions , thereby motivat...
1010.4673	c	in conclusion , we have demonstrated that the large-@xmath29 analytical description of the qmc ensemble developed in ref.@xcite allows one to make good predictions for the monte - carlo sampling of the qmc ensemble for finite-@xmath29 systems . the description of ref.@xcite is amenable to finite-@xmath29 corrections , ...	we demonstrate that the variance of energy fluctuations can be used to discriminate the qmc equilibrium from the bg equilibrium . we further suggest that the reason , why bg equilibrium commonly occurs in nature rather than the qmc - type equilibrium , has something to do with the notion of quantum collapse .	usual approach to the foundations of quantum statistical physics is based on conventional micro - canonical ensemble as a starting point for deriving boltzmann - gibbs ( bg ) equilibrium . it leaves , however , a number of conceptual and practical questions unanswered . here we discuss these questions , thereby motivat...
1412.1086	i	several recent experiments @xcite have provided strong evidence for a dramatic change in the nature of the low temperature electronic state of the hole - doped cuprate superconductors near optimal doping ( @xmath0 ) . moreover , zero field photoemission experiments carried out in the normal state have seen evidence for...	the theory contains a quantum phase transition between metals with large and small fermi surfaces of spinless fermions carrying the electromagnetic charge of the electron , but the transition does not directly involve any broken global symmetries . this higgs field measures the local antiferromagnetic correlations in a...	we analyze a candidate theory for the strange metal near optimal hole - doping in the cuprate superconductors . the theory contains a quantum phase transition between metals with large and small fermi surfaces of spinless fermions carrying the electromagnetic charge of the electron , but the transition does not directl...
0801.2159	i	the galactic bulge underwent an intense burst of star formation early in the formation of the galaxy , leading to a very different stellar population and chemical evolution history than found in the milky way disk or halo ( e.g. , * ? ? ? * ; * ? ? ? * ; * ? ? ? * ) . in particular , massive stars may dominate the poll...	we analyze a high - resolution spectrum of a microlensed g - dwarf in the galactic bulge , acquired when the star was magnified by a factor of 110 . we find that the abundance ratios of alpha and iron - peak elements are similar to those of bulge giants with the same metallicity .	we analyze a high - resolution spectrum of a microlensed g - dwarf in the galactic bulge , acquired when the star was magnified by a factor of 110 . we measure a spectroscopic temperature , derived from the wings of the balmer lines , that is the same as the photometric temperature , derived using the color determined ...
0801.2159	r	in table 2 , we summarize the abundances measured for 17 elements in . we include both log@xmath54 and its error , as well as [ x / fe ] and its error . to give an idea of the uncertainty due to scatter from the lines , rather than from atmospheric parameters , we give @xmath57 , the rms of abundances derived from ind...	for the first time , we measure the abundances of k and zn for a star in the bulge . the [ k / mg ] ratio is similar to the value measured in the halo and the disk , suggesting that k production closely tracks production . the [ cu / fe ] and [ zn / fe ] ratios support the theory that those elements are produced in typ...	we analyze a high - resolution spectrum of a microlensed g - dwarf in the galactic bulge , acquired when the star was magnified by a factor of 110 . we measure a spectroscopic temperature , derived from the wings of the balmer lines , that is the same as the photometric temperature , derived using the color determined ...
astro-ph0110235	c	the previous section shows that a simple analysis , not taking into account morphology or activity level ( h@xmath0 luminosity ) of the galaxies , gives that the percentage of liners , transition and absorption line galaxies with nearby companions is significantly higher than that of seyferts and hii galaxies . this re...	the comparison of the percentage of galaxies with nearby companions showed that there is a higher percentage of liners , transition , and absorption line galaxies with companions than seyferts and hii galaxies . however , we find that when we consider only galaxies of similar morphological types ( ellipticals or spiral...	we analyze the idea that nuclear activity , either agn or star formation , can be triggered by interactions , studying the percentage of active , hii and quiescent galaxies with companions . our sample was selected from the palomar survey , and avoids selection biases faced by previous studies . this sample was split i...
astro-ph0703350	i	fluorescent fe k lines are common in the x - ray spectra of accreting black holes , ranging from x - ray binaries to active galactic nuclei ( agns ) , and provide one of the best probes for studying accretion disks . if the fe k line is emitted from the inner part of the accretion disk , it becomes broad and asymmetric...	we analyze x - ray spectra of 43 palomar - green quasars observed with _ a feature resembling an emission line at 6.4 kev , identified with an fe k line , is detected in 33 objects . the fe line is relatively narrow (kev ) , with a center energy of 6.48kev and a mean equivalent width ( ew ) of 248ev . by combining blac...	we analyze x - ray spectra of 43 palomar - green quasars observed with _ xmm - newton _ in order to investigate their mean fe k line profile and its dependence on physical properties . the continuum spectra of 39 objects are well reproduced by a model consisting of a power law and a blackbody modified by galactic absor...
astro-ph0703350	r	the spectra of most objects are not well represented by a simple power law ; soft excess emission and an emission line - like feature around 6 kev are also often seen . therefore , we considered a model consisting of a power law , a blackbody component to represent the soft excess emission below @xmath9 2kev , and a ga...	xmm - newton _ in order to investigate their mean fe k line profile and its dependence on physical properties . approximately half of the sample show an absorption feature around 0.650.95 kev , which is due to absorption lines and edges of and . we fit the entire sample simultaneously to derive average fe line paramete...	we analyze x - ray spectra of 43 palomar - green quasars observed with _ xmm - newton _ in order to investigate their mean fe k line profile and its dependence on physical properties . the continuum spectra of 39 objects are well reproduced by a model consisting of a power law and a blackbody modified by galactic absor...
astro-ph0703350	c	we examined mean fe k line shapes for the four groups sorted by the eddington ratios , and found that the peak energy , width , and equivalent width become higher ( 6.4 to 6.8kev ) , broader ( 0.1 to 0.7kev ) , and larger ( 130 to 280ev ) , respectively , as the eddington ratio increases . in this section , we discuss ...	we examine the dependence of the fe k line profile on eddington ratio . as the eddington ratio increases , the line becomes systematically stronger ( ew = 130 to 280 ev ) , broader ( to 0.7kev ) , and peaks at higher energies ( 6.4 to 6.8kev ) .	we analyze x - ray spectra of 43 palomar - green quasars observed with _ xmm - newton _ in order to investigate their mean fe k line profile and its dependence on physical properties . the continuum spectra of 39 objects are well reproduced by a model consisting of a power law and a blackbody modified by galactic absor...
1101.5939	i	in this paper , we have investigated s - wave proton deuteron scattering in pionless effective field theory . in the quartet channel , we have calculated the elastic scattering phase shift up to using the power counting for coulomb contributions suggested by rupak and kong @xcite . the coulomb effects are included a...	deuteron scattering in the framework of pionless effective field theory . in the quartet channel , we calculate the elastic scattering phase shift up to next - to - next - to - leading order in the power counting . in the doublet channel , we perform a next - to - leading order calculation . we obtain good agreement wi...	we calculate low - energy proton deuteron scattering in the framework of pionless effective field theory . in the quartet channel , we calculate the elastic scattering phase shift up to next - to - next - to - leading order in the power counting . in the doublet channel , we perform a next - to - leading order calcula...
1112.5070	i	let @xmath0 be a standard one - dimensional brownian motion , @xmath1 be an integer , and let @xmath2 be a symmetric element of @xmath3 . denote by @xmath4 the @xmath5-tuple wiener - it integral of @xmath2 with respect to @xmath6 . it is well known that multiple wiener - it integrals of different orders are uncorrelate...	we characterize the asymptotic independence between blocks consisting of multiple wiener - it integrals . as a consequence of this characterization , we derive the celebrated fourth moment theorem of nualart and peccati , its multidimensional extension , and other related results on the multivariate convergence of mult...	we characterize the asymptotic independence between blocks consisting of multiple wiener - it integrals . as a consequence of this characterization , we derive the celebrated fourth moment theorem of nualart and peccati , its multidimensional extension , and other related results on the multivariate convergence of mult...
1602.06556	c	we have investigated pair creation by the schwinger mechanism in @xmath7 . specifically , we considered a charged massive scalar field coupled to a constant background electric field in @xmath7 . after the canonical quantization , bogoliubov coefficients were obtained , and then the decay rate and the density of create...	we consider a charged scalar field in a-dimensional de sitter spacetime and investigate pair creation by a schwinger mechanism in a constant electric field background . using a semiclassical approximation we find that the semiclassical current of the created pairs in the strong electric field limit responds as . going...	we consider a charged scalar field in a-dimensional de sitter spacetime and investigate pair creation by a schwinger mechanism in a constant electric field background . using a semiclassical approximation the current of the created pairs has been estimated . we find that the semiclassical current of the created pairs ...
0709.4581	i	for more than two decades milgrom s modified newtonian dynamics ( mond ) mond has been able to explain galaxy rotation curves which are conventionally considered as an evidence of cold dark matter ( cdm ) on galactic scales . mond modifies newton s second law of motion to @xmath1 where @xmath2 and @xmath3 are the accel...	the spacetime splitting approach is used to derive covariant and gauge invariant perturbation equations which are valid for a general class of lagrangians . restricting attention to the parameter space of these theories we also study the implications for late - time cosmology and find that the evolution of photon and n...	we consider cosmology in the einstein - ther theory ( the generally covariant theory of gravitation coupled to a dynamical timelike lorentz - violating vector field ) with a linear - lagrangian . the spacetime splitting approach is used to derive covariant and gauge invariant perturbation equations which are valid for...
0709.4581	c	in this paper we have studied the cosmology of the einstein- ther theory . after presenting the general field equations for such theories in the cgi formalism , we focussed on a specific class of models described in eq . ( [ eq : aelagrangian ] ) , and confined ourselves to the parameter space of models described by eq...	we consider cosmology in the einstein - ther theory ( the generally covariant theory of gravitation coupled to a dynamical timelike lorentz - violating vector field ) with a linear - lagrangian . the primordial power - spectrum of scalar perturbations in this model is shown to be the same that predicted by standard ge...	we consider cosmology in the einstein - ther theory ( the generally covariant theory of gravitation coupled to a dynamical timelike lorentz - violating vector field ) with a linear - lagrangian . the spacetime splitting approach is used to derive covariant and gauge invariant perturbation equations which are valid for...
0805.4309	i	the kerr family , discovered in 1963 @xcite , comprises perhaps the most important family of exact solutions to the einstein vacuum equations @xmath18 the governing equations of general relativity . for parameter values @xmath19 ( here @xmath1 denotes the mass and @xmath0 angular momentum per unit mass ) , the kerr so...	we consider kerr spacetimes with parameters and such that , kerr - newman spacetimes with parameters , , and more generally , stationary axisymmetric black hole exterior spacetimes which are sufficiently close to a schwarzschild metric with parameter , with appropriate geometric assumptions on the plane spanned by the ...	we consider kerr spacetimes with parameters and such that , kerr - newman spacetimes with parameters , , and more generally , stationary axisymmetric black hole exterior spacetimes which are sufficiently close to a schwarzschild metric with parameter , with appropriate geometric assumptions on the plane spanned by the ...
cond-mat0210211	i	the problem of electron motion in a disordered conductor in a periodic potential and strong magnetic field displays a rich combination of phenomena of both classical and quantum origin . the complexity arises from the appearance of two independent types of periodicities , of the potential and of the cyclotron orbits , ...	we consider magnetotransport in a disordered two - dimensional electron gas in the presence of a periodic modulation in one direction . existing quasiclassical and quantum approaches to this problem account for weiss oscillations in the resistivity tensor at moderate magnetic fields , as well as a strong modulation - i...	we consider magnetotransport in a disordered two - dimensional electron gas in the presence of a periodic modulation in one direction . existing quasiclassical and quantum approaches to this problem account for weiss oscillations in the resistivity tensor at moderate magnetic fields , as well as a strong modulation - i...
1210.3841	i	let @xmath8 be an algebraically closed field and @xmath9 be integers with @xmath10 . let @xmath11 denote the affine variety in @xmath12 defined by the vanishing of all @xmath13 minors of an @xmath3 matrix whose entries are independent indeterminates over @xmath8 . equivalently , @xmath11 is the locus of @xmath3 matrice...	when , this jet scheme has two irreducible components : a trivial component , isomorphic to an affine space , and a nontrivial component that is the closure of the jets supported over the smooth locus of . this second component is referred to as the _ principal component _ of ; it is , in fact , a cone and can also be ...	we consider the affine variety of first order jets over , where is the classical determinantal variety given by the vanishing of all minors of a generic matrix . when , this jet scheme has two irreducible components : a trivial component , isomorphic to an affine space , and a nontrivial component that is the closure o...
1502.05655	i	we consider a discrete - time complex valued branching random walk . the system starts with an initial particle , called the root , at time @xmath0 . at time @xmath1 , the particle dies and gives birth to @xmath2 particles , which form the particles at generation @xmath3 . at time @xmath4 , each of these particles dies...	@addtoreset p l [ section ] [ theorem]definition [ theorem]lemma [ theorem]proposition [ theorem]remark [ theorem]corollary [ theorem]conjecture * key words or phrases : * branching random walk , complex weights , boundary case , diffusivity . * msc 2000 subject classifications : 60j80 , 60g57 , 6...	we consider the complex branching random walk on a dyadic tree with gaussian weights on the boundary between the diffuse phase and the glassy phase . we study the branching random walk in the space of continuous functions and establish convergence in this space . the main difficulty here is that the expected modulus of...