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article_id stringlengths 9 15	section_id stringclasses 5 values	document stringlengths 503 67.8k	summary stringlengths 205 16.2k	abstract stringlengths 293 26.7k
nlin0607066	c	in this paper we have analyzed asymptotic behavior of the single - time structure functions @xmath300 of a passively advected scalar field by the compressible velocity field with small - scale anisotropy by using the field - theoretic renormalization group and the operator product expansion in a minimal - subtraction s...	model of a passive scalar field advected by the compressible gaussian strongly anisotropic velocity field with the covariance is studied by using the field theoretic renormalization group and the operator product expansion . it is shown that , as in the isotropic case , the presence of compressibility leads to the decr...	model of a passive scalar field advected by the compressible gaussian strongly anisotropic velocity field with the covariance is studied by using the field theoretic renormalization group and the operator product expansion . the inertial - range stability of the corresponding scaling regime is established . the anomalo...
hep-ph0501161	i	in the standard model(sm ) with fifteen fermions per family neutrinos are strictly massless and the charged leptons weak eigenstates can be chosen to be their mass eigenstates . thus , each generation has a separately conserved lepton number . if one neglects the tiny effects from nonperturbative processes , there is n...	models involving large extra spatial dimension(s ) have interesting predictions on lepton flavor violating processes . we show that in the models we discussed the branching ratio of like rare process is much smaller than the ones of like processes . this is in sharp contrast to most of the traditional wisdom based on f...	models involving large extra spatial dimension(s ) have interesting predictions on lepton flavor violating processes . we consider some 5d models which are related to neutrino mass generation or address the fermion masses hierarchy problem . we study the signatures in low energy experiments that can discriminate the di...
hep-ph0501161	c	we have studied and reviewed lfv processes in 5d gauge models that are related to neutrino mass generation or address the flavor problem . specifically we focus on two complete models which generate neutrino masses radiatively . this allows us to see in detail how the two issues can be related . the models are based on...	we consider some 5d models which are related to neutrino mass generation or address the fermion masses hierarchy problem . the focus is on muon - electron conversion in nuclei , and processes and their counterparts . moreover , some rare tau decays are more promising than the rare muon decays .	models involving large extra spatial dimension(s ) have interesting predictions on lepton flavor violating processes . we consider some 5d models which are related to neutrino mass generation or address the fermion masses hierarchy problem . we study the signatures in low energy experiments that can discriminate the di...
cond-mat0401007	i	in this study we have investigated the effects of moderate - to - large smooth disorder on the hofstadter butterfly expected for 2des in a perpendicular magnetic field and a pure periodic modulation . the parameters of our study are chosen so as to be suitable for the interpretation of recent experiments on a two dimen...	motivated by the recent experiments on periodically modulated , two dimensional electron systems placed in large transversal magnetic fields , we investigate the interplay between the effects of disorder and periodic potentials in the integer quantum hall regime . in particular , we study the case where disorder is lar...	motivated by the recent experiments on periodically modulated , two dimensional electron systems placed in large transversal magnetic fields , we investigate the interplay between the effects of disorder and periodic potentials in the integer quantum hall regime . in particular , we study the case where disorder is lar...
cond-mat0312422	i	molecular motors are proteins that convert the free energy released from chemical reactions into directed movements @xcite . here we focus on linear cytoskeletal motors which move along cytoskeletal filaments . many of these motors are processive in the sense that a single motor molecule can move a cargo over a large d...	detachment from this line is allowed to occur with a small probability . motion in the surrounding fluid is described by symmetric random walks . results are obtained for the fraction of bound motors , their average velocity and displacement . the occurrence of protofilaments on a microtubule is modeled by internal sta...	movements of molecular motors on cytoskeletal filaments are described by directed walks on a line . detachment from this line is allowed to occur with a small probability . motion in the surrounding fluid is described by symmetric random walks . effects of detachment and reattachment are calculated by an analytical sol...
nucl-th9801009	i	most hadrons are emitted in the final stage of a relativistic heavy ion collision . they do not probe directly the hot and dense intermediate stages where quarks and gluons are expected to be the relevant physical degrees of freedom for equilibration processes . the geometrical size and dynamical state of the hadronic ...	multiparticle symmetrization effects are contributions to the spectra of bose - symmetrized states which are not the product of pairwise correlations . usually they are neglected in particle interferometric calculations which aim at determining the geometry of the boson emitting source from the measured momentum distri...	multiparticle symmetrization effects are contributions to the spectra of bose - symmetrized states which are not the product of pairwise correlations . usually they are neglected in particle interferometric calculations which aim at determining the geometry of the boson emitting source from the measured momentum distri...
nucl-th9801009	c	the zajc - pratt algorithm provides a simple technique for the calculation of multiparticle symmetrization effects in one- and two - particle spectra . based on this algorithm , we have studied to what extent multiparticle correlations steepen the slope of the one - particle and broaden the width of the two - particle ...	also , we explain how multiparticle effects modify the normalization of the two - particle correlator . the resulting normalization conserves event probabilities , which is not the case for the commonly used pair approximation . finally , we propose a new method of calculating bose - einstein weights from the output of...	multiparticle symmetrization effects are contributions to the spectra of bose - symmetrized states which are not the product of pairwise correlations . usually they are neglected in particle interferometric calculations which aim at determining the geometry of the boson emitting source from the measured momentum distri...
astro-ph0406127	i	the astrophysical theory of hydrodynamic winds began with the solar wind equations proposed by @xcite , also see @xcite . parker s model predicted that the pressure gradient between the sun s outer atmosphere and the interstellar medium would drive the wind . in subsequent years parker s solutions to the hydrodynamic e...	this structure is stable and robust despite the pulsational wave disturbances , and appears to be strongly self - regulated . observational studies support these conclusions . the numerical models also show that dust - free winds are nearly adiabatic , with little heating or cooling . an important process or group of p...	numerical models of the dynamically extended atmospheres of long period variable or mira stars have shown that their winds have a very simple , power law structure when averaged over the pulsation cycle . this structure is stable and robust despite the pulsational wave disturbances , and appears to be strongly self - r...
astro-ph0209219	i	the gamma - ray burst ( grb ) duration has a bimodal distribution ( mazets et al . 1981 ; norris et al . 1984 ; hurley 1992 ; kouveliotou et al . this indicates the existence of two distinct morphological classes of events , namely short - duration ( < 2 s ) bursts and long - duration ( > 2 s ) bursts . approxim...	observational data on the short grbs obtained with the ggs - wind konus experiment in the period from 1994 to 2002 are presented . evidence of an early x - ray and gamma - ray afterglow for some of the short grbs is discussed . the catalog is available electronically at http://www.ioffe.ru / lea / shortgrbs / catalog/.	observational data on the short grbs obtained with the ggs - wind konus experiment in the period from 1994 to 2002 are presented . the catalog currently includes 130 events , detailing their appearance rate , time histories , and energy spectra . evidence of an early x - ray and gamma - ray afterglow for some of the sh...
astro-ph0009184	i	the central @xmath1 pc of the galaxy host a phenomenon that is unique within the galaxy : narrow , `` vertical '' ( i.e. @xmath0 to the galactic plane ) filaments of radio emission that are typically a few tens of parsecs long and only a fraction of a parsec wide ( morris 1996 ) . polarization measurements indicate tha...	observations of narrow radio - emitting filaments near the galactic center have been interpreted in previous studies as evidence of a pervasive vertical ( i.e. to the galactic plane ) milligauss magnetic field in the central pc of the galaxy . a simple cylindrically symmetric model for the equilibrium in this central r...	observations of narrow radio - emitting filaments near the galactic center have been interpreted in previous studies as evidence of a pervasive vertical ( i.e. to the galactic plane ) milligauss magnetic field in the central pc of the galaxy . a simple cylindrically symmetric model for the equilibrium in this central r...
astro-ph9811128	i	by definition , gigahertz peaked spectrum ( gps ) sources have convex spectra with a turnover frequency @xmath2 ghz . it is generally accepted that such a spectral shape results from synchrotron self - absorption due to a high compactness . indeed , the linear sizes of gps sources are very small ( 101000 pc ) and the...	these sources were selected from jvas and other catalogues to have convex spectra between 1.4 and 8.4 ghz , characteristic of gigahertz peaked spectrum ( gps ) sources . we have confirmed convex shapes of the spectra of 76 objects ( one half of our initial candidates ) thereby yielding the largest genuine sample of g...	observations with merlin at 408 mhz have been used to establish the low - frequency part of the spectra of more than a hundred compact radio sources taken from the part of the jodrell bank vla astrometric survey limited by . these sources were selected from jvas and other catalogues to have convex spectra between 1.4...
astro-ph9811128	i	gigahertz peaked spectrum objects are an astrophysically significant and important class yet they are still not well understood ( odea 1998 ) . they are not necessarily a uniform class , and one can easily name subclasses among the whole gps ensemble . for example csos make one well defined group all of them are gps ...	observations with merlin at 408 mhz have been used to establish the low - frequency part of the spectra of more than a hundred compact radio sources taken from the part of the jodrell bank vla astrometric survey limited by . seven of 17 identified quasars in the sample have large ( ) redshifts .	observations with merlin at 408 mhz have been used to establish the low - frequency part of the spectra of more than a hundred compact radio sources taken from the part of the jodrell bank vla astrometric survey limited by . these sources were selected from jvas and other catalogues to have convex spectra between 1.4...
1006.3829	i	light is a natural candidate to transmit information across large networks due to its high speed and low propagation losses . a major obstacle to building more advanced optical networks is the lack of an all - optically controlled device that can robustly delay or store optical wave - packets over a tunable amount of t...	one of the major advances needed to realize all - optical information processing of light is the ability to delay or coherently store and retrieve optical information in a rapidly tunable manner . in the classical domain , such a system also has profound implications for quantum information processing , serving as a lo...	one of the major advances needed to realize all - optical information processing of light is the ability to delay or coherently store and retrieve optical information in a rapidly tunable manner . in the classical domain , this optical buffering is expected to be a key ingredient to managing the flow of information ove...
quant-ph0607046	i	one major obstacle to the fulfillment of the promise of quantum computing is the current scarcity of quantum algorithms . quantum computing researchers simply have not yet found enough quantum algorithms to determine whether or not future quantum computers will be general purpose or special purpose computing devices . ...	one of the most promising and versatile approaches to creating new quantum algorithms is based on the quantum hidden subgroup ( qhs ) paradigm , originally suggested by alexei kitaev . this class of quantum algorithms encompasses the deutsch - jozsa , simon , shor algorithms , and many more . in this paper , our st...	one of the most promising and versatile approaches to creating new quantum algorithms is based on the quantum hidden subgroup ( qhs ) paradigm , originally suggested by alexei kitaev . this class of quantum algorithms encompasses the deutsch - jozsa , simon , shor algorithms , and many more . in this paper , our st...
astro-ph0311460	i	the central @xmath2100 pc around the galactic center is an extremely complex region containing a variety of astrophysical activities : i.e. , cold and warm molecular clouds , star clusters / formation , supernova remnants ( snrs ) , and hii regions , to name a few . earlier galactic plane surveys with the _ tenma _ and...	over the last three years , the galactic center region has been monitored with the _ chandra x - ray observatory_. besides the x - ray emission from the target object , sgr a * , diffuse x - ray emission was detected throughout most of the 17 17 field of view . with 11 the detected elemental species of the galactic cen...	over the last three years , the galactic center region has been monitored with the _ chandra x - ray observatory_. besides the x - ray emission from the target object , sgr a * , diffuse x - ray emission was detected throughout most of the 17 17 field of view . with 11 _ chandra _ observations through 2002 june , the t...
astro-ph0311460	c	the bright , hard x - ray filaments to the northeast of sgr a * stand out for having strong neutral fe emission . the spectral characteristics of knot 1 , for example , are consistent with those of the sgr b2 and sgr c clouds , both of which have been plausibly described by an xrn model illuminated by past activity of ...	the detection of molecular cloud counterparts to the 6.4 kev fe line emitting features indicates that these fe line features are associated with dense galactic center clouds and/or active star - forming regions , which strongly supports the proposed origins of the x - ray reflection and/or supernova ejecta for the fe l...	over the last three years , the galactic center region has been monitored with the _ chandra x - ray observatory_. besides the x - ray emission from the target object , sgr a * , diffuse x - ray emission was detected throughout most of the 17 17 field of view . with 11 _ chandra _ observations through 2002 june , the t...
astro-ph0110419	i	butcher & oemler ( 1978a ; 1984 , hereafter bo84 ) found that the fraction of blue galaxies increases dramatically between redshifts @xmath1 = 0 and @xmath7 0.5 , now usually referred to as the butcher oemler effect ( hereafter bo effect ) . this trend has been confirmed by e.g. rakos & schombert , ellingson et al . ,...	photometric redshifts are used to determine the rest frame luminosity function ( lf ) of both early - type and late - type galaxies to -17.6 for the cluster cl1601 + 42 at = 0.54 . the total lf shows a steep faint - end slope -1.4 , indicating the existence of a numerous population of dwarf galaxies . = = = = = = = = ...	photometric redshifts are used to determine the rest frame luminosity function ( lf ) of both early - type and late - type galaxies to -17.6 for the cluster cl1601 + 42 at = 0.54 . the total lf shows a steep faint - end slope -1.4 , indicating the existence of a numerous population of dwarf galaxies . luminous galaxies...
astro-ph0110419	c	luminosity functions for galaxies fainter than @xmath97 have previously been determined for clusters to @xmath98 . comparing the lfs for coma at @xmath99 @xcite , a2554 at @xmath100 ( smith et al . 1997 ) , a963 at @xmath101 @xcite and ms2255.7 + 2039 at @xmath102 ( nslund et al . 2000 ) reveals that both nearby and di...	compared to clusters at lower redshift , the steepening of the faint end starts at brighter magnitudes for cl1601 + 42 , which may indicate a brightening of todays dwarf population relative to the giant population with increasing redshift . bright , late - type galaxies are rare , consistent with a decrease in star for...	photometric redshifts are used to determine the rest frame luminosity function ( lf ) of both early - type and late - type galaxies to -17.6 for the cluster cl1601 + 42 at = 0.54 . the total lf shows a steep faint - end slope -1.4 , indicating the existence of a numerous population of dwarf galaxies . luminous galaxies...
astro-ph0110419	c	using photometry in five broad - band filters we determine photometric redshifts for the galaxies in the field of cl1601 + 42 at @xmath186 . cluster membership can therefore be assigned with a higher reliability for the individual galaxies , which , compared to statistical methods , significantly reduces the amount of ...	luminous galaxies , with are mostly red , early - type galaxies , with a lf best described by a gaussian . faint galaxies are predominantly blue , late - type galaxies , well fitted by a schechter function with -1.7 . early - type galaxies are centrally concentrated , and dominate the core region , implying that the ra...	photometric redshifts are used to determine the rest frame luminosity function ( lf ) of both early - type and late - type galaxies to -17.6 for the cluster cl1601 + 42 at = 0.54 . the total lf shows a steep faint - end slope -1.4 , indicating the existence of a numerous population of dwarf galaxies . luminous galaxies...
1512.03774	i	the maximum of the nucleon vector analyzing power , @xmath3 , and the deuteron vector analyzing power , @xmath4 , in neutron - deuteron ( @xmath7 ) and proton - deuteron ( @xmath8 ) scattering are significantly underpredicted by existing three - body calculations at low energies ( nucleon laboratory energies below @xma...	polarization observables in neutron - deuteron scattering are calculated to next - to - next - to - next - to - leading order ( ) in pionless effective field theory ( ) . at the two - body-wave contact interactions are found to be important contributions to the neutron vector analyzing power , , and the deuteron vector...	polarization observables in neutron - deuteron scattering are calculated to next - to - next - to - next - to - leading order ( ) in pionless effective field theory ( ) . at the two - body-wave contact interactions are found to be important contributions to the neutron vector analyzing power , , and the deuteron vector...
1109.5086	i	the model of random interlacements was recently introduced by sznitman in @xcite in order to describe the local picture left by the trajectory of a random walk on the discrete torus @xmath6 , @xmath7 when it runs up to times of order @xmath8 , or on the discrete cylinder @xmath9 , @xmath10 , when it runs up to times of...	random interlacements ( at level ) is a one parameter family of random subsets of introduced by sznitman in . the vacant set at level is the complement of the random interlacement at level . while the random interlacement induces a connected subgraph of for all levels , the vacant set has a non - trivial phase transiti...	random interlacements ( at level ) is a one parameter family of random subsets of introduced by sznitman in . the vacant set at level is the complement of the random interlacement at level . while the random interlacement induces a connected subgraph of for all levels , the vacant set has a non - trivial phase transiti...
hep-th0606066	i	in this paper , the proposal in @xcite that the rank - three tensor model can be used as theory of dynamical fuzzy spaces is applied to dynamical generation of commutative nonassociative fuzzy spaces . it is numerically shown that fuzzy flat torus and fuzzy spheres of various dimensions are classical solutions of the r...	rank - three tensor model may be regarded as theory of dynamical fuzzy spaces , because a fuzzy space is defined by a three - index coefficient of the product between functions on it , . in this paper , this previous proposal is applied to dynamical generation of commutative nonassociative fuzzy spaces . it is numerica...	rank - three tensor model may be regarded as theory of dynamical fuzzy spaces , because a fuzzy space is defined by a three - index coefficient of the product between functions on it , . in this paper , this previous proposal is applied to dynamical generation of commutative nonassociative fuzzy spaces . it is numerica...
1406.0274	c	we developed a phase - reduction theory for limit - cycle solutions of infinite - dimensional rd systems and illustrated its validity by analyzing mutual synchronization of a pair of rd systems exhibiting rhythmic dynamics . our theory does not assume rigidity and spatial symmetry ; therefore , it is generally applicab...	we develop a phase - reduction theory for stable limit - cycle solutions of infinite - dimensional reaction - diffusion systems . by generalizing the notion of isochrons to functional space , the phase sensitivity function nontrivial phase response properties and synchronization dynamics are revealed , reflecting their...	reaction - diffusion systems can describe a wide class of rhythmic spatiotemporal patterns observed in chemical and biological systems , such as circulating pulses on a ring , oscillating spots , target waves , and rotating spirals . these rhythmic dynamics can be considered limit cycles of reaction - diffusion systems...
1110.0845	i	ghost imaging is a transverse active - imaging technique that exploits the correlation between two light beams to image a target without spatially - resolving measurements of the light beam that has undergone target interaction . the two beams are the signal , which interacts with the target and then is measured by a s...	recent work has indicated that ghost imaging may have applications in standoff sensing . however , most theoretical work has addressed transmission - based ghost imaging . to be a viable remote - sensing system , the ghost imager needs to image rough - surfaced targets in reflection through long , turbulent optical pat...	recent work has indicated that ghost imaging may have applications in standoff sensing . however , most theoretical work has addressed transmission - based ghost imaging . to be a viable remote - sensing system , the ghost imager needs to image rough - surfaced targets in reflection through long , turbulent optical pat...
math0302200	i	unlike chaos in finite dimensional systems , the area of chaos in partial differential equations has been a long standing open field . during the past ten years , there have been some remarkable developments in the area of chaos in partial differential equations by the author and collaborators . our main results can be...	recently , the author and collaborators have developed a systematic program for proving the existence of homoclinic orbits in partial differential equations . two typical forms of homoclinic orbits thus obtained are : ( 1 ) silnikov homoclinic orbits . around the transversal homoclinic orbits in infinite dimensional au...	recently , the author and collaborators have developed a systematic program for proving the existence of homoclinic orbits in partial differential equations . two typical forms of homoclinic orbits thus obtained are : ( 1 ) . transversal homoclinic orbits , ( 2 ) . silnikov homoclinic orbits . around the transversal ho...
1207.6737	i	this paper is about an efficient numerical solver for elliptic boundary value problems in piecewise smooth domains . such a solver is useful for applications in physics and engineering , where computational domains of interest often have boundaries that contain singular points such as corners and triple junctions . fur...	recursively compressed inverse preconditioning ( rcip ) is a numerical method for obtaining highly accurate solutions to integral equations on piecewise smooth surfaces . the purpose of the present paper is threefold : first , to review the rcip method in a simple setting . second , to show how easily the method can be...	recursively compressed inverse preconditioning ( rcip ) is a numerical method for obtaining highly accurate solutions to integral equations on piecewise smooth surfaces . the method originated in 2008 as a technique for solving laplace s equation in two - dimensional domains with corners . in a series of subsequent pap...
1207.6737	i	the line of research on fast solvers for elliptic boundary value problems in piecewise smooth domains , leading up to the rcip method , grew out of work in computational fracture mechanics . early efforts concerned finding efficient integral equation formulations . corner singularities were either resolved with brute f...	the method originated in 2008 as a technique for solving laplace s equation in two - dimensional domains with corners . in a series of subsequent papers the technique was then refined and extended in various directions as to cover a broad range of boundary value problems in physics and engineering .	recursively compressed inverse preconditioning ( rcip ) is a numerical method for obtaining highly accurate solutions to integral equations on piecewise smooth surfaces . the method originated in 2008 as a technique for solving laplace s equation in two - dimensional domains with corners . in a series of subsequent pap...
1502.02938	i	within the quantum world , the question what quantities can be measured in an experiment is often a non - trivial one , e.g. , measuring time correlators ( with times @xmath0 ) requires finding the correct ordering of operators . concrete examples in mesoscopic physics and quantum optics are the measurements of charge ...	repeated measurements as typically occurring in two- or multi - time correlators rely on von neumann s projection postulate , telling how to restart the system after an intermediate measurement . we invoke the principle of deferred measurement to describe an alternative procedure where co - evolving quantum memories ex...	repeated measurements as typically occurring in two- or multi - time correlators rely on von neumann s projection postulate , telling how to restart the system after an intermediate measurement . we invoke the principle of deferred measurement to describe an alternative procedure where co - evolving quantum memories ex...
1105.6343	i	magnetic reconnection is one of the most important processes in plasma physics . it appears in a variety of phenomena in geo / astrophysics and fusion physics , which include dynamo , solar and stellar flares , magnetospheric substorms , disruptions in fusion devices , etc . in the framework of magnetohydrodynamics ( m...	roles of turbulence in the context of magnetic reconnection are investigated with special emphasis on the mutual interaction between flow ( large - scale inhomogeneous structure ) and turbulence . in order to evaluate the effective transport due to turbulence , in addition to the _ intensity _ information of turbulence...	roles of turbulence in the context of magnetic reconnection are investigated with special emphasis on the mutual interaction between flow ( large - scale inhomogeneous structure ) and turbulence . in order to evaluate the effective transport due to turbulence , in addition to the _ intensity _ information of turbulence...
1202.4357	i	recent advances in the observational cosmology make it real to start probing the most intriguing aspects of the universe . in particular , it is of importance to inquire whether the statistical isotropy of the scalar perturbations is exact or only approximate . this issue is of special interest because the statistical ...	search for the statistical anisotropy in the cmb data is a powerful tool for constraining models of the early universe . in this paper we focus on the recently proposed cosmological scenario with conformal rolling . we consider two sub - scenarios , one of which involves a long intermediate stage between conformal roll...	search for the statistical anisotropy in the cmb data is a powerful tool for constraining models of the early universe . in this paper we focus on the recently proposed cosmological scenario with conformal rolling . we consider two sub - scenarios , one of which involves a long intermediate stage between conformal roll...
astro-ph0607427	c	in this paper , limits to the diffuse flux from seven different agn source classes could be derived from point source stacking limits from amanda . there is in many cases an additional constraint on flux models at the lowest energies : while the general diffuse limit is restricted to the energy band of @xmath22 gev to...	second generation high energy neutrino telescopes are being built to reach sensitivities of neutrino emission from galactic and extragalactic sources . current neutrino detectors are already able to set limits which are in the range of some emission models . in particular , the * antarctic muon and neutrino ...	second generation high energy neutrino telescopes are being built to reach sensitivities of neutrino emission from galactic and extragalactic sources . current neutrino detectors are already able to set limits which are in the range of some emission models . in particular , the * antarctic muon and neutrino ...
1504.01911	i	coherent emission by pulsars usually has a flux density @xmath1 in the frequency interval @xmath2 mhz with a typical spectral index @xmath3 . it is remarkable that this is true over intervals of three orders of magnitude in the rotation period @xmath4 and five orders of magnitude in the spin - down inferred magnetic di...	the primary emission spectra are broadly universal in form over many orders of magnitude in rotation period and polar - cap magnetic flux density . the existence of nulls and mode - changes in some radio - loud pulsars can be understood only as a manifestation of magnetospheric bistability . [ firstpage ] instabilit...	several classes of neutron star are sources of coherent emission at frequencies of mhz : others are radio - quiet . the primary emission spectra are broadly universal in form over many orders of magnitude in rotation period and polar - cap magnetic flux density . the existence of nulls and mode - changes in some radio ...
1504.01911	c	the ideas summarized in section 2.1 are based on well - established nuclear physics and in our view there can be no serious doubt that an ion - proton plasma is produced at the polar cap of an @xmath13 neutron star . the motivation for the series of papers cited there was the belief that the problem of plasma compositi...	an ion - proton plasma with a possible background of electron - positron pairs is formed at the polar caps of stars with positive corotational charge density and is shown here to be a physical basis for the presence or absence of coherent emission and a likely reason why bistability may be present in the later stages o...	several classes of neutron star are sources of coherent emission at frequencies of mhz : others are radio - quiet . the primary emission spectra are broadly universal in form over many orders of magnitude in rotation period and polar - cap magnetic flux density . the existence of nulls and mode - changes in some radio ...
nucl-th0002017	i	the relativistic mean - field ( rmf ) theory @xcite has proved to be successful in providing a framework for description of various facets of nuclear properties @xcite . in the rmf theory , the nuclear force is produced by a virtual exchange of various mesons . the nuclear saturation is achieved by a balance between an...	we have introduced nonlinear vector self - coupling of-meson in the rhb theory . it is shown that the inclusion of the vector self - coupling of-meson in addition to the nonlinear scalar coupling of-meson provides a good agreement with the experimental data on shell effects in nuclei about the stability line . . = c...	shell effects in nuclei about the stability line are investigated within the framework of the relativistic hartree - bogoliubov ( rhb ) theory with self - consistent finite - range pairing . using 2-neutron separation energies of ni and sn isotopes , the role of- and-meson couplings on the shell effects in nuclei is ex...
nucl-th0002017	i	we have studied the shell effects in nuclei about the stability line in the rmf theory . the chains of ni and sn isotopes have been considered , where experimental data over a large range of isospin are available . first , employing the existing forces nl - sh and nl3 with the non - linear scalar self - coupling of @xm...	shell effects in nuclei about the stability line are investigated within the framework of the relativistic hartree - bogoliubov ( rhb ) theory with self - consistent finite - range pairing . using 2-neutron separation energies of ni and sn isotopes , the role of- and-meson couplings on the shell effects in nuclei is ex...	shell effects in nuclei about the stability line are investigated within the framework of the relativistic hartree - bogoliubov ( rhb ) theory with self - consistent finite - range pairing . using 2-neutron separation energies of ni and sn isotopes , the role of- and-meson couplings on the shell effects in nuclei is ex...
1511.02026	i	elastic network models of proteins , including all - atom models@xcite and coarse - grained models@xcite represent some of the simplest and most powerful types of theoretical models that can accurately reveal structure - dynamics relationships and the mechanisms underlying a protein s functional activities @xcite . suc...	simple elastic network models of dna were developed to reveal the structure - dynamics relationships for several nucleotide sequences . second , we propose a coarse - grained elastic network model of dna , where each nucleotide is described only by one node . , we exhaustively analyzed the dynamic features of a large n...	simple elastic network models of dna were developed to reveal the structure - dynamics relationships for several nucleotide sequences . first , we propose a simple all - atom elastic network model of dna that can explain the profiles of temperature factors for several crystal structures of dna . second , we propose a c...
1511.02026	i	in this study , simple elastic network models of double - stranded dnas were developed in order to perform an exhaustive analysis of several sequence - dependent dynamical features . first , we constructed a simple all - atom elastic network model that could reproduce the fluctuations of the motifs of each nucleotide (...	first , we propose a simple all - atom elastic network model of dna that can explain the profiles of temperature factors for several crystal structures of dna . this model could effectively reproduce the detailed dynamics obtained with the all - atom elastic network model according to the sequence - dependent geometry ...	simple elastic network models of dna were developed to reveal the structure - dynamics relationships for several nucleotide sequences . first , we propose a simple all - atom elastic network model of dna that can explain the profiles of temperature factors for several crystal structures of dna . second , we propose a c...
1508.00121	l	let us consider the tensor field @xmath33 , the _ mass - momentum - energy density - flux third order four - tensor _ of a single component fluid . we assume that the tensor field is symmetric in the second and third order , as it is indicated by the symbol @xmath34 . in the following we do not explicitly denote this s...	the usual basic fields of mass , momentum , energy and their current densities , the heat flux , pressure tensor and diffusion flux are the time- and spacelike components of the third order mass - momentum - energy density - flux four - tensor . the corresponding galilean transformation rules of the physical quantities...	single component nonrelativistic dissipative fluids are treated independently of reference frames and flow - frames . first the basic fields and their balances , then the related thermodynamic relations and the entropy production are calculated and the linear constitutive relations are given . the usual basic fields...
1703.01174	i	the shockley - queisser efficiency limit for single - junction solar cells@xcite can be circumvented@xcite by a molecular process called singlet fission in which an optically excited singlet state is converted into a pair of triplet excitons , which are transiently correlated in a spin - zero state . the prospect of en...	singlet fission , the molecular process through which photons are effectively converted into pairs of lower energy triplet excitons , holds promise as a means of boosting photovoltaic device efficiencies . in the preceding article of this series , we formulated a vibronic theory of singlet fission , inspired by previou...	singlet fission , the molecular process through which photons are effectively converted into pairs of lower energy triplet excitons , holds promise as a means of boosting photovoltaic device efficiencies . in the preceding article of this series , we formulated a vibronic theory of singlet fission , inspired by previou...
astro-ph0207409	i	type ia supernovae ( sne ia ) offer arguably the most precise method to measure cosmological distances . over the last ten years , these highly luminous explosions have been used to determine distances accurate to @xmath6 , despite the fact that we know little about their progenitors . these objects show considerable ...	sn 1999aw was discovered during the first campaign of the nearby galaxies supernova search ( _ ngss _ ) project . secondly , the photometric and spectral properties of this supernova indicate that it very likely was similar to the subclass of type ia supernovae whose prototype is sn 1999aa . this paper presents the _...	sn 1999aw was discovered during the first campaign of the nearby galaxies supernova search ( _ ngss _ ) project . this luminous , slow - declining ( ) type ia supernova was noteworthy in at least two respects . first , it occurred in an extremely low luminosity host galaxy that was not visible in the template images ,...