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cond-mat0102521	c	in this paper we have discussed the possibility of phase ordering of a sort which is dominated by strong fluctuations . in steady state , these fluctuations lead to variations of the order parameter of order unity , but the system stays ordered in the sense that with probability one , a finite fraction of the system is...	in which the order parameter has a broad distribution even in the thermodynamic limit , the distribution of particle cluster sizes decays as a power - law ( with an exponent ) , and the 2-point spatial correlation function has a cusp ( with an exponent ) at small values of the argument .	we study a new kind of phase ordering phenomenon in coarse - grained depth models of the hill - valley profile of fluctuating surfaces with zero overall tilt , and for hard - core particles sliding on such surfaces under gravity . we find that several such systems approach an ordered state with large scale fluctuations...
cond-mat0508551	i	an equation - free framework has recently been developed as a means of computationally analyzing the dynamical behavior of a large class of complex , multiscale dynamical systems . the systems may be either stochastic or deterministic with many of degrees of freedom and subject to random initial data . the key observat...	we explore situations in which certain stochastic and high - dimensional deterministic systems behave effectively as low - dimensional dynamical systems . we define and study moment maps , maps on spaces of low - order moments of evolving distributions , as a means of understanding equations - free multiscale algorithm...	we explore situations in which certain stochastic and high - dimensional deterministic systems behave effectively as low - dimensional dynamical systems . we define and study moment maps , maps on spaces of low - order moments of evolving distributions , as a means of understanding equations - free multiscale algorithm...
1312.6226	i	the wide use of gaussian and non - gaussian electromagnetic field states for various quantum tasks and protocols renders the generation and investigation of these quantum states an essential aspect of modern research . entangled states generated using both linear and nonlinear quantum optical operations have been exten...	we investigate the states generated in continuous variable ( cv ) optical fields on operating them with a number - conserving operator of the type , formed by the generalised superposition of products of field annihilation ( ) and creation ( ) operators , with . such an operator is experimentally realizable and can be ...	we investigate the states generated in continuous variable ( cv ) optical fields on operating them with a number - conserving operator of the type , formed by the generalised superposition of products of field annihilation ( ) and creation ( ) operators , with . such an operator is experimentally realizable and can be ...
1312.6226	c	in this paper , we have used a generalised superposition of products of annihilation and creation operators to obtain nonclassical continuous variable field states . we have applied the gsp operator along with linear optical interaction on single- and two - mode cv states such as coherent , thermal and squeezed states ...	this shows that nonclassical optical states generated using the above operations on classical coherent and thermal state inputs are not resourceful for cv teleportation . this investigation could prove useful in efficient implementation of noisy non - gaussian channels , formed by linear operations , in future teleport...	we investigate the states generated in continuous variable ( cv ) optical fields on operating them with a number - conserving operator of the type , formed by the generalised superposition of products of field annihilation ( ) and creation ( ) operators , with . such an operator is experimentally realizable and can be ...
astro-ph0702383	i	this study has been motivated by the apparent lack of a non - wkb analysis of alfvn waves in a multi - fluid solar wind with differentially flowing ions . to be more specific , this study is concerned with the propagation of dissipationless , hydromagnetic ( angular frequency @xmath10 well below ion gyro - frequencies ...	the propagation of dissipationless , hydromagnetic , purely toroidal alfvn waves in a realistic background three - fluid solar wind with axial symmetry and differential proton - alpha flow is investigated . the short wavelength wkb approximation is not invoked . instead , the equations that govern the wave transport ar...	the propagation of dissipationless , hydromagnetic , purely toroidal alfvn waves in a realistic background three - fluid solar wind with axial symmetry and differential proton - alpha flow is investigated . the short wavelength wkb approximation is not invoked . instead , the equations that govern the wave transport ar...
1602.02815	i	we consider the random vandermonde matrix @xmath2 , whose @xmath3-th entry is @xmath4 , where @xmath5 are independent with haar measure distribution on the unit circle . these have been studied in @xcite , @xcite , @xcite and @xcite and are of interest for applications in finance , signal array processing , wireless ...	appropriately normalized square random vandermonde matrices based on independent random variables with uniform distribution on the unit circle are studied . it is shown that as the matrix sizes increases without bound , with respect to the expectation of the trace there is an asymptotic-distribution , equal to that of ...	appropriately normalized square random vandermonde matrices based on independent random variables with uniform distribution on the unit circle are studied . it is shown that as the matrix sizes increases without bound , with respect to the expectation of the trace there is an asymptotic-distribution , equal to that of ...
math0411648	i	let @xmath0 be a complete riemannian manifold with infinite measure . the riesz transform @xmath15 on @xmath0 is the operator @xmath16 where @xmath17 is the positive laplace operator on @xmath0 . the riesz transform is always a bounded map from @xmath18 to @xmath19 . it is of interest to figure out the range of @xmath2...	let be a smooth riemannian manifold which is the union of a compact part and a finite number of euclidean ends , for some , each of which carries the standard metric . our main result is that the riesz transform on is bounded from for and unbounded for if there is more than one end . it follows from known results that ...	let be a smooth riemannian manifold which is the union of a compact part and a finite number of euclidean ends , for some , each of which carries the standard metric . our main result is that the riesz transform on is bounded from for and unbounded for if there is more than one end . it follows from known results that ...
cond-mat0210148	i	in many materials , the symmetry of the superconducting order parameter is unconventional , i.e. not @xmath8-wave . in the high-@xmath10 cuprates , it is the singlet @xmath11-wave @xcite . there is experimental evidence that , in the quasi - one - dimensional ( q1d ) organic superconductors @xmath12 @xcite , the symme...	for certain orientations of josephson junctions between two-wave or two-wave superconductors , the subgap andreev bound states produce a-periodic relation between the josephson current and the phase difference : . consequently , the ac josephson current has the fractional frequency , where is the dc voltage . in the tu...	for certain orientations of josephson junctions between two-wave or two-wave superconductors , the subgap andreev bound states produce a-periodic relation between the josephson current and the phase difference : . consequently , the ac josephson current has the fractional frequency , where is the dc voltage . in the tu...
1007.2014	i	cold atomic systems have provided an ideal playground for the experimental studies of the unitary evolution of thermally isolated quantum systems . @xcite apart from the experimental interest , studies of quantum evolution have shed light on some fundamental questions such as thermalization . @xcite a widely - studi...	we find that the area law survives at all times . adding disorder to the toric code couplings we argue that breaking the integrability with a small magnetic field could change the area law to a volume scaling as expected of thermalized states but is not sufficient for forming topological entanglement due to the presenc...	we study quantum quenches in the two - dimensional kitaev toric code model and compute exactly the time - dependent entanglement entropy of the non - equilibrium wave - function evolving from a paramagnetic initial state with the toric code hamiltonian . we find that the area law survives at all times . adding disorder...
astro-ph9907342	i	the presence of dust in galaxies has a profound impact on observable characteristics such as their apparent uv / optical / near - ir luminosity , their spectral energy distribution , their recognizable level of star - formation activity , and their morphology . in addition , dust directly affects and often controls the...	extinction and scattering properties for two types of interstellar dust , similar to those found in the average diffuse medium of the milky way galaxy ( mw ) and the bar of the small magellanic cloud ( smc ) , are considered . the examination of the models concentrates on the study of uv / visual / near - ir reddening ...	we present and discuss the results of new multiple - scattering radiative transfer calculations for three representative types of galactic environments , filled with either homogeneous or two - phase clumpy dust distributions . extinction and scattering properties for two types of interstellar dust , similar to those f...
astro-ph9907342	c	in this section we discuss which of our models with respect to geometry , optical depth , and dust type might best be used for the analysis of observations of different kinds of galaxies . in particular , we concentrate on dust attenuation studies of nearby starburst galaxies and lyman break galaxies . + + starbur...	embedded dust , especially when clumpy , leads to saturation at fairly low reddening values with correspondingly gray attenuation functions . the average far - uv attenuation factor for the calzetti sample is found to be 7.4 . the only relatively reliable measure for the uv attenuation factor for single galaxies was fo...	we present and discuss the results of new multiple - scattering radiative transfer calculations for three representative types of galactic environments , filled with either homogeneous or two - phase clumpy dust distributions . extinction and scattering properties for two types of interstellar dust , similar to those f...
astro-ph9907342	i	we have presented new multiple - scattering radiative transfer calculations for three representative types of galactic environments and two dust types , as found within the local group in the form of the average mw and smc type dust . both homogeneous and two - phase clumpy dust distributions have been explored over a ...	we present and discuss the results of new multiple - scattering radiative transfer calculations for three representative types of galactic environments , filled with either homogeneous or two - phase clumpy dust distributions . the wavelength coverage extends from 1000 to 30,000 , with particular emphasis on the res...	we present and discuss the results of new multiple - scattering radiative transfer calculations for three representative types of galactic environments , filled with either homogeneous or two - phase clumpy dust distributions . extinction and scattering properties for two types of interstellar dust , similar to those f...
0804.4520	c	as mentioned in @xmath68 , per ob1 is unusual in that it is not associated with a giant molecular cloud . based on the results described in @xmath69 , we now find that per ob1 is unusual in at least two other respects . first , most of its members exhibit a bulk motion away from the galactic plane with those at large...	we show from _ hipparcos _ data that the luminous members of this association exhibits a bulk motion away from the galactic plane , such that their average velocity increases with height above the galactic plane . the star - forming regions located at even larger heights above the galactic plane presumably correspond t...	the per ob1 association , which contains the remarkable double cluster and per , is unusual in not having a giant molecular cloud in its vicinity . we show from _ hipparcos _ data that the luminous members of this association exhibits a bulk motion away from the galactic plane , such that their average velocity incre...
0804.4520	i	the per ob1 association comprises the remarkable @xmath0 and @xmath1 per double cluster ( among the brightest and densest open clusters known ) , surrounded by luminous o / b and both early- and late - type supergiant stars . unlike virtually all other known ob associations in the galaxy , there is no known giant mol...	the per ob1 association , which contains the remarkable double cluster and per , is unusual in not having a giant molecular cloud in its vicinity . we argue that the observed motion of the luminous member stars is most naturally explained if many formed from molecular gas pushed and accelerated outwards by an expandi...	the per ob1 association , which contains the remarkable double cluster and per , is unusual in not having a giant molecular cloud in its vicinity . we show from _ hipparcos _ data that the luminous members of this association exhibits a bulk motion away from the galactic plane , such that their average velocity incre...
1008.2957	i	the epoch of reionization in hydrogen has become a topic of considerable interest ( barkana & loeb 2001 ; fan , carilli , & keating 2006 ; meiksin 2009 ; furlanetto et al . 2009 ) as a probe of the transition from neutral to ionized hydrogen in the intergalactic medium ( igm ) . this transition occurred somewhere betw...	we report ultraviolet spectra of the high - redshift ( ) quasar , he 2347 , taken by the cosmic origins spectrograph ( cos ) on the _ hubble space telescope _ ( _ hst _ ) . spectra in the g130 m ( medium - resolution , 11351440 ) and g140l ( low - resolution , 10302000 ) gratings exhibit patchy gunn - peterson abs...	we report ultraviolet spectra of the high - redshift ( ) quasar , he 2347 , taken by the cosmic origins spectrograph ( cos ) on the _ hubble space telescope _ ( _ hst _ ) . spectra in the g130 m ( medium - resolution , 11351440 ) and g140l ( low - resolution , 10302000 ) gratings exhibit patchy gunn - peterson abs...
1008.2957	r	the systemic redshift of he 2347@xmath14342 is of interest , both to fix the expected location of the edge and to infer the metagalactic radiation field from the qso proximity effect ( dallaglio , wisotzki , & worseck 2008a , b ) . a significant puzzle for this sight line is the 6 offset between the extent of stro...	the / optical - depth ratio varies ( 10100 for , and 5500 for ) on scales ( 10.8 mpc in comoving radial distance at ) , with numerous flux - transmission windows between 11351186 . the absorption extends to 1186.26 ( ) , including associated absorbers with and minimal proximity effect " of flux transmission a...	we report ultraviolet spectra of the high - redshift ( ) quasar , he 2347 , taken by the cosmic origins spectrograph ( cos ) on the _ hubble space telescope _ ( _ hst _ ) . spectra in the g130 m ( medium - resolution , 11351440 ) and g140l ( low - resolution , 10302000 ) gratings exhibit patchy gunn - peterson abs...
1504.08273	i	dwarf spheroidals ( dsphs ) are very faint galaxies ( some of the recently discovered dsph satellites of milky way are the faintest known galaxies , @xcite ) which tend to cluster around large galaxies @xcite . among the 50 or so local group dsphs discovered so far , only two ( tucana and cetus ) are relatively isolate...	using a flexible galactic model with variable stellar velocity anisotropy , i apply the classical jeans mass modeling approach to the five dwarf spheroidal galaxies with the largest homogeneous datasets of stellar line - of - sight velocities ( between 330 and 2500 stars per galaxy ) carina , fornax , leo i , sculpto...	using a flexible galactic model with variable stellar velocity anisotropy , i apply the classical jeans mass modeling approach to the five dwarf spheroidal galaxies with the largest homogeneous datasets of stellar line - of - sight velocities ( between 330 and 2500 stars per galaxy ) carina , fornax , leo i , sculpto...
1504.08273	c	i carried out the classical jeans mass modeling of the five dwarf spheroidal galaxies with the highest quality observational data carina , fornax , leo i , sculptor , and sextans . my primary goal was to push the analysis to its limits , by developing a flexible enough galactic model ( with variable stellar velocity ...	i carry out an exhaustive model parameter search , assigning absolute probabilities to each parameter combination . my main finding is that there is a well defined radius ( unique for each galaxy ) where the jeans analysis constraints on the enclosed mass are tightest , and are much better than the constraints at previ...	using a flexible galactic model with variable stellar velocity anisotropy , i apply the classical jeans mass modeling approach to the five dwarf spheroidal galaxies with the largest homogeneous datasets of stellar line - of - sight velocities ( between 330 and 2500 stars per galaxy ) carina , fornax , leo i , sculpto...
1212.1306	c	we have performed global 3d mhd simulations of turbulent accretion disks which start from fully equilibrium mhd initial conditions . the local linear theory of the mri is used as a predictor of the growth of magnetic field perturbations in the global simulations . additional tests have also been performed to compare re...	global three dimensional magnetohydrodynamic ( mhd ) simulations of turbulent accretion disks are presented which start from fully equilibrium initial conditions in which the magnetic forces are accounted for and the induction equation is satisfied . the local linear theory of the magnetorotational instability ( mri ) ...	global three dimensional magnetohydrodynamic ( mhd ) simulations of turbulent accretion disks are presented which start from fully equilibrium initial conditions in which the magnetic forces are accounted for and the induction equation is satisfied . the local linear theory of the magnetorotational instability ( mri ) ...
nucl-th0307035	i	in this work we have calculated the in - medium @xmath298 cross section within the opem taking into account the exchange pion collectivity , vertex corrections by the contact nuclear interactions and the effective masses of the nucleon and @xmath8 resonance . \(i ) we have observed that even without the effective mass ...	we present calculations of the cross section in nuclear matter within the one - pion exchange model taking into account pion collectivity , vertex renormalization by the contact nuclear interactions and dirac effective masses of the baryons due to coupling with the scalar field . introducing the dirac effective masses ...	we present calculations of the cross section in nuclear matter within the one - pion exchange model taking into account pion collectivity , vertex renormalization by the contact nuclear interactions and dirac effective masses of the baryons due to coupling with the scalar field . introducing the dirac effective masses ...
gr-qc0510111	i	there is growing concern in the numerical relativity community about the accuracy that can be achieved as robust implementations of the einstein equations become available . as has been discussed a number of times , the simulation of strongly gravitating astrophysical systems in 3d requires the stable and accurate hand...	efforts to achieve better accuracy in numerical relativity have so far focused either on implementing second order accurate adaptive mesh refinement or on defining higher order accurate differences and update schemes . here , we argue for the combination , that is a higher order accurate adaptive scheme . this combines...	efforts to achieve better accuracy in numerical relativity have so far focused either on implementing second order accurate adaptive mesh refinement or on defining higher order accurate differences and update schemes . here , we argue for the combination , that is a higher order accurate adaptive scheme . this combines...
1407.6695	i	a primary activity of the lhc program is the exploration of the properties of the higgs boson , which was discovered over two years ago by the atlas and cms collaborations @xcite . currently , only couplings to gauge bosons and third - generation fermions are measured directly @xcite . the couplings that are fixed th...	we improve the theoretical predictions for the decays of the higgs boson to an-wave vector quarkonium plus a photon by calculating the relativistic correction of order , where is the heavy - quark velocity in the quarkonium rest frame . these refinements reduce the theoretical uncertainties in the direct - production a...	we improve the theoretical predictions for the decays of the higgs boson to an-wave vector quarkonium plus a photon by calculating the relativistic correction of order , where is the heavy - quark velocity in the quarkonium rest frame . our numerical results are given for the and channels , with . the numerical results...
0805.3646	i	the muon - spin rotation ( @xmath0sr ) technique is one of the most powerful and unique tool to study the internal magnetic field distribution @xmath7 associated with the vortex lattice in type - ii superconductors ( see , e.g. refs . ) . in the vortex state for an applied magnetic field @xmath8 , or @xmath9 ( @xmath5 ...	a detailed analysis of muon - spin rotation (sr ) spectra in the vortex state of type - ii superconductors using different theoretical models is presented . analytical approximations of the london and ginzburg - landau ( gl ) models , as well as an exact solution of the gl model were used . the limits of the validity o...	a detailed analysis of muon - spin rotation (sr ) spectra in the vortex state of type - ii superconductors using different theoretical models is presented . analytical approximations of the london and ginzburg - landau ( gl ) models , as well as an exact solution of the gl model were used . the limits of the validity o...
0707.4182	i	observational cosmology has recently witnessed a tremendous increase in proficiency in the identification of galaxies at the earliest cosmic epochs . thanks in large part to the availability of large - format mosaic ccds well - suited for wide - field imaging and spectroscopic multiplexing , we are now transitioning fr...	we present a catalog of 59 -emitting galaxies spectroscopically confirmed in a campaign of keck / deimos follow - up observations to candidates selected in the large area lyman alpha ( lala ) narrow - band imaging survey . we targeted 97 candidates for spectroscopic follow - up ; by accounting for the variety of condit...	we present a catalog of 59 -emitting galaxies spectroscopically confirmed in a campaign of keck / deimos follow - up observations to candidates selected in the large area lyman alpha ( lala ) narrow - band imaging survey . we targeted 97 candidates for spectroscopic follow - up ; by accounting for the variety of condit...
0707.4182	c	together with the observations presented in paper i ( and accounting for minor overlap in the samples ) , the 59 -emitters confirmed herein bring the total catalog of spectroscopically confirmed @xmath0 -emitting galaxies to 73 objects in the @xmath3 degrees@xmath4 surveyed by the lala imaging . we now update the chara...	the 59 sources confirmed herein bring the total catalog to 73 spectroscopically confirmed -emitting galaxies in the degrees covered by the lala imaging . we find no significant evidence for luminosity function evolution from to . this result supports the conclusion that the intergalactic medium remains largely reioniz...	we present a catalog of 59 -emitting galaxies spectroscopically confirmed in a campaign of keck / deimos follow - up observations to candidates selected in the large area lyman alpha ( lala ) narrow - band imaging survey . we targeted 97 candidates for spectroscopic follow - up ; by accounting for the variety of condit...
0910.4279	c	the herschel atlas is the largest open - time key project that will be carried out with the herschel space observatory . it will survey 510 square degrees of the extragalactic sky , four times larger than all the other herschel surveys combined , in five far - infrared and submillimetre bands . we have described the su...	the herschel atlas is the largest open - time key project that will be carried out on the herschel space observatory . it will survey 510 square degrees of the extragalactic sky , four times larger than all the other herschel surveys combined , in five far - infrared and submillimetre bands . we describe the survey , t...	the herschel atlas is the largest open - time key project that will be carried out on the herschel space observatory . it will survey 510 square degrees of the extragalactic sky , four times larger than all the other herschel surveys combined , in five far - infrared and submillimetre bands . we describe the survey , t...
hep-ph0605285	i	we have studied in detail the possibility to describe the neutrino masses and mixing angles in the context of split supersymmetric scenarios where the sfermions and/or higgses are very heavy . we have considered all relevant contributions to the neutrino mass matrix up to one - loop level coming from the r - parity vio...	we investigate the possibility to generate neutrino masses in the context of split supersymmetric scenarios where all sfermions are very heavy . all relevant contributions coming from the r - parity violating terms to the neutrino mass matrix up to one - loop level are computed , showing the importance of the higgs one...	we investigate the possibility to generate neutrino masses in the context of split supersymmetric scenarios where all sfermions are very heavy . all relevant contributions coming from the r - parity violating terms to the neutrino mass matrix up to one - loop level are computed , showing the importance of the higgs one...
1410.5912	i	it is important to investigate the relationships between the power sources of galaxies ( i.e. , active galactic nuclei ( agn ) and/or starbursts ) and the chemical properties of the surrounding dense interstellar medium in order to study the effects on molecular abundances and to probe the power source with molecular l...	we present 0.8-mm band molecular images and spectra obtained with the atacama large millimeter / submillimeter array ( alma ) toward one of the nearest galaxies with an active galactic nucleus ( agn ) , ngc 1068 . we find that the abundances of shock - related molecules are more similar to abundances in hot cores and/o...	we present 0.8-mm band molecular images and spectra obtained with the atacama large millimeter / submillimeter array ( alma ) toward one of the nearest galaxies with an active galactic nucleus ( agn ) , ngc 1068 . distributions of co isotopic species (co and co ) = 32 , cn = 32 and cs = 76 are observed toward the circu...
1410.5912	c	we observed the seyfert 2 galaxy ngc 1068 with the 0.8-mm band in the cnd and starburst ring during the alma early science program . the analyses were carried out with our data obtained at 3-mm band ( paper-1 ) . the main results of this work are summarized in the following list . we successfully observed images of @xm...	distributions of co isotopic species (co and co ) = 32 , cn = 32 and cs = 76 are observed toward the circumnuclear disk ( cnd ) and a part of the starburst ring with an angular resolution of. 1. . the physical properties of these molecules and shock - related molecules such as hnco , chcn , so , and choh detected in th...	we present 0.8-mm band molecular images and spectra obtained with the atacama large millimeter / submillimeter array ( alma ) toward one of the nearest galaxies with an active galactic nucleus ( agn ) , ngc 1068 . distributions of co isotopic species (co and co ) = 32 , cn = 32 and cs = 76 are observed toward the circu...
1210.5409	i	the universal features of a large class of one - dimensional quantum models , exhibiting gapless excitations with linear spectrum , are successfully described @xcite by the tomonaga - luttinger ( tl ) liquid theory @xcite-@xcite . this theory applies to various systems , including nanowire junctions and carbon nanotube...	the boundary condition at the junction is fixed by an orthogonal matrix , which describes the splitting of the electric current among the leads . we develop a non - equilibrium bosonization procedure and compute some basic correlation functions . luttinger liquids with general anyon statistics are considered . both the...	we propose and investigate an exactly solvable model of non - equilibrium luttinger liquid on a star graph , modeling a multi - terminal quantum wire junction . the boundary condition at the junction is fixed by an orthogonal matrix , which describes the splitting of the electric current among the leads . the system is...
1210.5409	c	in this paper we constructed and investigated an exactly solvable model of a non - equilibrium luttinger junction . the basic points of our approach are : ( i ) : : a scale invariant point - like interaction , which is described by a scattering matrix @xmath0 and drives the system away from equilibrium ; ( ...	we propose and investigate an exactly solvable model of non - equilibrium luttinger liquid on a star graph , modeling a multi - terminal quantum wire junction . the system is driven away from equilibrium by connecting the leads to heat baths at different temperatures and chemical potentials . the associated non - equil...	we propose and investigate an exactly solvable model of non - equilibrium luttinger liquid on a star graph , modeling a multi - terminal quantum wire junction . the boundary condition at the junction is fixed by an orthogonal matrix , which describes the splitting of the electric current among the leads . the system is...
astro-ph0202175	i	the value of equipping telescopes with a large field of view has been recognised for some time . in 1986 the royal astronomical society report `` review of scientific priorities for uk astronomical research 19902000 '' @xcite put a wide - field multi - object spectroscopic facility at the top of its priority list for n...	the 2df ( two - degree field ) facility at the prime focus of the anglo - australian telescope provides multiple object spectroscopy over a field of view . the 2df facility began routine observations in 1997 . 2df has achieved its initial astronomical goals . we also briefly review its scientific applications and po...	the 2df ( two - degree field ) facility at the prime focus of the anglo - australian telescope provides multiple object spectroscopy over a field of view . up to 400 target fibres can be independently positioned by a complex robot . two spectrographs provide spectra with resolutions of between 500 and 2000 , over wavel...
1506.02540	i	the mathematical theory for the spread of infectious diseases has a long history and is by now quite rich ( e.g. , @xcite ) . one of the more common type of disease models is called sir ( susceptible @xmath1 infective @xmath1 recovered ) meaning that individuals are at first susceptible . if infected ( by someone ) th...	consider a large uniformly mixing dynamic population , which has constant birth rate and exponentially distributed lifetimes , with mean population size . a markovian sir ( susceptible infective recovered ) infectious disease , having importation of infectives , taking place in this population is analysed . the main si...	consider a large uniformly mixing dynamic population , which has constant birth rate and exponentially distributed lifetimes , with mean population size . a markovian sir ( susceptible infective recovered ) infectious disease , having importation of infectives , taking place in this population is analysed . the main si...
hep-ph9211304	i	effective low energy hamiltonians for non leptonic weak decays of hadrons are usually written as linear combinations of four quark operators . the coefficients of these operators , the wilson coefficient functions , can be calculated in the renormalization group improved perturbation theory , as long as the normaliza...	we calculate the two the calculation is performed in two schemes for : the dimensional regularization scheme with anticommuting ( ndr ) , and in the t hooft veltman scheme . we demonstrate how a direct calculation of diagrams involving in closed fermion loops can be avoided thus allowing a consistent calculation in t...	we calculate the two loop anomalous dimension matrix involving current current operators , qcd penguin operators , and electroweak penguin operators especially relevant for weak non leptonic decays , but also important for decays . the calculation is performed in two schemes for : the dimensional regularization sche...
hep-ph9211304	i	we have presented the details and the explicit results of the calculation of the two loop anomalous dimension matrix @xmath284 involving current - current , qcd - penguin and electroweak - penguin operators . performing the calculation in two schemes for @xmath5 , ndr and hv , we have verified the compatibility of the...	loop anomalous dimension matrix involving current current operators , qcd penguin operators , and electroweak penguin operators especially relevant for weak non leptonic decays , but also important for decays . the two loop anomalous dimension matrix , required for a consistent inclusion of electroweak penguin opera...	we calculate the two loop anomalous dimension matrix involving current current operators , qcd penguin operators , and electroweak penguin operators especially relevant for weak non leptonic decays , but also important for decays . the calculation is performed in two schemes for : the dimensional regularization sche...
1010.4504	i	the covariance graph ( aka bi - directed graph ) of a probability distribution @xmath0 is the undirected graph @xmath1 where two nodes are adjacent iff their corresponding random variables are marginally dependent in @xmath0 . covariance graphs were introduced in @xcite to represent independence models . since then , t...	the covariance graph ( aka bi - directed graph ) of a probability distribution is the undirected graph where two nodes are adjacent iff their corresponding random variables are marginally dependent in . implies that their corresponding random variables are marginally independent in . this difference in the definition i...	the covariance graph ( aka bi - directed graph ) of a probability distribution is the undirected graph where two nodes are adjacent iff their corresponding random variables are marginally dependent in . implies that their corresponding random variables are marginally independent in . this difference in the definition i...
0905.0020	i	after many years of preparation , interferometric gravitational wave ( gw ) detectors have now begun an era of long - duration observing . the three detectors of the laser interferometer gravitational - wave observatory ( ligo ) @xcite reached their design sensitivity levels in 2005 and began a `` science run '' that ...	we present the results obtained from an all - sky search for gravitational - wave ( gw ) bursts in the 642000hz frequency range in data collected by the ligo detectors during the first year ( november 2005 november 2006 ) of their fifth science run.the total analyzed livetime was 268.6 days . multiple hierarchical dat...	we present the results obtained from an all - sky search for gravitational - wave ( gw ) bursts in the 642000hz frequency range in data collected by the ligo detectors during the first year ( november 2005 november 2006 ) of their fifth science run.the total analyzed livetime was 268.6 days . multiple hierarchical dat...
cond-mat0505420	i	interactions between localized defects which are mediated by the continuum they are embedded in , play an important role in many areas of physics . typical examples are the rkky interaction between spins in a fermi liquid or the interaction between vortices in superfluids . in the present work , we discuss interactions...	the friedel oscillations of the interacting system are replaced , at long distances , by a universal casimir - type interaction which depends only on the sound velocity and decays inversely with the separation . the casimir - type interaction between localized perturbations embedded in a fermionic environment gives ris...	we discuss the effective interactions between two localized perturbations in one - dimensional ( 1d ) quantum liquids . for non - interacting fermions , the interactions exhibit friedel oscillations , giving rise to a rkky - type interaction familiar from impurity spins in metals . in the interacting case , at low ener...
astro-ph0309292	i	the spin down luminosity of a rotating pulsar powers the emission of an associated synchrotron nebula by driving an initially poynting flux - dominated wind ( the poynting - to - matter energy flux ratio is @xmath4 ) that flows along the open magnetic field lines . the density of the outflowing matter is enhanced by pa...	using relativistic , steady , axisymmetric , ideal magnetohydrodynamics ( mhd ) we analyze the super - alfvnic regime of a pulsar wind by means of solving the momentum equation along the flow as well as in the transfield direction . employing a self - similar model , we demonstrate that ideal mhd can account for the fu...	using relativistic , steady , axisymmetric , ideal magnetohydrodynamics ( mhd ) we analyze the super - alfvnic regime of a pulsar wind by means of solving the momentum equation along the flow as well as in the transfield direction . employing a self - similar model , we demonstrate that ideal mhd can account for the fu...
1402.4813	i	how do coefficients of a wave - function change at continuous quantum phase transitions ? in a given basis , this question can be addressed by monitoring the behavior of ( inverse ) participation ratios , which have a long history _ e.g. _ in localization physics @xcite . more recently , the study of related quantities...	universal features in the scalings of shannon - rnyi entropies of many - body groundstates are studied for interacting spin- systems across ( 2 + 1 ) dimensional critical points , using quantum monte carlo simulations on dimerized and plaquettized heisenberg models on the square lattice . considering both full systems ...	universal features in the scalings of shannon - rnyi entropies of many - body groundstates are studied for interacting spin- systems across ( 2 + 1 ) dimensional critical points , using quantum monte carlo simulations on dimerized and plaquettized heisenberg models on the square lattice . considering both full systems ...