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cond-mat0511225	i	in recent years substantial efforts have been invested in miniaturizing chemical processes by building microfluidic systems . the `` lab on a chip '' concept integrates a great variety of chemical and physical processes into a single device @xcite in a similar way as an integrated circuit incorporates many electronic d...	we investigate the flow of a nano - scale incompressible ridge of low - volatility liquid along a `` chemical channel '' : a long , straight , and completely wetting stripe embedded in a planar substrate , and sandwiched between two extended less wetting solid regions . pearling instability develops if the thickness of...	we investigate the flow of a nano - scale incompressible ridge of low - volatility liquid along a `` chemical channel '' : a long , straight , and completely wetting stripe embedded in a planar substrate , and sandwiched between two extended less wetting solid regions . molecular dynamics simulations , a simple long - ...
astro-ph0607095	i	advances in submillimeter continuum imaging techniques in the past decade have dramatically improved our understanding of the structure of the dense , cold interstellar medium ( ism ) in star - forming regions . in every region studied , the cold , dusty ism exhibits a clumpy , often filamentary structure whose density...	we investigate the mass function of cold , dusty clumps in 11 low- and high - mass star - forming regions . using a homogeneous fitting technique we find that the submillimeter continuum clump mass function in low - mass star - forming regions is typically best fit by a lognormal distribution , while that in high - mas...	we investigate the mass function of cold , dusty clumps in 11 low- and high - mass star - forming regions . using a homogeneous fitting technique , we analyze the shape of each region s clump mass function and examine the commonalities among them . we find that the submillimeter continuum clump mass function in low - m...
astro-ph0607095	i	in this paper , we have examined the issue of the functional form of the clump / core mass function derived from millimeter / submillimeter continuum observations of galactic star - forming regions . we have demonstrated that , even in the case of a strict single power - law mass function , great care must be taken in ...	fitting all of the regions with a double power law , we find the mean power law exponent at the high - mass end of each mass function is , consistent with the salpeter result of . this result is consistent with the hypothesis that the clump mass distribution is determined by a highly stochastic process , such as turbul...	we investigate the mass function of cold , dusty clumps in 11 low- and high - mass star - forming regions . using a homogeneous fitting technique , we analyze the shape of each region s clump mass function and examine the commonalities among them . we find that the submillimeter continuum clump mass function in low - m...
0904.3096	i	the rigorous , statistical confirmation of bimodality within the luminous ( @xmath0 mag ) , nearby galaxy population has proven a key result to emerge from modern wide - field imaging surveys implying the existence of two principal evolutionary pathways for bright systems . this bimodality is clearly evident in the di...	we investigate the origin of the galaxy color - concentration bimodality at the bright - end of the luminosity function ( mag ) with regard to the bulge - disc nature of galaxies . via ( 2d ) finally , within the two - component population we confirm a previously - reported correlation between bulge and disc color ( wi...	we investigate the origin of the galaxy color - concentration bimodality at the bright - end of the luminosity function ( mag ) with regard to the bulge - disc nature of galaxies . via ( 2d ) surface brightness profile modeling with gim2d , we subdivide the local galaxy population in the millennium galaxy catalogue int...
0904.3096	c	our key conclusions may be summarized as follows . via bulge - disc decomposition and quantitative morphological classification ( i.e. , the logical filter in @xcite ) of luminous ( @xmath0 mag ) , nearby ( @xmath35 ) galaxies in the mgc , we have demonstrated that : \(i ) one - component systems ( predominantly ell...	we reveal that one - component ( elliptical and disc - only ) systems define the two peaks of the galaxy color - concentration distribution ( with total stellar mass densities of and mpc respectively ) , while two - component systems contribute to both a bridging population and the red , concentrated peak ( with total ...	we investigate the origin of the galaxy color - concentration bimodality at the bright - end of the luminosity function ( mag ) with regard to the bulge - disc nature of galaxies . via ( 2d ) surface brightness profile modeling with gim2d , we subdivide the local galaxy population in the millennium galaxy catalogue int...
1302.2196	i	now that the higgs - like particle has been discovered in large hadron collider ( lhc ) @xcite , one of primary interests of particle physics is to understand mechanism of dynamical electroweak symmetry breaking . to settle down the unsolved issues including the hierarchy problem , there have been proposed several prom...	our result is qualitatively consistent with the recent lattice calculations . when fundamental quarks are introduced in addition to adjoint quarks , the split phase becomes more dominant and larger as a result of explicit center symmetry breaking . we study chiral properties in these theories and show that chiral conde...	we investigate the phase structure of gauge theory in four and five dimensions with one compact dimension by using perturbative one - loop and pnjl - model - based effective potentials , with emphasis on spontaneous gauge symmetry breaking . when adjoint matter with the periodic boundary condition is introduced , we ha...
1302.2196	i	in this paper we have studied the phase diagram for @xmath0 gauge theories with a compact spatial dimension by using the effective models , with emphasis on the dynamical gauge symmetry breaking . we show that introduction of adjoint matter with periodic boundary condition leads to the unusual phases with spontaneous g...	we investigate the phase structure of gauge theory in four and five dimensions with one compact dimension by using perturbative one - loop and pnjl - model - based effective potentials , with emphasis on spontaneous gauge symmetry breaking . when adjoint matter with the periodic boundary condition is introduced , we ha...	we investigate the phase structure of gauge theory in four and five dimensions with one compact dimension by using perturbative one - loop and pnjl - model - based effective potentials , with emphasis on spontaneous gauge symmetry breaking . when adjoint matter with the periodic boundary condition is introduced , we ha...
0812.1851	i	the astounding range of experimental and theoretical studies performed on carbon nanotubes @xcite has revealed a spectrum of physics characteristic of strongly correlated low - dimensional electronic systems @xcite . the underlying graphene lattice structure of these tubes uniquely affects band structure , effective ...	we investigate the properties of conduction electrons in single - walled armchair carbon nanotubes ( swnt ) in the presence of both transverse electric and magnetic fields . we find that these fields provide a controlled means of tuning low - energy band structure properties such as inducing gaps in the spectrum , brea...	we investigate the properties of conduction electrons in single - walled armchair carbon nanotubes ( swnt ) in the presence of both transverse electric and magnetic fields . we find that these fields provide a controlled means of tuning low - energy band structure properties such as inducing gaps in the spectrum , brea...
1209.3302	i	it has been known that nanostructures based on carbon possess unique mechanical , electrical and optical properties.@xcite among them particular attention has been given to graphene , a two - dimensional sheet of carbon atoms arranged in a hexagonal structure with low - energy electronic excitations described by the di...	we investigate the thermal casimir interaction of a suspended graphene described by the dirac model with a plate made of dielectric or metallic materials . we demonstrate that for a graphene with nonzero mass gap parameter the casimir free energy remains nearly constant ( and the thermal correction negligibly small ) o...	we investigate the thermal casimir interaction of a suspended graphene described by the dirac model with a plate made of dielectric or metallic materials . the reflection coefficients on graphene expressed in terms of a temperature - dependent polarization tensor are used . we demonstrate that for a graphene with nonze...
1209.3302	c	in the foregoing , we have investigated the casimir free energy and the thermal correction to the casimir energy at zero temperature for a suspended graphene sheet interacting with a material plate , either dielectric or metallic . in so doing graphene was described by the fully relativistic dirac model with temperatur...	the free energy is nearly the same , irrespective of whether the metal is nonmagnetic or magnetic and whether it is described using the drude- or plasma - model approaches . however , for nonmagnetic metals described by the plasma model and for magnetic metals , a severe dependence on the chosen theoretical description...	we investigate the thermal casimir interaction of a suspended graphene described by the dirac model with a plate made of dielectric or metallic materials . the reflection coefficients on graphene expressed in terms of a temperature - dependent polarization tensor are used . we demonstrate that for a graphene with nonze...
1509.04637	i	quantum markovian master equations are the simplest but also the most used cases of study for the dynamics of open quantum systems . the concept of open systems plays an important role since perfect isolation in the quantum realm and access to all degrees of freedom is not possible . the main source of inspiration was ...	we investigate two interacting open quantum systems whose time evolutions are governed by markovian master equations . we show a class of coupled systems whose interaction leaves invariant the steady state of one of the systems , i.e. , only one of the reduced steady states is sensitive to the interactions .	we investigate two interacting open quantum systems whose time evolutions are governed by markovian master equations . we show a class of coupled systems whose interaction leaves invariant the steady state of one of the systems , i.e. , only one of the reduced steady states is sensitive to the interactions . a detailed...
1502.05428	i	although the source - channel separation architecture is asymptotically optimal in the point - to - point communication setting @xcite as well as several classes of multiuser communication settings ( see _ e.g. , _ @xcite and references therein ) , uncoded schemes have several particularly attractive properties . first...	we investigate whether uncoded schemes are optimal for gaussian sources on multiuser gaussian channels . particularly , we consider two problems : the first is to send correlated gaussian sources on a gaussian broadcast channel where each receiver is interested in reconstructing only one source component ( or one speci...	we investigate whether uncoded schemes are optimal for gaussian sources on multiuser gaussian channels . particularly , we consider two problems : the first is to send correlated gaussian sources on a gaussian broadcast channel where each receiver is interested in reconstructing only one source component ( or one speci...
1205.5920	i	communication networks are presenting ever - increasing challenges in a wide range of applications , and there is great interest in inferential methods for exploiting the information they contain . a common source of such data is a corpus of time - stamped messages such as e - mails or sms ( short message service ) . s...	we model messaging activities as a hierarchical doubly stochastic point process with three main levels , and develop an iterative algorithm for inferring actors relative latent positions from a stream of messaging activity data . = 1 social network ; multiple doubly stochastic processes ; classification ; clustering...	we model messaging activities as a hierarchical doubly stochastic point process with three main levels , and develop an iterative algorithm for inferring actors relative latent positions from a stream of messaging activity data . each of the message - exchanging actors is modeled as a process in a latent space . the ac...
1205.5920	l	for statistical inference when there is information available beyond @xmath5 , the cox - proportional hazard model is a natural choice . in @xcite and @xcite , for instance , instantaneous intensity of messaging activities between each pair of actors is assumed to be a function of , in the language of generalized linea...	each of the message - exchanging actors is modeled as a process in a latent space . each actor s movement in the latent space is modeled as being governed by two parameters that we call confidence and visibility , in addition to dependence on the population distribution . the messaging frequency between a pair of actor...	we model messaging activities as a hierarchical doubly stochastic point process with three main levels , and develop an iterative algorithm for inferring actors relative latent positions from a stream of messaging activity data . each of the message - exchanging actors is modeled as a process in a latent space . the ac...
astro-ph0411655	i	of the sample of stars observed from the cfht , those with planets ( with the exception of 51 peg ) show significant night - to - night variations in their ca ii h and k reversals . @xmath5 ceti and the sun , which have no close planets , remained very steady throughout each of the four observing runs . hd 179949 a...	four stars display short - term ( days ) cyclical activity . for two , short - term chromospheric activity appears weakly dependent on the mean k - line reversal intensities for the sample of 13 stars . also , a suggestive correlation exists between this activity and thesin of the star s hot jupiter . because of their ...	we monitored the chromospheric activity in the ca ii h & k lines of 13 solar - type stars ( including the sun ) ; 8 of them over three years at the cfht and 5 in a single run at the vlt . ten of the 13 targets have close planetary companions . all of the stars observed at the cfht show long - term ( months to years ) c...
0903.0569	i	factorization theorems are fundamental to modern calculations in qcd of the amplitudes for hard - scattering exclusive hadronic processes . they allow one to separate contributions to the amplitudes that involve states of high virtuality from those that involve states of low virtuality . the former , short - distance c...	we outline a proof of factorization in exclusive processes , taking into account the presence of soft and collinear modes of arbitrarily low energy , which arise when the external lines of the process are taken on shell . specifically , we examine the process of annihilation through a virtual photon into two light meso...	we outline a proof of factorization in exclusive processes , taking into account the presence of soft and collinear modes of arbitrarily low energy , which arise when the external lines of the process are taken on shell . specifically , we examine the process of annihilation through a virtual photon into two light meso...
1212.5606	i	with what seems to be the recent discovery of the higgs boson @xcite , the high energy physics enters into the solitude of a path that no one knows where or how it may found new physics ( np ) . although a light higgs requires either , fine - tuning , or np at the tev scale , the experimental results do not show any hi...	we perform a general parton level analysis for the search of heavy resonant states in the production of pairs at the lhc with an integrated luminosity of 30 fb . we assume the existence of resonances that only couple to quarks and propose kinematic cuts in order to increase the amount of events produced through quark -...	we perform a general parton level analysis for the search of heavy resonant states in the production of pairs at the lhc with an integrated luminosity of 30 fb . we assume the existence of resonances that only couple to quarks and propose kinematic cuts in order to increase the amount of events produced through quark -...
1412.1103	c	the distribution of matter at small scales may provide insights on the nature of dark matter particles and potentially constrain scenarios alternative to the standard cold dark matter paradigm . in this work we have performed a first study of the nonlinear clustering of late - forming dark matter using a suite of high ...	we perform a study of the nonlinear clustering of matter in the late - forming dark matter ( lfdm ) scenario in which dark matter results from the transition of a nonminimally coupled scalar field from radiation to collisionless matter . the analysis of the lfdm halo velocity function shows a better agreement than thec...	we perform a study of the nonlinear clustering of matter in the late - forming dark matter ( lfdm ) scenario in which dark matter results from the transition of a nonminimally coupled scalar field from radiation to collisionless matter . a distinct feature of this model is the presence of a damped oscillatory cutoff in...
hep-th0109125	i	noncommutative field theories@xcite@xcite are obtained in an @xmath7 limit of the open string theory . this noncommutativity is inherent in the open string theory@xcite . by considering an open string in an ns - ns @xmath0 field background and taking a specific field theory limit the effects of the @xmath0 field are en...	the degrees of the freedom associated with both ends are not decoupled and accordingly , the effective action must be quite different from that of the ordinary noncommutative gauge theory for a constant background . we will then propose a prescription for reducing this bi - local effective action to that in dimensions ...	we point out that when a d - brane is placed in an ns - ns field background with non - vanishing field strength ( ) along the d - brane worldvolume , the coordinate of one end of the open string does not commute with that of the other in the low energy limit . the degrees of the freedom associated with both ends are no...
gr-qc0404080	i	investigations on how the spacetime structures would be during and after gravitational collapses are important topics in gravitational physics and spacetime physics . nonlinear nature of gravity is making our understanding of the phenomena very difficult , both conceptually and technically . steady development of numer...	the model has been introduced previously but has been awaiting for proper analysis . here the analysis is put forward : it is proved that , as far as the weak energy condition is satisfied outside the shell , the collapsing shell bounces back at some point irrespective of the initial conditions , and escapes from the s...	we prepare a general framework for analyzing the dynamics of a cylindrical shell in the spacetime with cylindrical symmetry . based on the framework , we investigate a particular model of a cylindrical shell - collapse with rotational pressure , accompanying the radiation of gravitational waves and massless particles ....
gr-qc0404080	i	in this paper , we have studied the dynamics of a cylindrical shell in the spacetime cylindrical symmetry . we have started with constructing a general framework for analyzing a cylindrical spacetime and a shell in it , which might be useful for future investigations . based on the framework , we have investigated a cy...	we prepare a general framework for analyzing the dynamics of a cylindrical shell in the spacetime with cylindrical symmetry . based on the framework , we investigate a particular model of a cylindrical shell - collapse with rotational pressure , accompanying the radiation of gravitational waves and massless particles ....	we prepare a general framework for analyzing the dynamics of a cylindrical shell in the spacetime with cylindrical symmetry . based on the framework , we investigate a particular model of a cylindrical shell - collapse with rotational pressure , accompanying the radiation of gravitational waves and massless particles ....
0707.2865	c	the observations of 3c227 , 327 and 390.3 almost all show differences between the structure observed in the radio and that observed in the x - ray . to summarize , the only ` simple ' hotspots seen in these three objects are the weak compact components in the e hotspot of 3c227 and ( probably ) the s hotspot of 3c390.3...	we find that in fact some secondary hotspots are x - ray sources , and thus probably locations for high - energy particle acceleration after the initial jet termination shock . in detail , though , we show that the spatial structures seen in x - ray are not consistent with nave expectations from a simple shock model : ...	we present _ chandra _ observations of a small sample of nearby classical double radio galaxies which have more than one radio hotspot in at least one of their lobes . the x - ray emission from the hotspots of these comparatively low - power objects is expected to be synchrotron in origin , and therefore to provide inf...
0707.2865	c	we have looked with very high spatial resolution at the hotspot x - ray emission from a small sample of radio galaxies that show multiple radio hotspots . as in earlier work , we argue that the x - ray emission from the hotspots comes predominantly from the synchrotron process , and so traces high - energy particle acc...	the x - ray emission from the hotspots of these comparatively low - power objects is expected to be synchrotron in origin , and therefore to provide information about the locations of high - energy particle acceleration . in some models of the relationship between the jet and hotspot the hotspots that are not the curre...	we present _ chandra _ observations of a small sample of nearby classical double radio galaxies which have more than one radio hotspot in at least one of their lobes . the x - ray emission from the hotspots of these comparatively low - power objects is expected to be synchrotron in origin , and therefore to provide inf...
astro-ph0105043	i	the hubble deep field north ( * ? ? ? * hereafter w96 ) ranks among the most thoroughly studied portions of the extragalactic universe . the extremely deep multi color images obtained with the wfpc2 camera on the _ hubble space telescope _ , reaching ab mag @xmath5 with 0@xmath61 resolution , have revolutionized our u...	we present a catalog of 74 galaxies detected serendipitously during a campaign of spectroscopic observations of the hubble deep field north ( hdf ) and its environs . among the identified objects are five candidate lyemitters at , a galaxy cluster at , and a chandra source with a heretofore undetermined redshift of . o...	we present a catalog of 74 galaxies detected serendipitously during a campaign of spectroscopic observations of the hubble deep field north ( hdf ) and its environs . among the identified objects are five candidate lyemitters at , a galaxy cluster at , and a chandra source with a heretofore undetermined redshift of . w...
astro-ph0105043	c	the 74 galaxies in the serendipitous catalog span the redshift range @xmath57 , with a median redshift of @xmath2 . the vast majority of the galaxies are emission - line systems ; 5% of the sample show only absorption lines . this bias stems from the diminished likelihood of serendipitously detecting an absorption lin...	we discuss the redshift distribution of the serendipitous sample , which contains galaxies in the range with a median redshift of , and we present strong evidence for redshift clustering . by comparing our spectroscopic redshifts to optical / ir photometric studies of the hdf , we find that photometric redshifts are in...	we present a catalog of 74 galaxies detected serendipitously during a campaign of spectroscopic observations of the hubble deep field north ( hdf ) and its environs . among the identified objects are five candidate lyemitters at , a galaxy cluster at , and a chandra source with a heretofore undetermined redshift of . w...
astro-ph0603163	r	as we described in section [ sec : confused ] , there are many definitions for the source confusion . we compare these definitions and propose an appropriate definition for source confusion . in table [ tab_inst_para ] , we list the basic instrumental parameters of present and future ir space missions ; the aperture of...	we present a comprehensive analysis for the determination of the confusion levels for the current and the next generation of far - infrared surveys assuming three different cosmological evolutionary scenarios . we use our derived sensitivities to suggest best survey strategies for the current and the future far - infra...	we present a comprehensive analysis for the determination of the confusion levels for the current and the next generation of far - infrared surveys assuming three different cosmological evolutionary scenarios . we include an extensive model for diffuse emission from infrared cirrus in order to derive absolute sensitivi...
0805.2980	i	there is currently considerable interest in preparing exotic quantum states of many - body systems which can be used as resource states for measurement - based quantum computation ( mbqc ) that is , quantum computation that proceeds solely through local adaptive measurements on single quantum systems @xcite . the can...	we present a general procedure for constructing lattices of qubits with a hamiltonian composed of nearest - neighbour two - body interactions such that the ground state encodes a cluster state . we give specific details for lattices in one- , two- , and three - dimensions , investigating both periodic and fixed boundar...	we present a general procedure for constructing lattices of qubits with a hamiltonian composed of nearest - neighbour two - body interactions such that the ground state encodes a cluster state . we give specific details for lattices in one- , two- , and three - dimensions , investigating both periodic and fixed boundar...
1403.0005	i	we have presented a green s function formalism , which can correctly describe two required conditions for any consistent theory of bose einstein condensates ( becs ) : ( i ) the infrared divergence of the longitudinal susceptibility in the low - energy and low - momentum limit , as well as ( ii ) the nepomnyashchii n...	we present a green s function formalism for an interacting bose einstein condensate ( bec ) satisfying the two required conditions : ( i ) the infrared - divergent longitudinal susceptibility with respect to the bec order parameter , and ( ii ) the nepomnyashchii these conditions can not be described by the ordinary ...	we present a green s function formalism for an interacting bose einstein condensate ( bec ) satisfying the two required conditions : ( i ) the infrared - divergent longitudinal susceptibility with respect to the bec order parameter , and ( ii ) the nepomnyashchii nepomnyashchii identity stating the vanishing off - di...
1201.0910	i	previously , we have compared the quality of fit provided by atmospheric models , high resolution synthetic spectra , and spectral energy distributions ( seds , @xmath4 ) computed both in lte , and with many opacity sources treated in self - consistent non - lte ( nlte ) , for the the sun and the standard stars procyon...	we present a grid of atmospheric models and synthetic spectral energy distributions ( seds ) for late - type dwarfs and giants of solar and 1/3 solar metallicity with many opacity sources computed in self - consistent non - local thermodynamic equilibrium ( nlte ) , and compare them to the lte grid of ( paper i ) .	we present a grid of atmospheric models and synthetic spectral energy distributions ( seds ) for late - type dwarfs and giants of solar and 1/3 solar metallicity with many opacity sources computed in self - consistent non - local thermodynamic equilibrium ( nlte ) , and compare them to the lte grid of ( paper i ) . we ...
0905.3556	i	gas transport to the centers of galaxies is still mainly an unsolved problem ( e.g. * ? ? ? since most of this gas is residing in a rotating disk well beyond the center , it is essentially a problem of angular momentum transport . proposed transport mechanisms range from galactic interactions and bars , to nuclear bars...	three_-arm spiral in the non - circular motions , which agrees with a _ this nuclear spiral is consistent with a weak perturbation in the gravitational potential due to a two - arm logarithmic spiral , with a pitch angle of derived directly from the harmonic expansion of the velocity field . next , we use a simple spi...	we present a harmonic expansion of the observed line - of - sight velocity field as a method to recover and investigate spiral structures in the nuclear regions of galaxies . application to the emission - line velocity field within the circumnuclear starforming ring of ngc1097 , obtained with the gmos - ifu spectrogra...
0905.3556	i	we presented harmonic expansion of the line - of - sight velocity field as a suitable method to identify and quantify possible structures in the non - circular motions , including nuclear spirals . we showed that a weak perturbation in the gravitational potential of harmonic number @xmath47 , causes the surface brightn...	we present a harmonic expansion of the observed line - of - sight velocity field as a method to recover and investigate spiral structures in the nuclear regions of galaxies . application to the emission - line velocity field within the circumnuclear starforming ring of ngc1097 , obtained with the gmos - ifu spectrogra...	we present a harmonic expansion of the observed line - of - sight velocity field as a method to recover and investigate spiral structures in the nuclear regions of galaxies . application to the emission - line velocity field within the circumnuclear starforming ring of ngc1097 , obtained with the gmos - ifu spectrogra...
1702.06957	c	using data taken with the sdss boss spectrograph , we have compiled a new empirical stellar template library . our template library : * covers spectral types o5 through l3 * includes dwarf and giant separation for spectral types a0 through m8 * contains metallicity [ fe / h ] bins for spectral types a3 through m8 * ...	the templates cover spectral types o5 through l3 , are binned by metallicity from -2.0 dex through + 1.0 dex and are separated into main sequence ( dwarf ) stars and giant stars . with recently developed m dwarf metallicity indicators , we identify trends in color space with metallicity and surface gravity , which will...	we present a library of empirical stellar spectra created using spectra from the sloan digital sky survey s baryon oscillation spectroscopic survey ( boss ) . the templates cover spectral types o5 through l3 , are binned by metallicity from -2.0 dex through + 1.0 dex and are separated into main sequence ( dwarf ) stars...
1205.5930	i	we are concerned with weakly nonlinear geometric optics for entropy solutions of the following hyperbolic system of conservation laws : @xmath2 where @xmath3 : @xmath4 is a smooth function . the jacobian matrix @xmath5 is diagonalizable at any point @xmath6 and has @xmath7 real eigenvalues such that any eigenvalue has ...	we present a new approach to analyze the validation of weakly nonlinear geometric optics for entropy solutions of nonlinear hyperbolic systems of conservation laws whose eigenvalues are allowed to have constant multiplicity and corresponding characteristic fields to be linearly degenerate . the approach is based on our...	we present a new approach to analyze the validation of weakly nonlinear geometric optics for entropy solutions of nonlinear hyperbolic systems of conservation laws whose eigenvalues are allowed to have constant multiplicity and corresponding characteristic fields to be linearly degenerate . the approach is based on our...
1208.0714	i	approximately half of the elements heavier than iron in the universe are produced via a series of @xmath12 neutron capture reactions and competing @xmath13-decays ( the @xmath9-process ) . during the @xmath9-process , the neutron number density is relatively low , of the order of 10@xmath14 n @xmath15 . when the flux r...	this is believed to have a strong effect on the rate of thec(,)o reaction , the main neutron source for _ slow _ neutron captures ( the-process ) in asymptotic giant branch ( agb ) stars . we use the new rate and different rates available in the literature as input in simulations of agb stars to study their influence o...	we present a new measurement of the-spectroscopic factor ( ) and the asymptotic normalization coefficient ( anc ) for the 6.356 mev 1/2 subthreshold state ofo through thec(b,li)o transfer reaction and we determine the-width of this state . this is believed to have a strong effect on the rate of thec(,)o reaction , the ...
1208.0714	i	we determined the stellar rate of the @xmath4c(@xmath0,@xmath7)@xmath8o reaction and incorporated the new reaction rate in calculations of the @xmath9-process nucleosynthesis in agb stars . the @xmath1 and anc for the 6.356 mev 1/2@xmath2 subthreshold state in @xmath3o were obtained from the measurement of the @xmath4c...	we present a new measurement of the-spectroscopic factor ( ) and the asymptotic normalization coefficient ( anc ) for the 6.356 mev 1/2 subthreshold state ofo through thec(b,li)o transfer reaction and we determine the-width of this state . based on the new width we derive the astrophysical s - factor and the stellar ra...	we present a new measurement of the-spectroscopic factor ( ) and the asymptotic normalization coefficient ( anc ) for the 6.356 mev 1/2 subthreshold state ofo through thec(b,li)o transfer reaction and we determine the-width of this state . this is believed to have a strong effect on the rate of thec(,)o reaction , the ...
0810.2119	i	we have presented mass models for the nearby dwarf galaxies , ic 2574 and ngc 2366 , derived using the high - resolution data from things . these high - resolution data do not suffer from beam smearing , have a well - defined dynamical center and enable us to examine in detail the dark matter distribution of these gala...	the bulk velocity field rotation curves are significantly less affected by non - circular motions and constrain the dark matter distribution in our galaxies , allowing us to address the discrepancy between the inferred and predicted dark matter distribution in galaxies ( the `` cusp / core '' problem ) . _ # 1 # 1#1	we present a new method to remove the impact of random and small - scale non - circular motions from hi velocity fields in ( dwarf ) galaxies in order to better constrain the dark matter properties for these objects . this method extracts the circularly rotating velocity components from the hi data cube and condenses t...
astro-ph0004391	c	we present a new code which is designed to derive a sed for an arbitrary spatial distribution of stellar and gaseous components for a dusty starburst galaxy . by using this code , we can calculate seds based on numerical simulations that can analyze simultaneously dynamical and chemical evolution , structural and kinem...	we present a new numerical code which is designed to derive a spectral energy distribution ( sed ) for an arbitrary spatial distribution of stellar and gaseous components in a dusty starburst galaxy . as an example , we demonstrate when and how a major galaxy merger with dusty starburst becomes an ultra - luminous infr...	we present a new numerical code which is designed to derive a spectral energy distribution ( sed ) for an arbitrary spatial distribution of stellar and gaseous components in a dusty starburst galaxy . we apply a ray tracing method to numerical simulations and thereby estimate extinction and reemission of stellar light ...
1105.5683	i	the magnetohydrodynamics ( mhd ) approximation has some interesting properties , for example , the flux freezing and magnetic pressure ; the former can be used for the collimation of the jet , and the latter for the acceleration of the plasma . thus , the magnetic field is considered an essential ingredient for many as...	we present a new numerical method of special relativistic resistive magnetohydrodynamics with scalar resistivity that can treat a range of phenomena , from nonrelativistic to relativistic ( shock , contact discontinuity , and alfvn wave ) . our new scheme is particularly well suited to systems with initially weak magne...	we present a new numerical method of special relativistic resistive magnetohydrodynamics with scalar resistivity that can treat a range of phenomena , from nonrelativistic to relativistic ( shock , contact discontinuity , and alfvn wave ) . the present scheme calculates the numerical flux of fluid by using an approxima...
1105.5683	c	in this paper , we have presented a new numerical scheme of resistive rmhd for one - dimensional case which can solve matter dominated problems more accurately than the existing numerical method . since this new scheme uses different characteristic velocity for obtaining the numerical flux of fluid and electromagnetic ...	since this scheme uses appropriate characteristic velocities , it is capable of accurately solving problems that can not be approximated as ideal magnetohydrodynamics and whose characteristic velocity is much lower than light velocity . the numerical results show that our scheme can solve the above problems as well as ...	we present a new numerical method of special relativistic resistive magnetohydrodynamics with scalar resistivity that can treat a range of phenomena , from nonrelativistic to relativistic ( shock , contact discontinuity , and alfvn wave ) . the present scheme calculates the numerical flux of fluid by using an approxima...
0901.3790	r	we now test the validity of our theory by comparing our predictions against known experimental results in hot vapors , viz . in a he * cell @xcite . for he * , collisions are expected to play a favorable role through five different effects : ( i ) vccs enable one to span the entire doppler profile quickly and efficient...	velocity - changing collisions ( vccs ) are modeled in the strong collision limit effectively , which helps in achieving optical pumping by the coupling beam across the entire doppler profile . the predictions , taking into account a dynamic rate of influx of atoms in the two lower levels of the , are in excellent agre...	we present a realistic theoretical treatment of a three - level system in a hot atomic vapor interacting with a coupling and a probe field of arbitrary strengths , leading to electromagnetically - induced transparency and slow light under the two - photon resonance condition . we take into account all the relevant deco...