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708.3549
Lopsidedness and Sloshing in Centres of Advanced Mergers of Galaxies
We measure the non-axisymmetry in the luminosity distribution in the central few kpc of a sample of advanced mergers of galaxies, by analyzing their 2MASS images. All mergers show a high central asymmetry: the centres of isophotes show a striking sloshing pattern with a spatial variation of upto 30 % within the central 1 kpc; and the Fourier amplitude for lopsidedness (m=1) shows high values upto 0.2 within the central 5 kpc. The central asymmetry is estimated to be long-lived, lasting for ~ a few Gyr or ~ 100 local dynamical timescales. This will significantly affect the dynamical evolution of this region, by helping fuel the central active galactic nucleus, and also by causing the secular growth of the bulge driven by lopsidedness.
astro-ph
we measure the nonaxisymmetry in the luminosity distribution in the central few kpc of a sample of advanced mergers of galaxies by analyzing their 2mass images all mergers show a high central asymmetry the centres of isophotes show a striking sloshing pattern with a spatial variation of upto 30 within the central 1 kpc and the fourier amplitude for lopsidedness m1 shows high values upto 02 within the central 5 kpc the central asymmetry is estimated to be longlived lasting for a few gyr or 100 local dynamical timescales this will significantly affect the dynamical evolution of this region by helping fuel the central active galactic nucleus and also by causing the secular growth of the bulge driven by lopsidedness
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708.355
Is there a new physics between electroweak and Planck scales?
We argue that there may be no intermediate particle physics energy scale between the Planck mass $M_{Pl}\sim 10^{19}$ GeV and the electroweak scale $M_W \sim 100$ GeV. At the same time, the number of problems of the Standard Model (neutrino masses and oscillations, dark matter, baryon asymmetry of the Universe, strong CP-problem, gauge coupling unification, inflation) could find their solution at $M_{Pl}$ or $M_W$. The crucial experimental predictions of this point of view are outlined.
hep-th hep-ph
we argue that there may be no intermediate particle physics energy scale between the planck mass m_plsim 1019 gev and the electroweak scale m_w sim 100 gev at the same time the number of problems of the standard model neutrino masses and oscillations dark matter baryon asymmetry of the universe strong cpproblem gauge coupling unification inflation could find their solution at m_pl or m_w the crucial experimental predictions of this point of view are outlined
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708.3551
Theoretical analysis of the optimal conditions for photon-spin quantum state transfer
We analyzed the yield and fidelity of the quantum state transfer (QST) from a photon polarization qubit to an electron spin qubit in a spin-coherent photo detector consisting of a semiconductor quantum dot. We used a model consisting of the quantum dot, where the QST is carried out, coupled with a photonic cavity. We determined the optimal conditions that allow the realization of both high-yield and high-fidelity QST.
cond-mat.other cond-mat.mes-hall
we analyzed the yield and fidelity of the quantum state transfer qst from a photon polarization qubit to an electron spin qubit in a spincoherent photo detector consisting of a semiconductor quantum dot we used a model consisting of the quantum dot where the qst is carried out coupled with a photonic cavity we determined the optimal conditions that allow the realization of both highyield and highfidelity qst
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708.3552
An order result for the exponential divisor function
The integer $d=\prod_{i=1}^s p_i^{b_i}$ is called an exponential divisor of $n=\prod_{i=1}^s p_i^{a_i}>1$ if $b_i \mid a_i$ for every $i\in \{1,2,...,s\}$. Let $\tau^{(e)}(n)$ denote the number of exponential divisors of $n$, where $\tau^{(e)}(1)=1$ by convention. The aim of the present paper is to establish an asymptotic formula with remainder term for the $r$-th power of the function $\tau^{(e)}$, where $r\ge 1$ is an integer. This improves an earlier result of {\sc M. V. Subbarao} [5].
math.NT
the integer dprod_i1s p_ib_i is called an exponential divisor of nprod_i1s p_ia_i1 if b_i mid a_i for every iin 12s let tauen denote the number of exponential divisors of n where taue11 by convention the aim of the present paper is to establish an asymptotic formula with remainder term for the rth power of the function taue where rge 1 is an integer this improves an earlier result of sc m v subbarao 5
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708.3553
A study of the prompt and afterglow emission of the Short GRB 061201
Our knowledge of the intrinsic properties of short duration Gamma-Ray Bursts has relied, so far, only upon a few cases for which the estimate of the distance and an extended, multiwavelength monitoring of the afterglow have been obtained. We carried out multiwavelength observations of the short GRB 061201 aimed at estimating its distance and studying its properties. We performed a spectral and timing analysis of the prompt and afterglow emission and discuss the results in the context of the standard fireball model. A clear temporal break was observed in the X-ray light curve about 40 minutes after the burst trigger. We find that the spectral and timing behaviour of the X-ray afterglow is consistent with a jet origin of the observed break, although the optical data can not definitively confirm this and other scenarios are possible. No underlying host galaxy down to R~26 mag was found after fading of the optical afterglow. Thus, no secure redshift could be measured for this burst. The nearest galaxy is at z=0.111 and shows evidence of star formation activity. We discuss the association of GRB 061201 with this galaxy and with the ACO S 995 galaxy cluster, from which the source is at an angular distance of 17'' and 8.5', respectively. We also test the association with a possible undetected, positionally consistent galaxy at z~1. In all these cases, in the jet interpretation, we find a jet opening angle of 1-2 degrees.
astro-ph
our knowledge of the intrinsic properties of short duration gammaray bursts has relied so far only upon a few cases for which the estimate of the distance and an extended multiwavelength monitoring of the afterglow have been obtained we carried out multiwavelength observations of the short grb 061201 aimed at estimating its distance and studying its properties we performed a spectral and timing analysis of the prompt and afterglow emission and discuss the results in the context of the standard fireball model a clear temporal break was observed in the xray light curve about 40 minutes after the burst trigger we find that the spectral and timing behaviour of the xray afterglow is consistent with a jet origin of the observed break although the optical data can not definitively confirm this and other scenarios are possible no underlying host galaxy down to r26 mag was found after fading of the optical afterglow thus no secure redshift could be measured for this burst the nearest galaxy is at z0111 and shows evidence of star formation activity we discuss the association of grb 061201 with this galaxy and with the aco s 995 galaxy cluster from which the source is at an angular distance of 17 and 85 respectively we also test the association with a possible undetected positionally consistent galaxy at z1 in all these cases in the jet interpretation we find a jet opening angle of 12 degrees
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708.3554
Time-distance helioseismology: Sensitivity of f-mode travel times to flows
Time-distance helioseismology has shown that f-mode travel times contain information about horizontal flows in the Sun. The purpose of this study is to provide a simple interpretation of these travel times. We study the interaction of surface-gravity waves with horizontal flows in an incompressible, plane-parallel solar atmosphere. We show that for uniform flows less than roughly 250 m s$^{-1}$, the travel-time shifts are linear in the flow amplitude. For stronger flows, perturbation theory up to third order is needed to model waveforms. The case of small-amplitude spatially-varying flows is treated using the first-order Born approximation. We derive two-dimensional Fr\'{e}chet kernels that give the sensitivity of travel-time shifts to local flows. We show that the effect of flows on travel times depends on wave damping and on the direction from which the observations are made. The main physical effect is the advection of the waves by the flow rather than the advection of wave sources or the effect of flows on wave damping. We compare the two-dimensional sensitivity kernels with simplified three-dimensional kernels that only account for wave advection and assume a vertical line of sight. We find that the three-dimensional f-mode kernels approximately separate in the horizontal and vertical coordinates, with the horizontal variations given by the simplified two-dimensional kernels. This consistency between quite different models gives us confidence in the usefulness of these kernels for interpreting quiet-Sun observations.
astro-ph
timedistance helioseismology has shown that fmode travel times contain information about horizontal flows in the sun the purpose of this study is to provide a simple interpretation of these travel times we study the interaction of surfacegravity waves with horizontal flows in an incompressible planeparallel solar atmosphere we show that for uniform flows less than roughly 250 m s1 the traveltime shifts are linear in the flow amplitude for stronger flows perturbation theory up to third order is needed to model waveforms the case of smallamplitude spatiallyvarying flows is treated using the firstorder born approximation we derive twodimensional frechet kernels that give the sensitivity of traveltime shifts to local flows we show that the effect of flows on travel times depends on wave damping and on the direction from which the observations are made the main physical effect is the advection of the waves by the flow rather than the advection of wave sources or the effect of flows on wave damping we compare the twodimensional sensitivity kernels with simplified threedimensional kernels that only account for wave advection and assume a vertical line of sight we find that the threedimensional fmode kernels approximately separate in the horizontal and vertical coordinates with the horizontal variations given by the simplified twodimensional kernels this consistency between quite different models gives us confidence in the usefulness of these kernels for interpreting quietsun observations
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708.3555
Weakly anisotropic frustrated zigzag spin chain
The frustrated spin-1/2 model with weakly anisotropic ferromagnetic nearest-neighbor and antiferromagnetic next-nearest-neighbor exchanges is studied with use of variational mean-field approach, scaling estimates of the infrared divergencies in the perturbation theory and finite-size calculations. The ground state phase diagram of this model contains three phases: the ferromagnetic phase, the commensurate spin-liquid phase and the incommensurate phase. The non-trivial behavior of the boundaries between these phases and the character of the phase transitions in case of weak anisotropy are determined.
cond-mat.str-el
the frustrated spin12 model with weakly anisotropic ferromagnetic nearestneighbor and antiferromagnetic nextnearestneighbor exchanges is studied with use of variational meanfield approach scaling estimates of the infrared divergencies in the perturbation theory and finitesize calculations the ground state phase diagram of this model contains three phases the ferromagnetic phase the commensurate spinliquid phase and the incommensurate phase the nontrivial behavior of the boundaries between these phases and the character of the phase transitions in case of weak anisotropy are determined
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708.3556
Generalization error for multi-class margin classification
In this article, we study rates of convergence of the generalization error of multi-class margin classifiers. In particular, we develop an upper bound theory quantifying the generalization error of various large margin classifiers. The theory permits a treatment of general margin losses, convex or nonconvex, in presence or absence of a dominating class. Three main results are established. First, for any fixed margin loss, there may be a trade-off between the ideal and actual generalization performances with respect to the choice of the class of candidate decision functions, which is governed by the trade-off between the approximation and estimation errors. In fact, different margin losses lead to different ideal or actual performances in specific cases. Second, we demonstrate, in a problem of linear learning, that the convergence rate can be arbitrarily fast in the sample size $n$ depending on the joint distribution of the input/output pair. This goes beyond the anticipated rate $O(n^{-1})$. Third, we establish rates of convergence of several margin classifiers in feature selection with the number of candidate variables $p$ allowed to greatly exceed the sample size $n$ but no faster than $\exp(n)$.
math.ST stat.TH
in this article we study rates of convergence of the generalization error of multiclass margin classifiers in particular we develop an upper bound theory quantifying the generalization error of various large margin classifiers the theory permits a treatment of general margin losses convex or nonconvex in presence or absence of a dominating class three main results are established first for any fixed margin loss there may be a tradeoff between the ideal and actual generalization performances with respect to the choice of the class of candidate decision functions which is governed by the tradeoff between the approximation and estimation errors in fact different margin losses lead to different ideal or actual performances in specific cases second we demonstrate in a problem of linear learning that the convergence rate can be arbitrarily fast in the sample size n depending on the joint distribution of the inputoutput pair this goes beyond the anticipated rate on1 third we establish rates of convergence of several margin classifiers in feature selection with the number of candidate variables p allowed to greatly exceed the sample size n but no faster than expn
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708.3557
On certain arithmetic functions involving exponential divisors, II
Asymptotic properties of certain arithmetic functions involving exponential divisors are investigated.
math.NT
asymptotic properties of certain arithmetic functions involving exponential divisors are investigated
[['asymptotic', 'properties', 'of', 'certain', 'arithmetic', 'functions', 'involving', 'exponential', 'divisors', 'are', 'investigated']]
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708.3558
Teleparallel Killing Vectors of the Einstein Universe
In this short paper we establish the definition of the Lie derivative of a second rank tensor in the context of teleparallel theory of gravity and also extend it for a general tensor of rank $p+q$. This definition is then used to find Killing vectors of the Einstein universe. It turns out that Killing vectors of the Einstein universe in the teleparallel theory are the same as in General Relativity.
gr-qc
in this short paper we establish the definition of the lie derivative of a second rank tensor in the context of teleparallel theory of gravity and also extend it for a general tensor of rank pq this definition is then used to find killing vectors of the einstein universe it turns out that killing vectors of the einstein universe in the teleparallel theory are the same as in general relativity
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708.3559
Locally Indistinguishable Subspaces Spanned by Three-Qubit Unextendible Product Bases
We study the local distinguishability of general multi-qubit states and show that local projective measurements and classical communication are as powerful as the most general local measurements and classical communication. Remarkably, this indicates that the local distinguishability of multi-qubit states can be decided efficiently. Another useful consequence is that a set of orthogonal $n$-qubit states is locally distinguishable only if the summation of their orthogonal Schmidt numbers is less than the total dimension $2^n$. When $n=2$ such a condition is also sufficient. Employing these results, we show that any orthonormal basis of a subspace spanned by arbitrary three-qubit orthogonal unextendible product bases (UPB) cannot be exactly distinguishable by local operations and classical communication. This not only reveals another intrinsic property of three-qubit orthogonal UPB, but also provides a class of locally indistinguishable subspaces with dimension 4. We also explicitly construct locally indistinguishable subspaces with dimensions 3 and 5, respectively. In particular, 3 is the minimal possible dimension of locally indistinguishable subspaces. Combining with the previous results, we conclude that any positive integer between 3 and 7 is the possible dimension of some three-qubit locally indistinguishable subspace.
quant-ph
we study the local distinguishability of general multiqubit states and show that local projective measurements and classical communication are as powerful as the most general local measurements and classical communication remarkably this indicates that the local distinguishability of multiqubit states can be decided efficiently another useful consequence is that a set of orthogonal nqubit states is locally distinguishable only if the summation of their orthogonal schmidt numbers is less than the total dimension 2n when n2 such a condition is also sufficient employing these results we show that any orthonormal basis of a subspace spanned by arbitrary threequbit orthogonal unextendible product bases upb cannot be exactly distinguishable by local operations and classical communication this not only reveals another intrinsic property of threequbit orthogonal upb but also provides a class of locally indistinguishable subspaces with dimension 4 we also explicitly construct locally indistinguishable subspaces with dimensions 3 and 5 respectively in particular 3 is the minimal possible dimension of locally indistinguishable subspaces combining with the previous results we conclude that any positive integer between 3 and 7 is the possible dimension of some threequbit locally indistinguishable subspace
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708.356
Prompt photon hadroproduction at high energies in off-shell gluon-gluon fusion
The amplitude for production of a single photon associated with quark pair in the fusion of two off-shell gluons is calculated. The matrix element found is applied to the inclusive prompt photon hadroproduction at high energies in the framework of kt-factorization QCD approach. The total and differential cross sections are calculated in both central and forward pseudo-rapidity regions. The conservative error analisys is performed. We used the unintegrated gluon distributions in a proton which were obtained from the full CCFM evolution equation as well as from the Kimber-Martin-Ryskin prescription. Theoretical results were compared with recent experimental data taken by the D0 and CDF collaborations at Fermilab Tevatron. Theoretical predictions for the LHC energies are given.
hep-ph
the amplitude for production of a single photon associated with quark pair in the fusion of two offshell gluons is calculated the matrix element found is applied to the inclusive prompt photon hadroproduction at high energies in the framework of ktfactorization qcd approach the total and differential cross sections are calculated in both central and forward pseudorapidity regions the conservative error analisys is performed we used the unintegrated gluon distributions in a proton which were obtained from the full ccfm evolution equation as well as from the kimbermartinryskin prescription theoretical results were compared with recent experimental data taken by the d0 and cdf collaborations at fermilab tevatron theoretical predictions for the lhc energies are given
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708.3561
Phase transitions in a fluid surface model with a deficit angle term
Nambu-Goto model is investigated by using the canonical Monte Carlo simulation technique on dynamically triangulated surfaces of spherical topology. We find that the model has four distinct phases; crumpled, branched-polymer, linear, and tubular. The linear phase and the tubular phase appear to be separated by a first-order transition. It is also found that there is no long-range two-dimensional order in the model. In fact, no smooth surface can be seen in the whole region of the curvature modulus \alpha, which is the coefficient of the deficit angle term in the Hamiltonian. The bending energy, which is not included in the Hamiltonian, remains large even at sufficiently large \alpha in the tubular phase. On the other hand, the surface is spontaneously compactified into a one-dimensional smooth curve in the linear phase; one of the two degrees of freedom shrinks, and the other degree of freedom remains along the curve. Moreover, we find that the rotational symmetry of the model is spontaneously broken in the tubular phase just as in the same model on the fixed connectivity surfaces.
cond-mat.stat-mech cond-mat.soft
nambugoto model is investigated by using the canonical monte carlo simulation technique on dynamically triangulated surfaces of spherical topology we find that the model has four distinct phases crumpled branchedpolymer linear and tubular the linear phase and the tubular phase appear to be separated by a firstorder transition it is also found that there is no longrange twodimensional order in the model in fact no smooth surface can be seen in the whole region of the curvature modulus alpha which is the coefficient of the deficit angle term in the hamiltonian the bending energy which is not included in the hamiltonian remains large even at sufficiently large alpha in the tubular phase on the other hand the surface is spontaneously compactified into a onedimensional smooth curve in the linear phase one of the two degrees of freedom shrinks and the other degree of freedom remains along the curve moreover we find that the rotational symmetry of the model is spontaneously broken in the tubular phase just as in the same model on the fixed connectivity surfaces
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708.3562
First Passage Densities and Boundary Crossing Probabilities for Diffusion Processes
We consider the boundary crossing problem for time-homogeneous diffusions and general curvilinear boundaries. Bounds are derived for the approximation error of the one-sided (upper) boundary crossing probability when replacing the original boundary by a different one. In doing so we establish the existence of the first-passage time density and provide an upper bound for this function. In the case of processes with diffusion interval equal to whole real line this is extended to a lower bound, as well as bounds for the first crossing time of a lower boundary. An extension to some time-inhomogeneous diffusions is given. These results are illustrated by numerical examples.
math.PR
we consider the boundary crossing problem for timehomogeneous diffusions and general curvilinear boundaries bounds are derived for the approximation error of the onesided upper boundary crossing probability when replacing the original boundary by a different one in doing so we establish the existence of the firstpassage time density and provide an upper bound for this function in the case of processes with diffusion interval equal to whole real line this is extended to a lower bound as well as bounds for the first crossing time of a lower boundary an extension to some timeinhomogeneous diffusions is given these results are illustrated by numerical examples
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708.3563
Renormalization of vacuum energy in linearized quantum gravity
In linearized quantum gravity, a shift of the average energy-momentum can be compensated by a shift of the average gravitational field. This allows a renormalization scheme that naturally removes the contribution of quantum vacuum fluctuations to the cosmological constant, solving the old cosmological-constant problem for weak gravitational fields.
gr-qc hep-th
in linearized quantum gravity a shift of the average energymomentum can be compensated by a shift of the average gravitational field this allows a renormalization scheme that naturally removes the contribution of quantum vacuum fluctuations to the cosmological constant solving the old cosmologicalconstant problem for weak gravitational fields
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708.3564
Deciding security properties for cryptographic protocols. Application to key cycles
There is a large amount of work dedicated to the formal verification of security protocols. In this paper, we revisit and extend the NP-complete decision procedure for a bounded number of sessions. We use a, now standard, deducibility constraints formalism for modeling security protocols. Our first contribution is to give a simple set of constraint simplification rules, that allows to reduce any deducibility constraint system to a set of solved forms, representing all solutions (within the bound on sessions). As a consequence, we prove that deciding the existence of key cycles is NP-complete for a bounded number of sessions. The problem of key-cycles has been put forward by recent works relating computational and symbolic models. The so-called soundness of the symbolic model requires indeed that no key cycle (e.g., enc(k,k)) ever occurs in the execution of the protocol. Otherwise, stronger security assumptions (such as KDM-security) are required. We show that our decision procedure can also be applied to prove again the decidability of authentication-like properties and the decidability of a significant fragment of protocols with timestamps.
cs.LO cs.CR
there is a large amount of work dedicated to the formal verification of security protocols in this paper we revisit and extend the npcomplete decision procedure for a bounded number of sessions we use a now standard deducibility constraints formalism for modeling security protocols our first contribution is to give a simple set of constraint simplification rules that allows to reduce any deducibility constraint system to a set of solved forms representing all solutions within the bound on sessions as a consequence we prove that deciding the existence of key cycles is npcomplete for a bounded number of sessions the problem of keycycles has been put forward by recent works relating computational and symbolic models the socalled soundness of the symbolic model requires indeed that no key cycle eg enckk ever occurs in the execution of the protocol otherwise stronger security assumptions such as kdmsecurity are required we show that our decision procedure can also be applied to prove again the decidability of authenticationlike properties and the decidability of a significant fragment of protocols with timestamps
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708.3565
The double-mode RR Lyrae variable BS Com
We present the frequency analysis of the multicolour time series photometry of the field RRd variable BS Comae. The large number of data points in each of the BV(RI)_c bands and the ~0.01 magnitude accuracy of the individual measurements allow us a high precision analysis of the properties of the combination frequencies due to nonlinear coupling. Through the combination of the frequency spectra in different colors we show that except for the components corresponding to the linear combinations of the two pulsation modes, there are no other components present above the millimagnitude amplitude level.
astro-ph
we present the frequency analysis of the multicolour time series photometry of the field rrd variable bs comae the large number of data points in each of the bvri_c bands and the 001 magnitude accuracy of the individual measurements allow us a high precision analysis of the properties of the combination frequencies due to nonlinear coupling through the combination of the frequency spectra in different colors we show that except for the components corresponding to the linear combinations of the two pulsation modes there are no other components present above the millimagnitude amplitude level
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708.3566
Does Sub-millisecond Pulsar XTE J1739-285 Contain a Low Magnetic Neutron Star or Quark Star ?
With the possible detection of the fastest spinning nuclear-powered pulsar XTE J1739-285 of frequency 1122 Hz (0.8913 ms), it arouses us to constrain the mass and radius of its central compact object and to imply the stellar matter compositions: neutrons or quarks. Spun-up by the accreting materials to such a high rotating speed, the compact star should have either a small radius or short innermost stable circular orbit. By the empirical relation between the upper kHz quasi-periodic oscillation frequency and star spin frequency, a strong constraint on mass and radius is obtained as 1.51 solar masses and 10.9 km, which excludes most equations of states (EOSs) of normal neutrons and strongly hints the star promisingly to be a strange quark star. Furthermore, the star magnetic field is estimated to be about $4\times10^{7} (G) < B < 10^{9} (G) $, which reconciles with those of millisecond radio pulsars, revealing the clues of the evolution linkage of two types of astrophysical objects.
astro-ph
with the possible detection of the fastest spinning nuclearpowered pulsar xte j1739285 of frequency 1122 hz 08913 ms it arouses us to constrain the mass and radius of its central compact object and to imply the stellar matter compositions neutrons or quarks spunup by the accreting materials to such a high rotating speed the compact star should have either a small radius or short innermost stable circular orbit by the empirical relation between the upper khz quasiperiodic oscillation frequency and star spin frequency a strong constraint on mass and radius is obtained as 151 solar masses and 109 km which excludes most equations of states eoss of normal neutrons and strongly hints the star promisingly to be a strange quark star furthermore the star magnetic field is estimated to be about 4times107 g b 109 g which reconciles with those of millisecond radio pulsars revealing the clues of the evolution linkage of two types of astrophysical objects
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708.3567
On the Distortion of the Eigenvalue Spectrum in MIMO Amplify-and-Forward Multi-Hop Channels
Consider a wireless MIMO multi-hop channel with n_s non-cooperating source antennas and n_d fully cooperating destination antennas, as well as L clusters containing k non-cooperating relay antennas each. The source signal traverses all L clusters of relay antennas, before it reaches the destination. When relay antennas within the same cluster scale their received signals by the same constant before the retransmission, the equivalent channel matrix H relating the input signals at the source antennas to the output signals at the destination antennas is proportional to the product of channel matrices H_l, l=1,...,L+1, corresponding to the individual hops. We perform an asymptotic capacity analysis for this channel as follows: In a first instance we take the limits n_s->infty, n_d->infty and k->infty, but keep both n_s/n_d and k/n_d fixed. Then, we take the limits L->infty and k/n_d->infty. Requiring that the H_l's satisfy the conditions needed for the Marcenko-Pastur law, we prove that the capacity scales linearly in min{n_s,n_d}, as long as the ratio k/n_d scales at least linearly in L. Moreover, we show that up to a noise penalty and a pre-log factor the capacity of a point-to-point MIMO channel is approached, when this scaling is slightly faster than linear. Conversely, almost all spatial degrees of freedom vanish for less than linear scaling.
cs.IT math.IT
consider a wireless mimo multihop channel with n_s noncooperating source antennas and n_d fully cooperating destination antennas as well as l clusters containing k noncooperating relay antennas each the source signal traverses all l clusters of relay antennas before it reaches the destination when relay antennas within the same cluster scale their received signals by the same constant before the retransmission the equivalent channel matrix h relating the input signals at the source antennas to the output signals at the destination antennas is proportional to the product of channel matrices h_l l1l1 corresponding to the individual hops we perform an asymptotic capacity analysis for this channel as follows in a first instance we take the limits n_sinfty n_dinfty and kinfty but keep both n_sn_d and kn_d fixed then we take the limits linfty and kn_dinfty requiring that the h_ls satisfy the conditions needed for the marcenkopastur law we prove that the capacity scales linearly in minn_sn_d as long as the ratio kn_d scales at least linearly in l moreover we show that up to a noise penalty and a prelog factor the capacity of a pointtopoint mimo channel is approached when this scaling is slightly faster than linear conversely almost all spatial degrees of freedom vanish for less than linear scaling
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708.3568
A Polynomial-time Algorithm for Computing the Permanent in GF(3^q)
A polynomial-time algorithm for computing the permanent in any field of characteristic 3 is presented in this article. The principal objects utilized for that purpose are the Cauchy and Vandermonde matrices, the discriminant function and their generalizations of various types. Classical theorems on the permanent such as the Binet-Minc identity and Borchadt's formula are widely applied, while a special new technique involving the notion of limit re-defined for fields of finite characteristics and corresponding computational methods was developed in order to deal with a number of polynomial-time reductions. All the constructions preserve a strictly algebraic nature ignoring the structure of the basic field, while applying its infinite extensions for calculating limits. A natural corollary of the polynomial-time computability of the permanent in a field of a characteristic different from 2 is the non-uniform equality between the complexity classes P and NP what is equivalent to RP=NP (Ref. [1]).
cs.CC
a polynomialtime algorithm for computing the permanent in any field of characteristic 3 is presented in this article the principal objects utilized for that purpose are the cauchy and vandermonde matrices the discriminant function and their generalizations of various types classical theorems on the permanent such as the binetminc identity and borchadts formula are widely applied while a special new technique involving the notion of limit redefined for fields of finite characteristics and corresponding computational methods was developed in order to deal with a number of polynomialtime reductions all the constructions preserve a strictly algebraic nature ignoring the structure of the basic field while applying its infinite extensions for calculating limits a natural corollary of the polynomialtime computability of the permanent in a field of a characteristic different from 2 is the nonuniform equality between the complexity classes p and np what is equivalent to rpnp ref 1
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708.3569
The role of the quark and gluon GPDs in hard vector-meson electroproduction
Electroproduction of light vector mesons is analyzed on the basis of handbag factorization. The required generalized parton distributions are constructed from the CTEQ6 parton distributions with the help of double distributions. The partonic subprocesses are calculated within the modified perturbative approach. The present work extends our previous analysis of the longitudinal cross section to the transverse one and other observables related to both the corresponding amplitudes. Our results are compared to recent experimental findings in detail.
hep-ph
electroproduction of light vector mesons is analyzed on the basis of handbag factorization the required generalized parton distributions are constructed from the cteq6 parton distributions with the help of double distributions the partonic subprocesses are calculated within the modified perturbative approach the present work extends our previous analysis of the longitudinal cross section to the transverse one and other observables related to both the corresponding amplitudes our results are compared to recent experimental findings in detail
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708.357
Coherent destruction of tunneling, dynamic localization and the Landau-Zener formula
We clarify the internal relationship between the coherent destruction of tunneling (CDT) for a two-state model and the dynamic localization (DL) for a one-dimensional tight-binding model, under the periodical driving field. The time-evolution of the tight-binding model is reproduced from that of the two-state model by a mapping of equation of motion onto a set of ${\rm SU}(2)$ operators. It is shown that DL is effectively an infinitely large dimensional representation of the CDT in the ${\rm SU}(2)$ operators. We also show that both of the CDT and the DL can be interpreted as a result of destructive interference in repeated Landau-Zener level-crossings.
cond-mat.mes-hall
we clarify the internal relationship between the coherent destruction of tunneling cdt for a twostate model and the dynamic localization dl for a onedimensional tightbinding model under the periodical driving field the timeevolution of the tightbinding model is reproduced from that of the twostate model by a mapping of equation of motion onto a set of rm su2 operators it is shown that dl is effectively an infinitely large dimensional representation of the cdt in the rm su2 operators we also show that both of the cdt and the dl can be interpreted as a result of destructive interference in repeated landauzener levelcrossings
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708.3571
MAGIC multiwavelength observations: policy, and some recent results
MAGIC, 17 meters of diameter, is the world's largest single dish Imaging Atmospheric Cherenkov Telescope, and reaches in the analysis the lowest energy threshold (60 GeV) among the VHE gamma detectors. Completed in September 2004, MAGIC started full operation with its first cycle of data taking in February 2005. MAGIC observations in the galaxy cover, among others, supernova remnants, the Galactic Center and binary systems. The low threshold makes of MAGIC the IACT looking deepest in the Universe: the record of extragalactic sources detected includes Active Galactic Nuclei (AGN) at z > 0.2. Here we discuss the present performance of MAGIC and the policy for the use of MAGIC data in multiwavelength campaigns. After a review of some recent highlights from MW studies, including the discovery of the most distant source ever detected (the AGN 3C279 at z = 0.54), we present the expected performance of MAGIC after the inauguration of the second telescope, scheduled for September 21st, 2008. Multiwavelength studies are a key for the study of emission mechanisms from galactic and extragalactic sources, and Very-High Energy photon detectors are becoming crucial as the GLAST era approaches.
astro-ph
magic 17 meters of diameter is the worlds largest single dish imaging atmospheric cherenkov telescope and reaches in the analysis the lowest energy threshold 60 gev among the vhe gamma detectors completed in september 2004 magic started full operation with its first cycle of data taking in february 2005 magic observations in the galaxy cover among others supernova remnants the galactic center and binary systems the low threshold makes of magic the iact looking deepest in the universe the record of extragalactic sources detected includes active galactic nuclei agn at z 02 here we discuss the present performance of magic and the policy for the use of magic data in multiwavelength campaigns after a review of some recent highlights from mw studies including the discovery of the most distant source ever detected the agn 3c279 at z 054 we present the expected performance of magic after the inauguration of the second telescope scheduled for september 21st 2008 multiwavelength studies are a key for the study of emission mechanisms from galactic and extragalactic sources and veryhigh energy photon detectors are becoming crucial as the glast era approaches
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708.3572
Neutrino spin-flavor oscillations in electromagnetic fields of various configurations
We study spin-flavor oscillations of Dirac neutrinos with mixing and having non-zero matrix of magnetic moments in magnetic fields of various configurations. We discuss constant transversal and twisting magnetic fields. To describe the dynamics of Dirac neutrinos we use relativistic quantum mechanics approach based on the exact solutions to the Dirac-Pauli equation in an external electromagnetic field. We derive transition probabilities for different neutrino magnetic moments matrices.
hep-ph hep-th
we study spinflavor oscillations of dirac neutrinos with mixing and having nonzero matrix of magnetic moments in magnetic fields of various configurations we discuss constant transversal and twisting magnetic fields to describe the dynamics of dirac neutrinos we use relativistic quantum mechanics approach based on the exact solutions to the diracpauli equation in an external electromagnetic field we derive transition probabilities for different neutrino magnetic moments matrices
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708.3573
On the Outage Capacity of a Practical Decoder Accounting for Channel Estimation Inaccuracies
The optimal decoder achieving the outage capacity under imperfect channel estimation is investigated. First, by searching into the family of nearest neighbor decoders, which can be easily implemented on most practical coded modulation systems, we derive a decoding metric that minimizes the average of the transmission error probability over all channel estimation errors. Next, we specialize our general expression to obtain the corresponding decoding metric for fading MIMO channels. According to the notion of estimation-induced outage (EIO) capacity introduced in our previous work and assuming no channel state information (CSI) at the transmitter, we characterize maximal achievable information rates, using Gaussian codebooks, associated to the proposed decoder. In the case of uncorrelated Rayleigh fading, these achievable rates are compared to the rates achieved by the classical mismatched maximum-likelihood (ML) decoder and the ultimate limits given by the EIO capacity. Numerical results show that the derived metric provides significant gains for the considered scenario, in terms of achievable information rates and bit error rate (BER), in a bit interleaved coded modulation (BICM) framework, without introducing any additional decoding complexity.
cs.IT math.IT
the optimal decoder achieving the outage capacity under imperfect channel estimation is investigated first by searching into the family of nearest neighbor decoders which can be easily implemented on most practical coded modulation systems we derive a decoding metric that minimizes the average of the transmission error probability over all channel estimation errors next we specialize our general expression to obtain the corresponding decoding metric for fading mimo channels according to the notion of estimationinduced outage eio capacity introduced in our previous work and assuming no channel state information csi at the transmitter we characterize maximal achievable information rates using gaussian codebooks associated to the proposed decoder in the case of uncorrelated rayleigh fading these achievable rates are compared to the rates achieved by the classical mismatched maximumlikelihood ml decoder and the ultimate limits given by the eio capacity numerical results show that the derived metric provides significant gains for the considered scenario in terms of achievable information rates and bit error rate ber in a bit interleaved coded modulation bicm framework without introducing any additional decoding complexity
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708.3574
Nonadiabatic charge pumping in a one-dimensional system of noninteracting electrons by an oscillating potential
Using a tight-binding model, we study one-parameter charge pumping in a one-dimensional system of non-interacting electrons. An oscillating potential is applied at one site while a static potential is applied in a different region. Using Floquet scattering theory, we calculate the current up to second order in the oscillation amplitude and exactly in the oscillation frequency. For low frequency, the charge pumped per cycle is proportional to the frequency and therefore vanishes in the adiabatic limit. If the static potential has a bound state, we find that such a state has a significant effect on the pumped charge if the oscillating potential can excite the bound state into the continuum states or vice versa. Finally, we use the equation of motion for the density matrix to numerically compute the pumped current for any value of the amplitude and frequency. The numerical results confirm the unusual effect of a bound state.
cond-mat.mes-hall
using a tightbinding model we study oneparameter charge pumping in a onedimensional system of noninteracting electrons an oscillating potential is applied at one site while a static potential is applied in a different region using floquet scattering theory we calculate the current up to second order in the oscillation amplitude and exactly in the oscillation frequency for low frequency the charge pumped per cycle is proportional to the frequency and therefore vanishes in the adiabatic limit if the static potential has a bound state we find that such a state has a significant effect on the pumped charge if the oscillating potential can excite the bound state into the continuum states or vice versa finally we use the equation of motion for the density matrix to numerically compute the pumped current for any value of the amplitude and frequency the numerical results confirm the unusual effect of a bound state
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708.3575
How really effective are Multimodal Hints in enhancing Visual Target Spotting? Some evidence from a usability study
The main aim of the work presented here is to contribute to computer science advances in the multimodal usability area, in-as-much as it addresses one of the major issues relating to the generation of effective oral system messages: how to design messages which effectively help users to locate specific graphical objects in information visualisations? An experimental study was carried out to determine whether oral messages including coarse information on the locations of graphical objects on the current display may facilitate target detection tasks sufficiently for making it worth while to integrate such messages in GUIs. The display spatial layout varied in order to test the influence of visual presentation structure on the contribution of these messages to facilitating visual search on crowded displays. Finally, three levels of task difficulty were defined, based mainly on the target visual complexity and the number of distractors in the scene. The findings suggest that spatial information messages improve participants' visual search performances significantly; they are more appropriate to radial structures than to matrix, random and elleptic structures; and, they are particularly useful for performing difficult visual search tasks.
cs.HC
the main aim of the work presented here is to contribute to computer science advances in the multimodal usability area inasmuch as it addresses one of the major issues relating to the generation of effective oral system messages how to design messages which effectively help users to locate specific graphical objects in information visualisations an experimental study was carried out to determine whether oral messages including coarse information on the locations of graphical objects on the current display may facilitate target detection tasks sufficiently for making it worth while to integrate such messages in guis the display spatial layout varied in order to test the influence of visual presentation structure on the contribution of these messages to facilitating visual search on crowded displays finally three levels of task difficulty were defined based mainly on the target visual complexity and the number of distractors in the scene the findings suggest that spatial information messages improve participants visual search performances significantly they are more appropriate to radial structures than to matrix random and elleptic structures and they are particularly useful for performing difficult visual search tasks
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708.3576
Canonical Hilbert-Burch matrices for ideals of $k[x,y]$
An Artinian ideal $I$ of $k[x,y]$ has many Hilbert-Burch matrices. We show that there is a canonical choice. As an application, we determine the dimension of certain affine Gr\"obner cells and their Betti strata recovering results of Ellingsrud and Str{\o}mme, G\"ottsche and Iarrobino.
math.AC math.AG
an artinian ideal i of kxy has many hilbertburch matrices we show that there is a canonical choice as an application we determine the dimension of certain affine grobner cells and their betti strata recovering results of ellingsrud and stromme gottsche and iarrobino
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708.3577
An Equilibrium Balance of the Universe
An alternative cosmological model is presented, which avoids the requirement of dark energy and dark matter. Based on the proposition that energy conservation should be valid not only locally but also globally, the energy tensor of general relativity has to be corrected, including potential energy of matter explicitly. This leads to the consequence that a homogeneous universe must be static, as potential energy acts as a field with negative pressure. In this static universe cosmological red shift can be understood as energy loss by gravitational radiation. There exists a continuous matter cycle, beginning from hot intergalactic plasma, which is replenished by the jets of quasars, the formation of large web-like structures, the formation of galaxies and stars, to the final collapse into quasars again. The model is confirmed qualitatively by the observed size distribution of cosmic structures. Quantitative confirmation is obtained from the diffuse x-ray background and from observations of supernovas. As the total energy content of the universe (trace of the energy tensor) is zero in this model, creation ex nihilo is possible, but requires changes of our elementary particle models. An idea of a modified model is presented.
physics.gen-ph
an alternative cosmological model is presented which avoids the requirement of dark energy and dark matter based on the proposition that energy conservation should be valid not only locally but also globally the energy tensor of general relativity has to be corrected including potential energy of matter explicitly this leads to the consequence that a homogeneous universe must be static as potential energy acts as a field with negative pressure in this static universe cosmological red shift can be understood as energy loss by gravitational radiation there exists a continuous matter cycle beginning from hot intergalactic plasma which is replenished by the jets of quasars the formation of large weblike structures the formation of galaxies and stars to the final collapse into quasars again the model is confirmed qualitatively by the observed size distribution of cosmic structures quantitative confirmation is obtained from the diffuse xray background and from observations of supernovas as the total energy content of the universe trace of the energy tensor is zero in this model creation ex nihilo is possible but requires changes of our elementary particle models an idea of a modified model is presented
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708.3578
Relative Hyperbolicity, Trees of Spaces and Cannon-Thurston Maps
We prove the existence of continuous boundary extensions (Cannon-Thurston maps) for the inclusion of a vertex space into a tree of (strongly) relatively hyperbolic spaces satisfying the qi-embedded condition. This implies the same result for inclusion of vertex (or edge) subgroups in finite graphs of (strongly) relatively hyperbolic groups. This generalises a result of Bowditch for punctured surfaces in 3 manifolds and a result of Mitra for trees of hyperbolic metric spaces.
math.GR math.GT
we prove the existence of continuous boundary extensions cannonthurston maps for the inclusion of a vertex space into a tree of strongly relatively hyperbolic spaces satisfying the qiembedded condition this implies the same result for inclusion of vertex or edge subgroups in finite graphs of strongly relatively hyperbolic groups this generalises a result of bowditch for punctured surfaces in 3 manifolds and a result of mitra for trees of hyperbolic metric spaces
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708.3579
The Nature of the Gould Belt from a Fractal Analysis of its Stellar Population
The Gould Belt (GB) is a system of gas and young, bright stars distributed along a plane that is inclined with respect to the main plane of the Milky Way. Observational evidence suggests that the GB is our closest star formation complex, but its true nature and origin remain rather controversial. In this work we analyze the fractal structure of the stellar component of the GB. In order to do this, we tailor and apply an algorithm that estimates the fractal dimension in a precise and accurate way, avoiding both boundary and small data set problems. We find that early OB stars (of spectral types earlier than B4) in the GB have a fractal dimension very similar to that of the gas clouds in our Galaxy. On the contrary, stars in the GB of later spectral types show a larger fractal dimension, similar to that found for OB stars of both age groups in the local Galactic disk (LGD). This result seems to indicate that while the younger OB stars in the GB preserve the memory of the spatial structure of the cloud where they were born, older stars are distributed following a similar morphology as that found for the LGD stars. The possible causes for these differences are discussed.
astro-ph
the gould belt gb is a system of gas and young bright stars distributed along a plane that is inclined with respect to the main plane of the milky way observational evidence suggests that the gb is our closest star formation complex but its true nature and origin remain rather controversial in this work we analyze the fractal structure of the stellar component of the gb in order to do this we tailor and apply an algorithm that estimates the fractal dimension in a precise and accurate way avoiding both boundary and small data set problems we find that early ob stars of spectral types earlier than b4 in the gb have a fractal dimension very similar to that of the gas clouds in our galaxy on the contrary stars in the gb of later spectral types show a larger fractal dimension similar to that found for ob stars of both age groups in the local galactic disk lgd this result seems to indicate that while the younger ob stars in the gb preserve the memory of the spatial structure of the cloud where they were born older stars are distributed following a similar morphology as that found for the lgd stars the possible causes for these differences are discussed
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708.358
Ambient Multimodality: an Asset for Developing Universal Access to the Information Society
The paper tries to point out the benefits that can be derived from research advances in the implementation of concepts such as ambient intelligence (AmI) and ubiquitous or pervasive computing for promoting Universal Access (UA) to the Information Society, that is, for contributing to enable everybody, especially Physically Disabled (PD) people, to have easy access to all computing resources and information services that the coming worldwide Information Society will soon make available to the general public. Following definitions of basic concepts relating to multimodal interaction, the significant contribution of multimodality to developing UA is briefly argued. Then, a short state of the art in AmI research is presented. In the last section we bring out the potential contribution of advances in AmI research and technology to the improvement of computer access for PD people. This claim is supported by the following observations: (i) most projects aiming at implementing AmI focus on the design of new interaction modalities and flexible multimodal user interfaces which may facilitate PD users' computer access ; (ii) targeted applications will support users in a wide range of daily activities which will be performed simultaneously with supporting computing tasks; therefore, users will be placed in contexts where they will be confronted with similar difficulties to those encountered by PD users; (iii) AmI applications being intended for the general public, a wide range of new interaction devices and flexible processing software will be available, making it possible to provide PD users with human-computer facilities tailored to their specific needs at reasonable expense..
cs.HC
the paper tries to point out the benefits that can be derived from research advances in the implementation of concepts such as ambient intelligence ami and ubiquitous or pervasive computing for promoting universal access ua to the information society that is for contributing to enable everybody especially physically disabled pd people to have easy access to all computing resources and information services that the coming worldwide information society will soon make available to the general public following definitions of basic concepts relating to multimodal interaction the significant contribution of multimodality to developing ua is briefly argued then a short state of the art in ami research is presented in the last section we bring out the potential contribution of advances in ami research and technology to the improvement of computer access for pd people this claim is supported by the following observations i most projects aiming at implementing ami focus on the design of new interaction modalities and flexible multimodal user interfaces which may facilitate pd users computer access ii targeted applications will support users in a wide range of daily activities which will be performed simultaneously with supporting computing tasks therefore users will be placed in contexts where they will be confronted with similar difficulties to those encountered by pd users iii ami applications being intended for the general public a wide range of new interaction devices and flexible processing software will be available making it possible to provide pd users with humancomputer facilities tailored to their specific needs at reasonable expense
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708.3581
Hyper-atoms and the Kemperman's critical pair Theory
In the present work, we introduce the notion of a hyper-atom and prove their main structure theorem. We then apply the global isoperimetric methodology to give a new proof for Kemperman's structure Theory and a slight improvement.
math.NT math.CO
in the present work we introduce the notion of a hyperatom and prove their main structure theorem we then apply the global isoperimetric methodology to give a new proof for kempermans structure theory and a slight improvement
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708.3582
HORPO with Computability Closure : A Reconstruction
This paper provides a new, decidable definition of the higher- order recursive path ordering in which type comparisons are made only when needed, therefore eliminating the need for the computability clo- sure, and bound variables are handled explicitly, making it possible to handle recursors for arbitrary strictly positive inductive types.
cs.LO
this paper provides a new decidable definition of the higher order recursive path ordering in which type comparisons are made only when needed therefore eliminating the need for the computability clo sure and bound variables are handled explicitly making it possible to handle recursors for arbitrary strictly positive inductive types
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708.3583
Defining Relations of Low Degree of Invariants of Two $4 \times 4$ Matrices
Over a field K of characteristic 0, we study the algebra of invariants of the general linear group GL(4,K) acting by simultaneous conjugation on two matrices of order 4. It coincides with the trace algebra generated by all traces of products of two generic matrices of order 4. It is known that the minimal degree of the defining relations of any homogeneous minimal generating set of this algebra is equal to 12. Starting with the generating set given recently by Drensky and Sadikova, we have determined all relations of degree < 15. For this purpose we have developed further algorithms based on representation theory of the general linear group and easy computer calculations with standard functions of Maple.
math.RA math.AC
over a field k of characteristic 0 we study the algebra of invariants of the general linear group gl4k acting by simultaneous conjugation on two matrices of order 4 it coincides with the trace algebra generated by all traces of products of two generic matrices of order 4 it is known that the minimal degree of the defining relations of any homogeneous minimal generating set of this algebra is equal to 12 starting with the generating set given recently by drensky and sadikova we have determined all relations of degree 15 for this purpose we have developed further algorithms based on representation theory of the general linear group and easy computer calculations with standard functions of maple
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708.3584
Globular realization and cubical underlying homotopy type of time flow of process algebra
We construct a small realization as flow of every precubical set (modeling for example a process algebra). The realization is small in the sense that the construction does not make use of any cofibrant replacement functor and of any transfinite construction. In particular, if the precubical set is finite, then the corresponding flow has a finite globular decomposition. Two applications are given. The first one presents a realization functor from precubical sets to globular complexes which is characterized up to a natural S-homotopy. The second one proves that, for such flows, the underlying homotopy type is naturally isomorphic to the homotopy type of the standard cubical complex associated with the precubical set.
math.AT math.CT
we construct a small realization as flow of every precubical set modeling for example a process algebra the realization is small in the sense that the construction does not make use of any cofibrant replacement functor and of any transfinite construction in particular if the precubical set is finite then the corresponding flow has a finite globular decomposition two applications are given the first one presents a realization functor from precubical sets to globular complexes which is characterized up to a natural shomotopy the second one proves that for such flows the underlying homotopy type is naturally isomorphic to the homotopy type of the standard cubical complex associated with the precubical set
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708.3585
Critical conductance of the chiral 2d random flux model
The two-terminal conductance of a random flux model defined on a square lattice is investigated numerically at the band center using a transfer matrix method. Due to the chiral symmetry, there exists a critical point where the ensemble averaged mean conductance is scale independent. We also study the conductance distribution function which depends on the boundary conditions and on the number of lattice sites being even or odd. We derive a critical exponent $\nu=0.42\pm 0.05$ for square samples of even width using one-parameter scaling of the conductance. This result could not be obtained previously from the divergence of the localization length in quasi-one-dimensional systems due to pronounced finite-size effects.
cond-mat.mes-hall
the twoterminal conductance of a random flux model defined on a square lattice is investigated numerically at the band center using a transfer matrix method due to the chiral symmetry there exists a critical point where the ensemble averaged mean conductance is scale independent we also study the conductance distribution function which depends on the boundary conditions and on the number of lattice sites being even or odd we derive a critical exponent nu042pm 005 for square samples of even width using oneparameter scaling of the conductance this result could not be obtained previously from the divergence of the localization length in quasionedimensional systems due to pronounced finitesize effects
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708.3586
Calculations of $^{6}$He+p elastic scattering cross sections using folding approach and high-energy approximation for the optical potential
Calculations of microscopic optical potentials (OP's) (their real and imaginary parts) are performed to analyze the $^6$He+p elastic scattering data at a few tens of MeV/nucleon (MeV/N). The OP's and the cross sections are calculated using three model densities of $^6$He. Effects of the regularization of the NN forces and their dependence on nuclear density are investigated. Also, the role of the spin-orbit terms and of the non-linearity in the calculations of the OP's, as well as effects of their renormalization are studied. The sensitivity of the cross sections to the nuclear densities was tested and one of them that gives a better agreement with the data was chosen.
nucl-th
calculations of microscopic optical potentials ops their real and imaginary parts are performed to analyze the 6hep elastic scattering data at a few tens of mevnucleon mevn the ops and the cross sections are calculated using three model densities of 6he effects of the regularization of the nn forces and their dependence on nuclear density are investigated also the role of the spinorbit terms and of the nonlinearity in the calculations of the ops as well as effects of their renormalization are studied the sensitivity of the cross sections to the nuclear densities was tested and one of them that gives a better agreement with the data was chosen
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708.3587
Fixed points of smooth varieties with Kodaira dimension zero
In this paper, we study the growth of the number of fixed points from iterating an endomorphism of an abelian variety. Using the estimates obtained on an abelian variety, we are able to extend the results to endomorphisms on varieties of Kodaira dimension zero and more generally their periodic subvarieties.
math.AG
in this paper we study the growth of the number of fixed points from iterating an endomorphism of an abelian variety using the estimates obtained on an abelian variety we are able to extend the results to endomorphisms on varieties of kodaira dimension zero and more generally their periodic subvarieties
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708.3588
Electron-phonon coupling in a two-dimensional inhomogeneous electron gas: consequences for surface spectral properties
We investigate the coupling of an inhomogeneous electron system to phonons. The properties of an electronic system composed of a mixture of microscopic ordered and disordered islands are changed fundamentally by a phonon mode. In high-Tc cuprates, such a phase separation scenario is supported by recent STM and nuclear quadrupole resonance studies. We show that even a weak or moderate electron-phonon coupling can be sufficient to produce dramatic changes in the electronic state of the inhomogeneous electron gas. The spectral properties calculated in our approach provide a natural explanation of the low-energy nodal ARPES features and exhibit a novel non-Fermi-liquid state stabilized through electron-phonon coupling.
cond-mat.supr-con cond-mat.str-el
we investigate the coupling of an inhomogeneous electron system to phonons the properties of an electronic system composed of a mixture of microscopic ordered and disordered islands are changed fundamentally by a phonon mode in hightc cuprates such a phase separation scenario is supported by recent stm and nuclear quadrupole resonance studies we show that even a weak or moderate electronphonon coupling can be sufficient to produce dramatic changes in the electronic state of the inhomogeneous electron gas the spectral properties calculated in our approach provide a natural explanation of the lowenergy nodal arpes features and exhibit a novel nonfermiliquid state stabilized through electronphonon coupling
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708.3589
A First Principles Theory of Nuclear Magnetic Resonance J-Coupling in solid-state systems
A method to calculate NMR J-coupling constants from first principles in extended systems is presented. It is based on density functional theory and is formulated within a planewave-pseudopotential framework. The all-electron properties are recovered using the projector augmented wave approach. The method is validated by comparison with existing quantum chemical calculations of solution-state systems and with experimental data. The approach has been applied to verify measured J-coupling in a silicophosphate structure, Si5O(PO4)6
cond-mat.mtrl-sci
a method to calculate nmr jcoupling constants from first principles in extended systems is presented it is based on density functional theory and is formulated within a planewavepseudopotential framework the allelectron properties are recovered using the projector augmented wave approach the method is validated by comparison with existing quantum chemical calculations of solutionstate systems and with experimental data the approach has been applied to verify measured jcoupling in a silicophosphate structure si5opo46
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708.359
Torus knots are Fourier-(1,1,2) knots
Every torus knot can be represented as a Fourier-(1,1,2) knot which is the simplest possible Fourier representation for such a knot. This answers a question of Kauffman and confirms the conjecture made by Boocher, Daigle, Hoste and Zheng. In particular, the torus knot T(p,q) can be parameterized as x(t)=cos(pt), y(t)=cos(qt+pi/(2p)), and z(t)=cos(pt+pi/2)\cos((q-p)t+pi/(2p)-pi/(4q)).
math.GT
every torus knot can be represented as a fourier112 knot which is the simplest possible fourier representation for such a knot this answers a question of kauffman and confirms the conjecture made by boocher daigle hoste and zheng in particular the torus knot tpq can be parameterized as xtcospt ytcosqtpi2p and ztcosptpi2cosqptpi2ppi4q
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708.3591
Non commutative functional calculus: bounded operators
In this paper we develop a functional calculus for bounded operators defined on quaternionic Banach spaces. This calculus is based on the notion of slice-regularity, see \cite{gs}, and the key tools are a new resolvent operator and a new eigenvalue problem.
math.SP
in this paper we develop a functional calculus for bounded operators defined on quaternionic banach spaces this calculus is based on the notion of sliceregularity see citegs and the key tools are a new resolvent operator and a new eigenvalue problem
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708.3592
Non commutative functional calculus: unbounded operators
In a recent work, \cite{cgss}, we developed a functional calculus for bounded operators defined on quaternionic Banach spaces. In this paper we show how the results from \cite{cgss} can be extended to the unbounded case, and we highlight the crucial differences between the two cases. In particular, we deduce a new eigenvalue equation, suitable for the construction of a functional calculus for operators whose spectrum is not necessarily real.
math.SP
in a recent work citecgss we developed a functional calculus for bounded operators defined on quaternionic banach spaces in this paper we show how the results from citecgss can be extended to the unbounded case and we highlight the crucial differences between the two cases in particular we deduce a new eigenvalue equation suitable for the construction of a functional calculus for operators whose spectrum is not necessarily real
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708.3593
A hidden solution to the mu/B_mu problem in gauge mediation
We propose a solution to the mu/B_mu problem in gauge mediation. The novel feature of our solution is that it uses dynamics of the hidden sector, which is often present in models with dynamical supersymmetry breaking. We give an explicit example model of gauge mediation where a very simple messenger sector generates both mu and B_mu at one loop. The usual problem, that B_mu is then too large, is solved by strong renormalization effects from the hidden sector which suppress B_mu relative to mu. Our mechanism relies on an assumption about the signs of certain incalculable anomalous dimensions in the hidden sector. Making these assumptions not only allows us to solve the mu/B_mu problem but also leads to a characteristic superpartner spectrum which would be a smoking gun signal for our mechanism.
hep-ph hep-th
we propose a solution to the mub_mu problem in gauge mediation the novel feature of our solution is that it uses dynamics of the hidden sector which is often present in models with dynamical supersymmetry breaking we give an explicit example model of gauge mediation where a very simple messenger sector generates both mu and b_mu at one loop the usual problem that b_mu is then too large is solved by strong renormalization effects from the hidden sector which suppress b_mu relative to mu our mechanism relies on an assumption about the signs of certain incalculable anomalous dimensions in the hidden sector making these assumptions not only allows us to solve the mub_mu problem but also leads to a characteristic superpartner spectrum which would be a smoking gun signal for our mechanism
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708.3594
A new functional calculus for non-commuting operators
In this paper we use the notion of slice monogenic functions \cite{slicecss} to define a new functional calculus for an $n$-tuple $T$ of not necessarily commuting operators. This calculus is different from the one discussed in \cite{jefferies} and it allows the explicit construction of the eigenvalue equation for the $n$-tuple $T$ based on a new notion of spectrum for $T$. Our functional calculus is consistent with the Riesz-Dunford calculus in the case of a single operator.
math.SP
in this paper we use the notion of slice monogenic functions citeslicecss to define a new functional calculus for an ntuple t of not necessarily commuting operators this calculus is different from the one discussed in citejefferies and it allows the explicit construction of the eigenvalue equation for the ntuple t based on a new notion of spectrum for t our functional calculus is consistent with the rieszdunford calculus in the case of a single operator
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708.3595
Slice monogenic functions
In this paper we offer a definition of monogenicity for functions defined on $\rr^{n+1}$ with values in the Clifford algebra $\rr_n$ following an idea inspired by the recent papers \cite{gs}, \cite{advances}. This new class of monogenic functions contains the polynomials (and, more in general, power series) with coefficients in the Clifford algebra $\rr_n$. We will prove a Cauchy integral formula as well as some of its consequences. Finally, we deal with the zeroes of some polynomials and power series.
math.CV
in this paper we offer a definition of monogenicity for functions defined on rrn1 with values in the clifford algebra rr_n following an idea inspired by the recent papers citegs citeadvances this new class of monogenic functions contains the polynomials and more in general power series with coefficients in the clifford algebra rr_n we will prove a cauchy integral formula as well as some of its consequences finally we deal with the zeroes of some polynomials and power series
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708.3596
Chemical analysis and aqueous solution properties of Charged Amphiphilic Block Copolymers PBA-b-PAA synthesized by MADIX
We have linked the structural and dynamic properties in aqueous solution of amphiphilic charged diblock copolymers poly(butyl acrylate)-b-poly(acrylic acid), PBA-b-PAA, synthesized by controlled radical polymerization, with the physico-chemical characteristics of the samples. Despite product imperfections, the samples self-assemble in melt and aqueous solutions as predicted by monodisperse microphase separation theory. However, the PBA core are abnormally large; the swelling of PBA cores is not due to AA (the Flory parameter chiPBA/PAA, determined at 0.25, means strong segregation), but to h-PBA homopolymers (content determined by Liquid Chromatography at the Point of Exclusion and Adsorption Transition LC-PEAT). Beside the dominant population of micelles detected by scattering experiments, capillary electrophoresis CE analysis permitted detection of two other populations, one of h-PAA, and the other of free PBA-b-PAA chains, that have very short PBA blocks and never self-assemble. Despite the presence of these free unimers, the self-assembly in solution was found out of equilibrium: the aggregation state is history dependant and no unimer exchange between micelles occurs over months (time-evolution SANS). The high PBA/water interfacial tension, measured at 20 mN/m, prohibits unimer exchange between micelles. PBA-b-PAA solution systems are neither at thermal equilibrium nor completely frozen systems: internal fractionation of individual aggregates can occur.
cond-mat.soft
we have linked the structural and dynamic properties in aqueous solution of amphiphilic charged diblock copolymers polybutyl acrylatebpolyacrylic acid pbabpaa synthesized by controlled radical polymerization with the physicochemical characteristics of the samples despite product imperfections the samples selfassemble in melt and aqueous solutions as predicted by monodisperse microphase separation theory however the pba core are abnormally large the swelling of pba cores is not due to aa the flory parameter chipbapaa determined at 025 means strong segregation but to hpba homopolymers content determined by liquid chromatography at the point of exclusion and adsorption transition lcpeat beside the dominant population of micelles detected by scattering experiments capillary electrophoresis ce analysis permitted detection of two other populations one of hpaa and the other of free pbabpaa chains that have very short pba blocks and never selfassemble despite the presence of these free unimers the selfassembly in solution was found out of equilibrium the aggregation state is history dependant and no unimer exchange between micelles occurs over months timeevolution sans the high pbawater interfacial tension measured at 20 mnm prohibits unimer exchange between micelles pbabpaa solution systems are neither at thermal equilibrium nor completely frozen systems internal fractionation of individual aggregates can occur
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708.3597
Equilibrium Configurations of Strongly Magnetized Neutron Stars with Realistic Equations of State
We investigate equilibrium sequences of magnetized rotating stars with four kinds of realistic equations of state (EOSs) of SLy (Douchin et al.), FPS (Pandharipande et al.), Shen (Shen et al.), and LS (Lattimer & Swesty). Employing the Tomimura-Eriguchi scheme to construct the equilibrium configurations. we study the basic physical properties of the sequences in the framework of Newton gravity. In addition we newly take into account a general relativistic effect to the magnetized rotating configurations. With these computations, we find that the properties of the Newtonian magnetized stars, e.g., structure of magnetic field, highly depends on the EOSs. The toroidal magnetic fields concentrate rather near the surface for Shen and LS EOSs than those for SLy and FPS EOSs. The poloidal fields are also affected by the toroidal configurations. Paying attention to the stiffness of the EOSs, we analyze this tendency in detail. In the general relativistic stars, we find that the difference due to the EOSs becomes small because all the employed EOSs become sufficiently stiff for the large maximum density, typically greater than $10^{15}\rm{g} \rm{cm}^{-3}$. The maximum baryon mass of the magnetized stars with axis ratio $q\sim 0.7$ increases about up to twenty percents for that of spherical stars. We furthermore compute equilibrium sequences at finite temperature, which should serve as an initial condition for the hydrodynamic study of newly-born magnetars. Our results suggest that we may obtain information about the EOSs from the observation of the masses of magnetars.
astro-ph gr-qc
we investigate equilibrium sequences of magnetized rotating stars with four kinds of realistic equations of state eoss of sly douchin et al fps pandharipande et al shen shen et al and ls lattimer swesty employing the tomimuraeriguchi scheme to construct the equilibrium configurations we study the basic physical properties of the sequences in the framework of newton gravity in addition we newly take into account a general relativistic effect to the magnetized rotating configurations with these computations we find that the properties of the newtonian magnetized stars eg structure of magnetic field highly depends on the eoss the toroidal magnetic fields concentrate rather near the surface for shen and ls eoss than those for sly and fps eoss the poloidal fields are also affected by the toroidal configurations paying attention to the stiffness of the eoss we analyze this tendency in detail in the general relativistic stars we find that the difference due to the eoss becomes small because all the employed eoss become sufficiently stiff for the large maximum density typically greater than 1015rmg rmcm3 the maximum baryon mass of the magnetized stars with axis ratio qsim 07 increases about up to twenty percents for that of spherical stars we furthermore compute equilibrium sequences at finite temperature which should serve as an initial condition for the hydrodynamic study of newlyborn magnetars our results suggest that we may obtain information about the eoss from the observation of the masses of magnetars
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708.3598
Variations on Homological Reduction
In this paper, we are concerned with the BFV-reduction of first class constraints in classsical Hamiltonian mechanics and deformation quantization. As a result, we obtain continuous star products for certain singular reduced symplectic quotients. We relate the notion of "irreducibility" of a constraint to the notion of complete intersection used in commutative algebra. We generalize the classical BFV construction to the case of projective Tate generators using a super-Poisson bracket discovered by M. Rothstein. We also discuss the problem of infinite reducibility. Several examples are elaborated on.
math.QA math-ph math.MP
in this paper we are concerned with the bfvreduction of first class constraints in classsical hamiltonian mechanics and deformation quantization as a result we obtain continuous star products for certain singular reduced symplectic quotients we relate the notion of irreducibility of a constraint to the notion of complete intersection used in commutative algebra we generalize the classical bfv construction to the case of projective tate generators using a superpoisson bracket discovered by m rothstein we also discuss the problem of infinite reducibility several examples are elaborated on
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708.3599
Enzyme localization can drastically affect signal amplification in signal transduction pathways
Push-pull networks are ubiquitous in signal transduction pathways in both prokaryotic and eukaryotic cells. They allow cells to strongly amplify signals via the mechanism of zero-order ultrasensitivity. In a push-pull network, two antagonistic enzymes control the activity of a protein by covalent modification. These enzymes are often uniformly distributed in the cytoplasm. They can, however, also be colocalized in space, for instance, near the pole of the cell. Moreover, it is increasingly recognized that these enzymes can also be spatially separated, leading to gradients of the active form of the messenger protein. Here, we investigate the consequences of the spatial distributions of the enzymes for the amplification properties of push-pull networks. Our calculations reveal that enzyme localization by itself can have a dramatic effect on the gain. The gain is maximized when the two enzymes are either uniformly distributed or colocalized in one region in the cell. Depending on the diffusion constants, however, the sharpness of the response can be strongly reduced when the enzymes are spatially separated. We discuss how our predictions could be tested experimentally.
q-bio.MN
pushpull networks are ubiquitous in signal transduction pathways in both prokaryotic and eukaryotic cells they allow cells to strongly amplify signals via the mechanism of zeroorder ultrasensitivity in a pushpull network two antagonistic enzymes control the activity of a protein by covalent modification these enzymes are often uniformly distributed in the cytoplasm they can however also be colocalized in space for instance near the pole of the cell moreover it is increasingly recognized that these enzymes can also be spatially separated leading to gradients of the active form of the messenger protein here we investigate the consequences of the spatial distributions of the enzymes for the amplification properties of pushpull networks our calculations reveal that enzyme localization by itself can have a dramatic effect on the gain the gain is maximized when the two enzymes are either uniformly distributed or colocalized in one region in the cell depending on the diffusion constants however the sharpness of the response can be strongly reduced when the enzymes are spatially separated we discuss how our predictions could be tested experimentally
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708.36
Supersymmetric Candidates for Dark Matter (in German)
The identity of dark matter is one of the greatest puzzles of our Universe. Its solution may be associated with supersymmetry which is a fundamental space-time symmetry that has not been verified experimentally so far. In many supersymmetric extensions of the Standard Model of particle physics, the lightest supersymmetric particle cannot decay and is hence a promising dark matter candidate. The lightest neutralino, which appears already in the minimal supersymmetric model, can be identified as such a candidate in indirect and direct dark matter searches and at future colliders. As the superpartner of the graviton, the gravitino is another candidate for the lightest superparticle that provides a compelling explanation of dark matter. While it will neither be detected in indirect or direct searches nor be produced directly at accelerators, the analysis of late-decaying charged particles can allow for an experimental identification of the gravitino at future accelerators. In this way, the upcoming experiments at the CERN Large Hadron Collider may become a key to the understanding of our Universe.
hep-ph astro-ph hep-ex physics.pop-ph
the identity of dark matter is one of the greatest puzzles of our universe its solution may be associated with supersymmetry which is a fundamental spacetime symmetry that has not been verified experimentally so far in many supersymmetric extensions of the standard model of particle physics the lightest supersymmetric particle cannot decay and is hence a promising dark matter candidate the lightest neutralino which appears already in the minimal supersymmetric model can be identified as such a candidate in indirect and direct dark matter searches and at future colliders as the superpartner of the graviton the gravitino is another candidate for the lightest superparticle that provides a compelling explanation of dark matter while it will neither be detected in indirect or direct searches nor be produced directly at accelerators the analysis of latedecaying charged particles can allow for an experimental identification of the gravitino at future accelerators in this way the upcoming experiments at the cern large hadron collider may become a key to the understanding of our universe
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708.3601
A correlated topic model of Science
Topic models, such as latent Dirichlet allocation (LDA), can be useful tools for the statistical analysis of document collections and other discrete data. The LDA model assumes that the words of each document arise from a mixture of topics, each of which is a distribution over the vocabulary. A limitation of LDA is the inability to model topic correlation even though, for example, a document about genetics is more likely to also be about disease than X-ray astronomy. This limitation stems from the use of the Dirichlet distribution to model the variability among the topic proportions. In this paper we develop the correlated topic model (CTM), where the topic proportions exhibit correlation via the logistic normal distribution [J. Roy. Statist. Soc. Ser. B 44 (1982) 139--177]. We derive a fast variational inference algorithm for approximate posterior inference in this model, which is complicated by the fact that the logistic normal is not conjugate to the multinomial. We apply the CTM to the articles from Science published from 1990--1999, a data set that comprises 57M words. The CTM gives a better fit of the data than LDA, and we demonstrate its use as an exploratory tool of large document collections.
stat.AP
topic models such as latent dirichlet allocation lda can be useful tools for the statistical analysis of document collections and other discrete data the lda model assumes that the words of each document arise from a mixture of topics each of which is a distribution over the vocabulary a limitation of lda is the inability to model topic correlation even though for example a document about genetics is more likely to also be about disease than xray astronomy this limitation stems from the use of the dirichlet distribution to model the variability among the topic proportions in this paper we develop the correlated topic model ctm where the topic proportions exhibit correlation via the logistic normal distribution j roy statist soc ser b 44 1982 139177 we derive a fast variational inference algorithm for approximate posterior inference in this model which is complicated by the fact that the logistic normal is not conjugate to the multinomial we apply the ctm to the articles from science published from 19901999 a data set that comprises 57m words the ctm gives a better fit of the data than lda and we demonstrate its use as an exploratory tool of large document collections
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708.3602
Strain-driven elastic and orbital-ordering effects on thickness-dependent properties of manganite thin films
We report on the structural and magnetic characterization of (110) and (001) La2/3Ca1/3MnO3 (LCMO) epitaxial thin films simultaneously grown on (110) and (001)SrTiO3 substrates, with thicknesses t varying between 8 nm and 150 nm. It is found that while the in-plane interplanar distances of the (001) films are strongly clamped to those of the substrate and the films remain strained up to well above t=100 nm, the (110) films relax much earlier. Accurate determination of the in-plane and out-of-plane interplanar distances has allowed concluding that in all cases the unit cell volume of the manganite reduces gradually when increasing thickness, approaching the bulk value. It is observed that the magnetic properties (Curie temperature and saturation magnetization) of the (110) films are significantly improved compared to those of (001) films. These observations, combined with 55Mn-nuclear magnetic resonance data and X-ray photoemission spectroscopy, signal that the depression of the magnetic properties of the more strained (001)LCMO films is not caused by an elastic deformation of the perovskite lattice but rather due to the electronic and chemical phase separation caused by the substrate-induced strain. On the contrary, the thickness dependence of the magnetic properties of the less strained (110)LCMO films are simply described by the elastic deformation of the manganite lattice. We will argue that the different behavior of (001) and (110)LCMO films is a consequence of the dissimilar electronic structure of these interfaces.
cond-mat.mtrl-sci
we report on the structural and magnetic characterization of 110 and 001 la23ca13mno3 lcmo epitaxial thin films simultaneously grown on 110 and 001srtio3 substrates with thicknesses t varying between 8 nm and 150 nm it is found that while the inplane interplanar distances of the 001 films are strongly clamped to those of the substrate and the films remain strained up to well above t100 nm the 110 films relax much earlier accurate determination of the inplane and outofplane interplanar distances has allowed concluding that in all cases the unit cell volume of the manganite reduces gradually when increasing thickness approaching the bulk value it is observed that the magnetic properties curie temperature and saturation magnetization of the 110 films are significantly improved compared to those of 001 films these observations combined with 55mnnuclear magnetic resonance data and xray photoemission spectroscopy signal that the depression of the magnetic properties of the more strained 001lcmo films is not caused by an elastic deformation of the perovskite lattice but rather due to the electronic and chemical phase separation caused by the substrateinduced strain on the contrary the thickness dependence of the magnetic properties of the less strained 110lcmo films are simply described by the elastic deformation of the manganite lattice we will argue that the different behavior of 001 and 110lcmo films is a consequence of the dissimilar electronic structure of these interfaces
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708.3603
Chiral symmetry breaking and the Lorentz nature of confinement
We address the question of the Lorentz nature of the effective interquark interaction in QCD which leads to the formation of the QCD string between colour charges. In particular, we start from a manifestly vectorial fundamental interaction mediated by gluons and demonstrate that, as soon as chiral symmetry is broken spontaneously, the effective interquark interaction acquires a selfconsistently generated scalar part which is eventually responsible for the formation of the QCD string. We demonstrate this explicitly for a heavy-light quarkonium, using the approach of the Schwinger-Dyson-type equation and the quantum-mechanical Hamiltonian method of the QCD string with quarks at the ends.
hep-ph
we address the question of the lorentz nature of the effective interquark interaction in qcd which leads to the formation of the qcd string between colour charges in particular we start from a manifestly vectorial fundamental interaction mediated by gluons and demonstrate that as soon as chiral symmetry is broken spontaneously the effective interquark interaction acquires a selfconsistently generated scalar part which is eventually responsible for the formation of the qcd string we demonstrate this explicitly for a heavylight quarkonium using the approach of the schwingerdysontype equation and the quantummechanical hamiltonian method of the qcd string with quarks at the ends
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708.3604
Looking for the Kondo cloud
We study the spatial distribution of the Kondo screening cloud. We find that in 3 D the spatial range of the cloud is limited to distances of the order of the Fermi wavelength due to angular dispersion effects. In lower dimensions this effect is less important and thus the Kondo length determines the localization of the cloud around the magnetic impurity. We clarify the role of the Kondo cloud in the impurity-impurity interactions: the hole coherence factor of the Kondo-doublet interaction is proportional to the amplitude of the Kondo cloud. We single out an experimental setup in which the Kondo cloud could be directly measured.
cond-mat.mes-hall cond-mat.str-el
we study the spatial distribution of the kondo screening cloud we find that in 3 d the spatial range of the cloud is limited to distances of the order of the fermi wavelength due to angular dispersion effects in lower dimensions this effect is less important and thus the kondo length determines the localization of the cloud around the magnetic impurity we clarify the role of the kondo cloud in the impurityimpurity interactions the hole coherence factor of the kondodoublet interaction is proportional to the amplitude of the kondo cloud we single out an experimental setup in which the kondo cloud could be directly measured
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708.3605
Cosmological simulations using a static scalar-tensor theory
We present $\Lambda$CDM $N$-body cosmological simulations in the framework of a static general scalar-tensor theory of gravity. Due to the influence of the non-minimally coupled scalar field, the gravitational potential is modified by a Yukawa type term, yielding a new structure formation dynamics. We present some preliminary results and, in particular, we compute the density and velocity profiles of the most massive group.
astro-ph
we present lambdacdm nbody cosmological simulations in the framework of a static general scalartensor theory of gravity due to the influence of the nonminimally coupled scalar field the gravitational potential is modified by a yukawa type term yielding a new structure formation dynamics we present some preliminary results and in particular we compute the density and velocity profiles of the most massive group
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708.3606
Variable Cosmological Constant model: the reconstruction equations and constraints from current observational data
In this paper we first give a brief review of the variable cosmological constant model and its scalar field description. We mainly discuss two types of variable cosmological constant models: $a$ power law and $H$ power law models. A method to obtain all of the equivalent scalar field potentials and the effective equation of state of the two models is presented. In addition, the dynamics of such scalar field potentials and effective equation of state are discussed in detail. The parameters of the two models are constrained by current 307 high-quality "Union" SN Ia data set, baryon acoustic oscillation (BAO) measurement from the Sloan Digital Sky Survey (SDSS), 9 observational \textrm{H(z)} data derived from the Gemini Deep Deep Survey (GDDS) and the shift parameter of the cosmic microwave background (CMB) given by the three-year Wilkinson Microwave Anisotropy Probe (\textrm{WMAP}) observations. We also calculate and draw the picture of the Hubble parameter, the deceleration parameter and the matter density of the two models. Then, we show that the indices $m$ and $n$ in the two models have specific meaning in determining properties of the models. Moreover, The reasons that indices $m$ and $n$ may also influence the behavior of effective equation of state and scalar field potentials are presented.
astro-ph
in this paper we first give a brief review of the variable cosmological constant model and its scalar field description we mainly discuss two types of variable cosmological constant models a power law and h power law models a method to obtain all of the equivalent scalar field potentials and the effective equation of state of the two models is presented in addition the dynamics of such scalar field potentials and effective equation of state are discussed in detail the parameters of the two models are constrained by current 307 highquality union sn ia data set baryon acoustic oscillation bao measurement from the sloan digital sky survey sdss 9 observational textrmhz data derived from the gemini deep deep survey gdds and the shift parameter of the cosmic microwave background cmb given by the threeyear wilkinson microwave anisotropy probe textrmwmap observations we also calculate and draw the picture of the hubble parameter the deceleration parameter and the matter density of the two models then we show that the indices m and n in the two models have specific meaning in determining properties of the models moreover the reasons that indices m and n may also influence the behavior of effective equation of state and scalar field potentials are presented
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708.3607
Parametric stiffness analysis of the Orthoglide
This paper presents a parametric stiffness analysis of the Orthoglide. A compliant modeling and a symbolic expression of the stiffness matrix are conducted. This allows a simple systematic analysis of the influence of the geometric design parameters and to quickly identify the critical link parameters. Our symbolic model is used to display the stiffest areas of the workspace for a specific machining task. Our approach can be applied to any parallel manipulator for which stiffness is a critical issue.
cs.RO
this paper presents a parametric stiffness analysis of the orthoglide a compliant modeling and a symbolic expression of the stiffness matrix are conducted this allows a simple systematic analysis of the influence of the geometric design parameters and to quickly identify the critical link parameters our symbolic model is used to display the stiffest areas of the workspace for a specific machining task our approach can be applied to any parallel manipulator for which stiffness is a critical issue
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708.3608
Continuous functions taking every value a given number of times
We give necessary and sufficient conditions on a function $f:[0,1]\to {0,1,2,...,\omega,\continuum}$ under which there exists a continuous function $F:[0,1]\to [0,1]$ such that for every $y\in[0,1]$ we have $|F^{-1}(y)|=f(y)$.
math.LO math.GN
we give necessary and sufficient conditions on a function f01to 012omegacontinuum under which there exists a continuous function f01to 01 such that for every yin01 we have f1yfy
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708.3609
Thompson's Group F
We introduce forest diagrams and strand diagrams for elements of Thompson's group F. A forest diagram is a pair of infinite, bounded binary forests together with an order-preserving bijection of the leaves. Using forest diagrams, we derive a simple length formula for elements of F, and we discuss applications to the geometry of the Cayley graph, including a new upper bound on the isoperimetric constant (a.k.a. Cheeger constant) of F. Strand diagrams are similar to tree diagrams, but they can be concatenated like braids. Motivated by the fact that configuration spaces are classifying spaces for braid groups, we present a classifying space for F that is the ``configuration space'' of finitely many points on a line, with the points allowed to split and merge in pairs. Strand diagrams are related to a description of F as a groupoid, which we use to derive presentations for F, T, V, and the braided Thompson group BV. In addition to the new results, we include a thorough exposition of the basic theory of the group F. Highlights include a simplified proof that the commutator subgroup of F is simple, a discussion of open problems (with a focus on amenability), and a simplified derivation of the standard presentation and normal forms for F using forest diagrams.
math.GR
we introduce forest diagrams and strand diagrams for elements of thompsons group f a forest diagram is a pair of infinite bounded binary forests together with an orderpreserving bijection of the leaves using forest diagrams we derive a simple length formula for elements of f and we discuss applications to the geometry of the cayley graph including a new upper bound on the isoperimetric constant aka cheeger constant of f strand diagrams are similar to tree diagrams but they can be concatenated like braids motivated by the fact that configuration spaces are classifying spaces for braid groups we present a classifying space for f that is the configuration space of finitely many points on a line with the points allowed to split and merge in pairs strand diagrams are related to a description of f as a groupoid which we use to derive presentations for f t v and the braided thompson group bv in addition to the new results we include a thorough exposition of the basic theory of the group f highlights include a simplified proof that the commutator subgroup of f is simple a discussion of open problems with a focus on amenability and a simplified derivation of the standard presentation and normal forms for f using forest diagrams
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708.361
Heavy-heavy-light quark potential in SU(3) lattice QCD
We perform the first study for the heavy-heavy-light quark (QQq) potential in SU(3) lattice QCD. The calculations are done with the standard gauge and $O(a)$-improved Wilson fermion action on the $16^4$ lattice at $\beta =6.0$ at the quenched level. We calculate the energy of QQq systems as the function of the distance between the two heavy quarks, and find that the QQq potential is well described with a Coulomb plus linear potential form. Compared to the static three-quark case, the Coulomb term does not change but the effective string tension between the heavy quarks is significantly reduced by the light-quark effect. We also investigate the light-quark mass dependence of the QQq potential using the four hopping parameters, $\kappa =0.1200,0.1300,0.1340$, and 0.1380. The reduction of the effective string tension is considered to be a general property for baryons and multi-quark hadrons.
hep-lat
we perform the first study for the heavyheavylight quark qqq potential in su3 lattice qcd the calculations are done with the standard gauge and oaimproved wilson fermion action on the 164 lattice at beta 60 at the quenched level we calculate the energy of qqq systems as the function of the distance between the two heavy quarks and find that the qqq potential is well described with a coulomb plus linear potential form compared to the static threequark case the coulomb term does not change but the effective string tension between the heavy quarks is significantly reduced by the lightquark effect we also investigate the lightquark mass dependence of the qqq potential using the four hopping parameters kappa 012000130001340 and 01380 the reduction of the effective string tension is considered to be a general property for baryons and multiquark hadrons
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708.3611
Structural and dynamical characteristics of mesoscopic H$^+$[H$_2$O]$_n$ clusters
Structural and dynamical characteristics pertaining to the solvation of an excess proton in liquid-like nanoclusters of the type [H$_2$O]$_n$ are investigated using Molecular Dynamics experiments. Three different aggregate sizes were analyzed: $n=10,$ 21 and 125. The simulation experiments were performed using a multistate empirical valence bond Hamiltonian model. While in the smallest aggregates the proton occupies a central position, the stable solvation environments for $n=21$ and 125 are located at the cluster boundaries. In all cases, the structure of the closest solvation shell of the excess charge remains practically unchanged and coincides with that observed in bulk water. Compared to results obtained in bulk, the computed rates for proton transfer in clusters are between one and two orders of magnitude slower, and tend to increase for larger cluster sizes.
physics.chem-ph physics.atm-clus physics.comp-ph
structural and dynamical characteristics pertaining to the solvation of an excess proton in liquidlike nanoclusters of the type h_2o_n are investigated using molecular dynamics experiments three different aggregate sizes were analyzed n10 21 and 125 the simulation experiments were performed using a multistate empirical valence bond hamiltonian model while in the smallest aggregates the proton occupies a central position the stable solvation environments for n21 and 125 are located at the cluster boundaries in all cases the structure of the closest solvation shell of the excess charge remains practically unchanged and coincides with that observed in bulk water compared to results obtained in bulk the computed rates for proton transfer in clusters are between one and two orders of magnitude slower and tend to increase for larger cluster sizes
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708.3612
CP Asymmetries in Higgs decays to ZZ at the LHC
We examine the effect of a general HZZ coupling through a study of the Higgs decay to leptons via Z bosons at the LHC. We discuss various methods for placing limits on additional couplings, including measurement of the partial width, threshold scans, and asymmetries constructed from angular observables. We find that only the asymmetries provide a definitive test of additional couplings. We further estimate the significances they provide.
hep-ph
we examine the effect of a general hzz coupling through a study of the higgs decay to leptons via z bosons at the lhc we discuss various methods for placing limits on additional couplings including measurement of the partial width threshold scans and asymmetries constructed from angular observables we find that only the asymmetries provide a definitive test of additional couplings we further estimate the significances they provide
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708.3613
Kinematics and Workspace Analysis of a Three-Axis Parallel Manipulator: the Orthoglide
The paper addresses kinematic and geometrical aspects of the Orthoglide, a three-DOF parallel mechanism. This machine consists of three fixed linear joints, which are mounted orthogonally, three identical legs and a mobile platform, which moves in the Cartesian x-y-z space with fixed orientation. New solutions to solve inverse/direct kinematics are proposed and we perform a detailed workspace and singularity analysis, taking into account specific joint limit constraints.
cs.RO
the paper addresses kinematic and geometrical aspects of the orthoglide a threedof parallel mechanism this machine consists of three fixed linear joints which are mounted orthogonally three identical legs and a mobile platform which moves in the cartesian xyz space with fixed orientation new solutions to solve inversedirect kinematics are proposed and we perform a detailed workspace and singularity analysis taking into account specific joint limit constraints
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708.3614
Correlated $\Lambda d$ pairs from the $K^{-}_{stop} A \to \Lambda d A'$ reaction
Correlated $\Lambda d$ pairs emitted after the absorption of negative kaons at rest $K^{-}_{stop}A\to \Lambda d A'$ in light nuclei $^6Li$ and $^{12}C$ are studied. $\Lambda$-hyperons and deuterons are found to be preferentially emitted in opposite directions. The $\Lambda d$ invariant mass spectrum of $^6Li$ shows a bump whose mass is 3251$\pm$6 MeV/c$^2$. The bump mass (binding energy), width and yield are reported. The appearance of a bump is discussed in the realm of the [$\bar{K}3N$] clustering process in nuclei. The experiment was performed with the FINUDA spectrometer at DA$\Phi$NE (LNF).
nucl-ex
correlated lambda d pairs emitted after the absorption of negative kaons at rest k_stopato lambda d a in light nuclei 6li and 12c are studied lambdahyperons and deuterons are found to be preferentially emitted in opposite directions the lambda d invariant mass spectrum of 6li shows a bump whose mass is 3251pm6 mevc2 the bump mass binding energy width and yield are reported the appearance of a bump is discussed in the realm of the bark3n clustering process in nuclei the experiment was performed with the finuda spectrometer at daphine lnf
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708.3615
Relativistic iron emission lines in neutron star low-mass X-ray binaries as probes of neutron star radii
Using Suzaku observations of three neutron star low-mass X-ray binaries (Ser X-1, 4U 1820-30 and GX 349+2) we have found broad, asymmetric, relativistic Fe K emission lines in all three objects. These Fe K lines can be well fit by a model for lines from a relativistic accretion disk ('diskline'), allowing a measurement of the inner radius of the accretion disk, and hence an upper limit on the neutron star radius. These upper limits correspond to 14.5 - 16.5 km for a 1.4 M(solar) neutron star. The inner disk radii we measure with Fe K lines are in good agreement with the inner disk radii implied by kHz QPOs observed in both 4U 1820-30 and GX 349+2, supporting the inner disk nature of kHz QPOs. Additionally, the Fe K lines observed in these neutron stars are narrower than those in the black holes that are thought to be close to maximally spinning, as one would expect if inferences for spin are robust.
astro-ph
using suzaku observations of three neutron star lowmass xray binaries ser x1 4u 182030 and gx 3492 we have found broad asymmetric relativistic fe k emission lines in all three objects these fe k lines can be well fit by a model for lines from a relativistic accretion disk diskline allowing a measurement of the inner radius of the accretion disk and hence an upper limit on the neutron star radius these upper limits correspond to 145 165 km for a 14 msolar neutron star the inner disk radii we measure with fe k lines are in good agreement with the inner disk radii implied by khz qpos observed in both 4u 182030 and gx 3492 supporting the inner disk nature of khz qpos additionally the fe k lines observed in these neutron stars are narrower than those in the black holes that are thought to be close to maximally spinning as one would expect if inferences for spin are robust
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708.3616
Hydrodynamic simulations of irradiated secondaries in dwarf novae
We investigate numerically the surface flow on the secondary star during outbursts. We use a simple model for the irradiation and the geometry of the secondary star: the irradiation temperature is treated as a free parameter and the secondary is replaced by a spherical star with a space-dependent Coriolis force that mimics the effect of the Roche geometry. The Euler equations are solved in spherical coordinates with the TVD-MacCormack scheme. We show that the Coriolis force leads to the formation of a circulation flow from high latitude region to the close vicinity of the $L_1$ point. However no heat can be efficiently transported to the $L_1$ region due to the rapid radiative cooling of the hot material as it enters the equatorial belt shadowed from irradiation. Under the assumption of hydrostatic equilibrium, the Coriolis force could lead to a moderate increase of the mass transfer rate by pushing the gas in the vertical direction at the $L_1$ point, but only during the initial phases of the outburst (about 15 -- 20 orbital periods). We conclude that the Coriolis force does not prevent a flow from the heated regions of the secondary towards the $L_1$ region, at least during the initial phase of an outburst, but the resulting increase of the mass transfer rate is moderate, and it is unlikely to be able to account for the duration of long outbursts.
astro-ph
we investigate numerically the surface flow on the secondary star during outbursts we use a simple model for the irradiation and the geometry of the secondary star the irradiation temperature is treated as a free parameter and the secondary is replaced by a spherical star with a spacedependent coriolis force that mimics the effect of the roche geometry the euler equations are solved in spherical coordinates with the tvdmaccormack scheme we show that the coriolis force leads to the formation of a circulation flow from high latitude region to the close vicinity of the l_1 point however no heat can be efficiently transported to the l_1 region due to the rapid radiative cooling of the hot material as it enters the equatorial belt shadowed from irradiation under the assumption of hydrostatic equilibrium the coriolis force could lead to a moderate increase of the mass transfer rate by pushing the gas in the vertical direction at the l_1 point but only during the initial phases of the outburst about 15 20 orbital periods we conclude that the coriolis force does not prevent a flow from the heated regions of the secondary towards the l_1 region at least during the initial phase of an outburst but the resulting increase of the mass transfer rate is moderate and it is unlikely to be able to account for the duration of long outbursts
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708.3617
Spin relaxation in the impurity band of a semiconductor in the external magnetic field
Spin relaxation in the impurity band of a 2D semiconductor with spin-split spectrum in the external magnetic field is considered. Several mechanisms of spin relaxation are shown to be relevant. The first one is attributed to phonon-assisted transitions between Zeeman sublevels of the ground state of an isolated impurity, while other mechanisms can be described in terms of spin precession in a random magnetic field during the electron motion over the impurity band. In the later case there are two contributions to the spin relaxation: the one given by optimal impurity configurations with the hop-waiting time inversely proportional to the external magnetic field and another one related to the electron motion on a large scale. The average spin relaxation rate is calculated.
cond-mat.mes-hall
spin relaxation in the impurity band of a 2d semiconductor with spinsplit spectrum in the external magnetic field is considered several mechanisms of spin relaxation are shown to be relevant the first one is attributed to phononassisted transitions between zeeman sublevels of the ground state of an isolated impurity while other mechanisms can be described in terms of spin precession in a random magnetic field during the electron motion over the impurity band in the later case there are two contributions to the spin relaxation the one given by optimal impurity configurations with the hopwaiting time inversely proportional to the external magnetic field and another one related to the electron motion on a large scale the average spin relaxation rate is calculated
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708.3618
Diffusive-Ballistic Crossover and the Persistent Spin Helix
Conventional transport theory focuses on either the diffusive or ballistic regimes and neglects the crossover region between the two. In the presence of spin-orbit coupling, the transport equations are known only in the diffusive regime, where the spin precession angle is small. In this paper, we develop a semiclassical theory of transport valid throughout the diffusive - ballistic crossover of a special SU(2) symmetric spin-orbit coupled system. The theory is also valid in the physically interesting regime where the spin precession angle is large. We obtain exact expressions for the density and spin structure factors in both 2 and 3 dimensional samples with spin-orbit coupling.
cond-mat.mes-hall
conventional transport theory focuses on either the diffusive or ballistic regimes and neglects the crossover region between the two in the presence of spinorbit coupling the transport equations are known only in the diffusive regime where the spin precession angle is small in this paper we develop a semiclassical theory of transport valid throughout the diffusive ballistic crossover of a special su2 symmetric spinorbit coupled system the theory is also valid in the physically interesting regime where the spin precession angle is large we obtain exact expressions for the density and spin structure factors in both 2 and 3 dimensional samples with spinorbit coupling
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708.3619
Explicit Evaluation of Certain Exponential Sums of Quadratic Functions over $\Bbb F_{p^n}$, $p$ Odd
Let $p$ be an odd prime and let $f(x)=\sum_{i=1}^ka_ix^{p^{\alpha_i}+1}\in\Bbb F_{p^n}[x]$, where $0\le \alpha_1<...<\alpha_k$. We consider the exponential sum $S(f,n)=\sum_{x\in\Bbb F_{p^n}}e_n(f(x))$, where $e_n(y)=e^{2\pi i\text{Tr}_n(y)/p}$, $y\in\Bbb F_{p^n}$, $\text{Tr}_n=\text{Tr}_{\Bbb F_{p^n}/\Bbb F_p}$. There is an effective way to compute the nullity of the quadratic form $\text{Tr}_{mn}(f(x))$ for all integer $m>0$. Assuming that all such nullities are known, we find relative formulas for $S(f,mn)$ in terms of $S(f,n)$ when $\nu_p(m) \le \min\{\nu_p(\alpha_i):1\le i\le k\}$, where $\nu_p$ is the $p$-adic order. We also find an explicit formula for $S(f,n)$ when $\nu_2(\alpha_1)=...= \nu_2(\alpha_k)<\nu_2(n)$. These results generalize those by Carlitz and by Baumert and McEliece. Parallel results with $p=2$ were obtained in a previous paper by the second author.
math.NT
let p be an odd prime and let fxsum_i1ka_ixpalpha_i1inbbb f_pnx where 0le alpha_1alpha_k we consider the exponential sum sfnsum_xinbbb f_pne_nfx where e_nye2pi itexttr_nyp yinbbb f_pn texttr_ntexttr_bbb f_pnbbb f_p there is an effective way to compute the nullity of the quadratic form texttr_mnfx for all integer m0 assuming that all such nullities are known we find relative formulas for sfmn in terms of sfn when nu_pm le minnu_palpha_i1le ile k where nu_p is the padic order we also find an explicit formula for sfn when nu_2alpha_1 nu_2alpha_knu_2n these results generalize those by carlitz and by baumert and mceliece parallel results with p2 were obtained in a previous paper by the second author
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708.362
Heavy Ion Collisions and New Forms of Matter
I discuss forms of high energy density matter in QCD. These include the Color Glass Condensate, the Glasma and the Quark Gluon Plasma. They all might be studied in ultra-relativistic heavy ion collisions, nd the Color Glass Condensate might also be probed in electron-hadron collisions. I present the properties of such matter and some aspects of what is known of their properties.
hep-ph
i discuss forms of high energy density matter in qcd these include the color glass condensate the glasma and the quark gluon plasma they all might be studied in ultrarelativistic heavy ion collisions nd the color glass condensate might also be probed in electronhadron collisions i present the properties of such matter and some aspects of what is known of their properties
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708.3621
The $\mathcal{Q}_p$ Carleson Measure Problem
Let $\mu$ be a nonnegative Borel measure on the open unit disk $\mathbb{D}\subset\mathbb{C}$. This note shows how to decide that the M\"obius invariant space $\mathcal{Q}_p$, covering $\mathcal{BMOA}$ and $\mathcal{B}$, is boundedly (resp., compactly) embedded in the quadratic tent-type space $T^\infty_p(\mu)$. Interestingly, the embedding result can be used to determine the boundedness (resp., the compactness) of the Volterra-type and multiplication operators on $\mathcal{Q}_p$.
math.CV math.FA
let mu be a nonnegative borel measure on the open unit disk mathbbdsubsetmathbbc this note shows how to decide that the mobius invariant space mathcalq_p covering mathcalbmoa and mathcalb is boundedly resp compactly embedded in the quadratic tenttype space tinfty_pmu interestingly the embedding result can be used to determine the boundedness resp the compactness of the volterratype and multiplication operators on mathcalq_p
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708.3622
On cosmological observables in a swiss-cheese universe
Photon geodesics are calculated in a swiss-cheese model, where the cheese is made of the usual Friedmann-Robertson-Walker solution and the holes are constructed from a Lemaitre-Tolman-Bondi solution of Einstein's equations. The observables on which we focus are the changes in the redshift, in the angular-diameter--distance relation, in the luminosity-distance--redshift relation, and in the corresponding distance modulus. We find that redshift effects are suppressed when the hole is small because of a compensation effect acting on the scale of half a hole resulting from the special case of spherical symmetry. However, we find interesting effects in the calculation of the angular distance: strong evolution of the inhomogeneities (as in the approach to caustic formation) causes the photon path to deviate from that of the FRW case. Therefore, the inhomogeneities are able to partly mimic the effects of a dark-energy component. Our results also suggest that the nonlinear effects of caustic formation in cold dark matter models may lead to interesting effects on photon trajectories.
astro-ph gr-qc
photon geodesics are calculated in a swisscheese model where the cheese is made of the usual friedmannrobertsonwalker solution and the holes are constructed from a lemaitretolmanbondi solution of einsteins equations the observables on which we focus are the changes in the redshift in the angulardiameterdistance relation in the luminositydistanceredshift relation and in the corresponding distance modulus we find that redshift effects are suppressed when the hole is small because of a compensation effect acting on the scale of half a hole resulting from the special case of spherical symmetry however we find interesting effects in the calculation of the angular distance strong evolution of the inhomogeneities as in the approach to caustic formation causes the photon path to deviate from that of the frw case therefore the inhomogeneities are able to partly mimic the effects of a darkenergy component our results also suggest that the nonlinear effects of caustic formation in cold dark matter models may lead to interesting effects on photon trajectories
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708.3623
Derangements and Relative Derangements of Type $B$
By introducing the notion of relative derangements of type $B$, also called signed relative derangements, which are defined in terms of signed permutations, we obtain a type $B$ analogue of the well-known relation between relative derangements and the classical derangements. While this fact can be proved by using the principle of inclusion and exclusion, we present a combinatorial interpretation with the aid of the intermediate structure of signed skew derangements.
math.CO
by introducing the notion of relative derangements of type b also called signed relative derangements which are defined in terms of signed permutations we obtain a type b analogue of the wellknown relation between relative derangements and the classical derangements while this fact can be proved by using the principle of inclusion and exclusion we present a combinatorial interpretation with the aid of the intermediate structure of signed skew derangements
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708.3624
Collapse models with non-white noises
We set up a general formalism for models of spontaneous wave function collapse with dynamics represented by a stochastic differential equation driven by general Gaussian noises, not necessarily white in time. In particular, we show that the non-Schrodinger terms of the equation induce the collapse of the wave function to one of the common eigenstates of the collapsing operators, and that the collapse occurs with the correct quantum probabilities. We also develop a perturbation expansion of the solution of the equation with respect to the parameter which sets the strength of the collapse process; such an approximation allows one to compute the leading order terms for the deviations of the predictions of collapse models with respect to those of standard quantum mechanics. This analysis shows that to leading order, the ``imaginary'' noise trick can be used for non-white Gaussian noise.
quant-ph
we set up a general formalism for models of spontaneous wave function collapse with dynamics represented by a stochastic differential equation driven by general gaussian noises not necessarily white in time in particular we show that the nonschrodinger terms of the equation induce the collapse of the wave function to one of the common eigenstates of the collapsing operators and that the collapse occurs with the correct quantum probabilities we also develop a perturbation expansion of the solution of the equation with respect to the parameter which sets the strength of the collapse process such an approximation allows one to compute the leading order terms for the deviations of the predictions of collapse models with respect to those of standard quantum mechanics this analysis shows that to leading order the imaginary noise trick can be used for nonwhite gaussian noise
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708.3625
Spin matrix elements in 2D Ising model on the finite lattice
We present explicit formulas for all spin matrix elements in the 2D Ising model with the nearest neighbor interaction on the finite periodic square lattice. These expressions generalize the known results [Phys. Rev. D19, (1979), 2477--2479; hep-th/0107117; hep-th/0112167] (coincide with them in the appropriate limits) and fulfill the test of straightforward transfer matrix calculations for finite $N$.
nlin.SI cond-mat.stat-mech hep-th math-ph math.MP
we present explicit formulas for all spin matrix elements in the 2d ising model with the nearest neighbor interaction on the finite periodic square lattice these expressions generalize the known results phys rev d19 1979 24772479 hepth0107117 hepth0112167 coincide with them in the appropriate limits and fulfill the test of straightforward transfer matrix calculations for finite n
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708.3626
Total cross-section and rapidity gap survival probability at the LHC through an eikonal with soft gluon resummation
New results are presented for total ${\rm pp}/ {\rm \bar p p}$ cross-sections, in the framework of our QCD based model (GGPS). This is an improved eikonal mini-jet model, where soft gluon radiation tames the fast energy rise normally present in mini-jet models. We discuss the variability in our predictions and provide a handy parametrization of our results for the LHC. We find that our model predictions span the range $\sigma_{tot}^{LHC}=100 ^{+10}_{-13} mb$. While this matches nicely with the range of most other models, it does not agree with recent ones which include a "hard" Pomeron, even though our model does include hard scattering. We compute the survival probability for Large Rapidity Gap (LRG) events at the LHC and at the Tevatron. These events are relevant, for example, for Higgs signal in the $WW$ fusion process. We also explore whether measurements of the total cross-sections at the LHC can help us sharpen the model parameters and hence estimates for these survival probabilities, further.
hep-ph
new results are presented for total rm pp rm bar p p crosssections in the framework of our qcd based model ggps this is an improved eikonal minijet model where soft gluon radiation tames the fast energy rise normally present in minijet models we discuss the variability in our predictions and provide a handy parametrization of our results for the lhc we find that our model predictions span the range sigma_totlhc100 10_13 mb while this matches nicely with the range of most other models it does not agree with recent ones which include a hard pomeron even though our model does include hard scattering we compute the survival probability for large rapidity gap lrg events at the lhc and at the tevatron these events are relevant for example for higgs signal in the ww fusion process we also explore whether measurements of the total crosssections at the lhc can help us sharpen the model parameters and hence estimates for these survival probabilities further
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708.3627
Optimizing Replica Exchange Moves For Molecular Dynamics
In this short note we sketch the statistical physics framework of the replica exchange technique when applied to molecular dynamics simulations. In particular, we draw attention to generalized move sets that allow a variety of optimizations as well as new applications of the method.
q-bio.QM cond-mat.stat-mech physics.comp-ph q-bio.BM
in this short note we sketch the statistical physics framework of the replica exchange technique when applied to molecular dynamics simulations in particular we draw attention to generalized move sets that allow a variety of optimizations as well as new applications of the method
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708.3628
Recursive Structure and Bandwidth of Hales-Numbered Hypercube
The Hales numbered $n$-dimensional hypercube and the corresponding adjacency matrix exhibit interesting recursive structures in $n$. These structures lead to a very simple proof of the well-known bandwidth formula for hypercube, whose proof was thought to be surprisingly difficult. A related problem called hypercube antibandwidth, for which Harper proposed an algorithm, is also reexamined in the light of the above recursive structures, and a close form solution is found.
cs.DM
the hales numbered ndimensional hypercube and the corresponding adjacency matrix exhibit interesting recursive structures in n these structures lead to a very simple proof of the wellknown bandwidth formula for hypercube whose proof was thought to be surprisingly difficult a related problem called hypercube antibandwidth for which harper proposed an algorithm is also reexamined in the light of the above recursive structures and a close form solution is found
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708.3629
Boundary conditions in the QCD nucleus-nucleus scattering problem
In the framework of the effective field theory for interacting BFKL pomerons, applied to nucleus-nucleus scattering, boundary conditions for the classical field equations are discussed. Correspondence with the QCD diagrams at the boundary rapidities requires pomeron interaction with the participating nuclei to be exponential and non-local. Commonly used 'eikonal' boundary conditions, local and linear in fields, follow in the limit of small QCD pomeron-nucleon coupling. Numerical solution of the classical field equations, which sum all tree diagrams for central gold-gold scattering, demonstrates that corrected boundary conditions lead to substantially different results, as compared to the eikonal conditions studied in earlier publications. A breakdown of projectile-target symmetry for particular solutions discovered earlier in \cite{bom} is found to occur at roughly twice lower rapidity. Most important, due to a high non-linearity of the problem, the found asymmetric solutions are not unique but form a family growing in number with rapidity. The minimal value for the action turns out to be much lower than with the eikonal boundary conditions and saturates at rapidities around 10.
hep-ph hep-th
in the framework of the effective field theory for interacting bfkl pomerons applied to nucleusnucleus scattering boundary conditions for the classical field equations are discussed correspondence with the qcd diagrams at the boundary rapidities requires pomeron interaction with the participating nuclei to be exponential and nonlocal commonly used eikonal boundary conditions local and linear in fields follow in the limit of small qcd pomeronnucleon coupling numerical solution of the classical field equations which sum all tree diagrams for central goldgold scattering demonstrates that corrected boundary conditions lead to substantially different results as compared to the eikonal conditions studied in earlier publications a breakdown of projectiletarget symmetry for particular solutions discovered earlier in citebom is found to occur at roughly twice lower rapidity most important due to a high nonlinearity of the problem the found asymmetric solutions are not unique but form a family growing in number with rapidity the minimal value for the action turns out to be much lower than with the eikonal boundary conditions and saturates at rapidities around 10
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708.363
Floating Entanglement Witness Measure and Genetic Algorithm
In this paper based on the notion of entanglement witness, a new measure of entanglement called floating entanglement witness measure is introduced which satisfies some of the usual properties of a good entanglement measure. By exploiting genetic algorithm, we introduce a classical algorithm that computes floating entanglement witness measure. This algorithm also provides a method for finding entanglement witness for a given entangled state.
quant-ph
in this paper based on the notion of entanglement witness a new measure of entanglement called floating entanglement witness measure is introduced which satisfies some of the usual properties of a good entanglement measure by exploiting genetic algorithm we introduce a classical algorithm that computes floating entanglement witness measure this algorithm also provides a method for finding entanglement witness for a given entangled state
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708.3631
Prediction of Fractional Processes with Long-range Dependence
We introduce a class of Gaussian processes with stationary increments which exhibit long-range dependence. The class includes fractional Brownian motion with Hurst parameter H>1/2 as a typical example. We establish infinite and finite past prediction formulas for the processes in which the predictor coefficients are given explicitly in terms of the MA and AR coefficients.
math.PR
we introduce a class of gaussian processes with stationary increments which exhibit longrange dependence the class includes fractional brownian motion with hurst parameter h12 as a typical example we establish infinite and finite past prediction formulas for the processes in which the predictor coefficients are given explicitly in terms of the ma and ar coefficients
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708.3632
Akhet Khufu: archaeo-astronomical hints at a common project of the two main pyramids of Giza, Egypt
The architectural complexes composed by the two main pyramids of Giza together with their temples are investigated from an inter-disciplinary point of view, taking into account their astronomical alignments as well as their relationships with the visible landscape. Combining already known facts together with new clues, the work strongly supports the idea that the two complexes were conceived as parts of a common project.
physics.hist-ph
the architectural complexes composed by the two main pyramids of giza together with their temples are investigated from an interdisciplinary point of view taking into account their astronomical alignments as well as their relationships with the visible landscape combining already known facts together with new clues the work strongly supports the idea that the two complexes were conceived as parts of a common project
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708.3633
Quantum critical scaling behavior of deconfined spinons
We perform a renormalization group analysis of some important effective field theoretic models for deconfined spinons. We show that deconfined spinons are critical for an isotropic SU(N) Heisenberg antiferromagnet, if $N$ is large enough. We argue that nonperturbatively this result should persist down to N=2 and provide further evidence for the so called deconfined quantum criticality scenario. Deconfined spinons are also shown to be critical for the case describing a transition between quantum spin nematic and dimerized phases. On the other hand, the deconfined quantum criticality scenario is shown to fail for a class of easy-plane models. For the cases where deconfined quantum criticality occurs, we calculate the critical exponent $\eta$ for the decay of the two-spin correlation function to first-order in $\epsilon=4-d$. We also note the scaling relation $\eta=d+2(1-\phi/\nu)$ connecting the exponent $\eta$ for the decay to the correlation length exponent $\nu$ and the crossover exponent $\phi$.
cond-mat.str-el hep-th
we perform a renormalization group analysis of some important effective field theoretic models for deconfined spinons we show that deconfined spinons are critical for an isotropic sun heisenberg antiferromagnet if n is large enough we argue that nonperturbatively this result should persist down to n2 and provide further evidence for the so called deconfined quantum criticality scenario deconfined spinons are also shown to be critical for the case describing a transition between quantum spin nematic and dimerized phases on the other hand the deconfined quantum criticality scenario is shown to fail for a class of easyplane models for the cases where deconfined quantum criticality occurs we calculate the critical exponent eta for the decay of the twospin correlation function to firstorder in epsilon4d we also note the scaling relation etad21phinu connecting the exponent eta for the decay to the correlation length exponent nu and the crossover exponent phi
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708.3634
Time reflection and the dynamics of particles and antiparticles
In this paper we continue our analysis of a formulation of electrodynamics fully covariant under the full Poincar\'e group. Transformations under the four different components of the group force on us the introduction of particles, either in the identification by Feynman or in the identification of Dirac.
math-ph math.DG math.MP
in this paper we continue our analysis of a formulation of electrodynamics fully covariant under the full poincare group transformations under the four different components of the group force on us the introduction of particles either in the identification by feynman or in the identification of dirac
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708.3635
A Multivariate Training Technique with Event Reweighting
An event reweighting technique incorporated in multivariate training algorithm has been developed and tested using the Artificial Neural Networks (ANN) and Boosted Decision Trees (BDT). The event reweighting training are compared to that of the conventional equal event weighting based on the ANN and the BDT performance. The comparison is performed in the context of the physics analysis of the ATLAS experiment at the Large Hadron Collider (LHC), which will explore the fundamental nature of matter and the basic forces that shape our universe. We demonstrate that the event reweighting technique provides an unbiased method of multivariate training for event pattern recognition.
physics.data-an
an event reweighting technique incorporated in multivariate training algorithm has been developed and tested using the artificial neural networks ann and boosted decision trees bdt the event reweighting training are compared to that of the conventional equal event weighting based on the ann and the bdt performance the comparison is performed in the context of the physics analysis of the atlas experiment at the large hadron collider lhc which will explore the fundamental nature of matter and the basic forces that shape our universe we demonstrate that the event reweighting technique provides an unbiased method of multivariate training for event pattern recognition
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708.3636
Evidences for two scales in hadrons
Some unusual features observed in hadronic collisions at high energies can be understood assuming that gluons in hadrons are located within small spots occupying only about 10% of the hadron's area. Such a conjecture about the presence of two scales in hadrons helps to explain: why diffractive gluon radiation so much suppressed; why the triple-Pomeron coupling shows no t-dependence; why total hadronic cross sections rise with energy so slowly; why diffraction cone shrinks so slowly, and why $\alpha^\prime_P\ll\alpha^\prime_R$; why the transition from hard to soft regimes in the structure functions occurs at rather large $Q^2$; why the observed Cronin effect at collider energies is so weak; why hard reactions sensitive to primordial parton motion (direct photon, Drell-Yan dileptons, heavy flavors, back-to-back di-hadrons, seagull effect, etc.) demand such a large transverse momenta of the projectile partons, which is not explained by NLO calculations; why the onset of nuclear shadowing for gluons is so much delayed compared to quarks, and why shadowing is so weak.
hep-ph
some unusual features observed in hadronic collisions at high energies can be understood assuming that gluons in hadrons are located within small spots occupying only about 10 of the hadrons area such a conjecture about the presence of two scales in hadrons helps to explain why diffractive gluon radiation so much suppressed why the triplepomeron coupling shows no tdependence why total hadronic cross sections rise with energy so slowly why diffraction cone shrinks so slowly and why alphaprime_pllalphaprime_r why the transition from hard to soft regimes in the structure functions occurs at rather large q2 why the observed cronin effect at collider energies is so weak why hard reactions sensitive to primordial parton motion direct photon drellyan dileptons heavy flavors backtoback dihadrons seagull effect etc demand such a large transverse momenta of the projectile partons which is not explained by nlo calculations why the onset of nuclear shadowing for gluons is so much delayed compared to quarks and why shadowing is so weak
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708.3637
Geometry of Two-Qubit State and Intertwining Quaternionic Conformal Mapping Under Local Unitary Transformations
In this paper the geometry of two-qubit systems under local unitary group $SO(2)\otimes SU(2)$ is discussed. It is shown that the quaternionic conformal map intertwines between this local unitary subgroup of $Sp(2)$ and the quaternionic M\"{o}bius transformation which is rather a generalization of the results of Lee et al (2002 Quantum Inf. Process. 1 129).
quant-ph
in this paper the geometry of twoqubit systems under local unitary group so2otimes su2 is discussed it is shown that the quaternionic conformal map intertwines between this local unitary subgroup of sp2 and the quaternionic mobius transformation which is rather a generalization of the results of lee et al 2002 quantum inf process 1 129
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708.3638
Spin dynamics in a one-dimensional ferromagnetic Bose gas
We investigate the propagation of spin excitations in a one-dimensional (1D) ferromagnetic Bose gas. While the spectrum of longitudinal spin waves in this system is sound-like, the dispersion of transverse spin excitations is quadratic making a direct application of the Luttinger Liquid (LL) theory impossible. By using a combination of different analytic methods we derive the large time asymptotic behavior of the spin-spin dynamical correlation function for strong interparticle repulsion. The result has an unusual structure associated with a crossover from the regime of trapped spin wave to an open regime and does not have analogues in known low-energy universality classes of quantum 1D systems.
cond-mat.other
we investigate the propagation of spin excitations in a onedimensional 1d ferromagnetic bose gas while the spectrum of longitudinal spin waves in this system is soundlike the dispersion of transverse spin excitations is quadratic making a direct application of the luttinger liquid ll theory impossible by using a combination of different analytic methods we derive the large time asymptotic behavior of the spinspin dynamical correlation function for strong interparticle repulsion the result has an unusual structure associated with a crossover from the regime of trapped spin wave to an open regime and does not have analogues in known lowenergy universality classes of quantum 1d systems
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708.3639
Bimodality - a Sign of Critical Behavior in Nuclear Reactions
The recently discovered coexistence of multifragmentation and residue production for the same total transverse energy of light charged particles can be well reproduced in numerical simulations of the heavy ion reactions. A detailed analysis shows that fluctuations (introduced by elementary nucleon-nucleon collisions) determine which of the exit states is realized. Thus we observe for the first time nonlinear dynamics in heavy ion reactions. Also the scaling of the coexistence region with beam energy is well reproduced in these results from the QMD simulation program.
nucl-th
the recently discovered coexistence of multifragmentation and residue production for the same total transverse energy of light charged particles can be well reproduced in numerical simulations of the heavy ion reactions a detailed analysis shows that fluctuations introduced by elementary nucleonnucleon collisions determine which of the exit states is realized thus we observe for the first time nonlinear dynamics in heavy ion reactions also the scaling of the coexistence region with beam energy is well reproduced in these results from the qmd simulation program
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708.364
Two-integral distribution functions for axisymmetric systems
Some formulae are presented for finding two-integral distribution functions (DFs) which depends only on the two classical integrals of the energy and the magnitude of the angular momentum with respect to the axis of symmetry for stellar systems with known axisymmetric densities. They come from an combination of the ideas of Eddington and Fricke and they are also an extension of those shown by Jiang and Ossipkov for finding anisotropic DFs for spherical galaxies. The density of the system is required to be expressed as a sum of products of functions of the potential and of the radial coordinate. The solution corresponding to this type of density is in turn a sum of products of functions of the energy and of the magnitude of the angular momentum about the axis of symmetry. The product of the density and its radial velocity dispersion can be also expressed as a sum of products of functions of the potential and of the radial coordinate. It can be further known that the density multipied by its rotational velocity dispersion is equal to a sum of products of functions of the potential and of the radial coordinate minus the product of the density and the square of its mean rotational velocity. These formulae can be applied to the Binney and the Lynden-Bell models. An infinity of the odd DFs for the Binney model can be also found under the assumption of the laws of the rotational velocity.
math-ph astro-ph math.MP
some formulae are presented for finding twointegral distribution functions dfs which depends only on the two classical integrals of the energy and the magnitude of the angular momentum with respect to the axis of symmetry for stellar systems with known axisymmetric densities they come from an combination of the ideas of eddington and fricke and they are also an extension of those shown by jiang and ossipkov for finding anisotropic dfs for spherical galaxies the density of the system is required to be expressed as a sum of products of functions of the potential and of the radial coordinate the solution corresponding to this type of density is in turn a sum of products of functions of the energy and of the magnitude of the angular momentum about the axis of symmetry the product of the density and its radial velocity dispersion can be also expressed as a sum of products of functions of the potential and of the radial coordinate it can be further known that the density multipied by its rotational velocity dispersion is equal to a sum of products of functions of the potential and of the radial coordinate minus the product of the density and the square of its mean rotational velocity these formulae can be applied to the binney and the lyndenbell models an infinity of the odd dfs for the binney model can be also found under the assumption of the laws of the rotational velocity
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708.3641
Guerra's interpolation using Derrida-Ruelle cascades
New results about Poisson-Dirichlet point processes and Derrida-Ruelle cascades allow us to express Guerra's interpolation entirely in the language of Derrida-Ruelle cascades and to streamline Guerra's computations. Moreover, our approach clarifies the nature of the error terms along the interpolation.
math.PR math-ph math.MP
new results about poissondirichlet point processes and derridaruelle cascades allow us to express guerras interpolation entirely in the language of derridaruelle cascades and to streamline guerras computations moreover our approach clarifies the nature of the error terms along the interpolation
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708.3642
First Run II Measurement of the W Boson Mass
We describe a measurement of the W boson mass mW using 200/pb of root-s = 1.96 TeV p-pbar collision data taken with the CDF II detector. With a sample of 63,964 W -> e nu candidates and 51,128 W -> mu nu candidates, we measure mW = [80.413 +- 0.034 (stat) +- 0.034 (sys) = 80.413 +- 0.048] GeV/c^2. This is the single most precise mW measurement to date. When combined with other measured electroweak parameters, this result further constrains the properties of unobserved particles coupling to W and Z bosons.
hep-ex
we describe a measurement of the w boson mass mw using 200pb of roots 196 tev ppbar collision data taken with the cdf ii detector with a sample of 63964 w e nu candidates and 51128 w mu nu candidates we measure mw 80413 0034 stat 0034 sys 80413 0048 gevc2 this is the single most precise mw measurement to date when combined with other measured electroweak parameters this result further constrains the properties of unobserved particles coupling to w and z bosons
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708.3643
Correlation function of the two-dimensional Ising model on a finite lattice. II
We calculate the two-point correlation function and magnetic susceptibility in the anisotropic 2D Ising model on a lattice with one infinite and the other finite dimension, along which periodic boundary conditions are imposed. Using exact expressions for a part of lattice form factors, we propose the formulas for arbitrary spin matrix elements, thus providing a possibility to compute all multipoint correlation functions in the anisotropic Ising model on cylindrical and toroidal lattices. The scaling limit of the corresponding expressions is also analyzed.
nlin.SI cond-mat.stat-mech hep-th math-ph math.MP
we calculate the twopoint correlation function and magnetic susceptibility in the anisotropic 2d ising model on a lattice with one infinite and the other finite dimension along which periodic boundary conditions are imposed using exact expressions for a part of lattice form factors we propose the formulas for arbitrary spin matrix elements thus providing a possibility to compute all multipoint correlation functions in the anisotropic ising model on cylindrical and toroidal lattices the scaling limit of the corresponding expressions is also analyzed
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708.3644
Inflation from IIB Superstrings with Fluxes
We study the conditions needed to have an early epoch of inflationary expansion with a potential coming from IIB superstring theory with fluxes involving two moduli fields. The phenomenology of this potential is different from the usual hybrid inflation scenario and we analize the possibility that the system of field equations undergo a period of inflation in three different regimes with the dynamics modified by a Randall-Sundrum II term in the Friedmann equation. We find that the system can produce inflation and due to the modification of the dynamics, a period of accelerated contraction can follow or preceed this inflationary stage depending on the sign of one of the parameters of the potential. We discuss on the viability of this model in a cosmological context.
astro-ph
we study the conditions needed to have an early epoch of inflationary expansion with a potential coming from iib superstring theory with fluxes involving two moduli fields the phenomenology of this potential is different from the usual hybrid inflation scenario and we analize the possibility that the system of field equations undergo a period of inflation in three different regimes with the dynamics modified by a randallsundrum ii term in the friedmann equation we find that the system can produce inflation and due to the modification of the dynamics a period of accelerated contraction can follow or preceed this inflationary stage depending on the sign of one of the parameters of the potential we discuss on the viability of this model in a cosmological context
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708.3645
Why Tau First?
Electron neutrino has been the first neutral lepton to be foreseen and discovered last century. The un-ordered muon and its neutrino arose later by cosmic rays. The tau discover, the heaviest, the most unstable charged lepton, was found surprisingly on 1975. Its neutrino was hardly revealed just on 2000. So why High Energy Neutrino Astronomy should rise first via tau neutrino, the last, the most rare one? The reasons are based on a chain of three favorable coincidences found last decade: the neutrino masses and their flavor mixing, the UHECR opacity on Cosmic Black Body (GZK cut off on BBR), the amplified tau air-shower decaying in flight. Indeed guaranteed UHE GZK tau neutrinos, feed by muon mixing, while skimming the Earth might lead to boosted UHE tau, mostly horizontal ones. These UHE lepton decay in flight are spread, amplified, noise free Air-Shower: a huge event for an unique particle. To be observed soon: within Auger sky, in present decade. Its discover may sign of the first tau appearance.
astro-ph hep-ph
electron neutrino has been the first neutral lepton to be foreseen and discovered last century the unordered muon and its neutrino arose later by cosmic rays the tau discover the heaviest the most unstable charged lepton was found surprisingly on 1975 its neutrino was hardly revealed just on 2000 so why high energy neutrino astronomy should rise first via tau neutrino the last the most rare one the reasons are based on a chain of three favorable coincidences found last decade the neutrino masses and their flavor mixing the uhecr opacity on cosmic black body gzk cut off on bbr the amplified tau airshower decaying in flight indeed guaranteed uhe gzk tau neutrinos feed by muon mixing while skimming the earth might lead to boosted uhe tau mostly horizontal ones these uhe lepton decay in flight are spread amplified noise free airshower a huge event for an unique particle to be observed soon within auger sky in present decade its discover may sign of the first tau appearance
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708.3646
Complex solitons with power law behaviour in Bose-Einstein condensates near Feshbach resonance
Complex, localized stable solitons, characterized by a power law behaviour, are found for a quasi-one-dimensional Bose-Einstein condensate near Feshbach resonance. Both dark and bright solitons can be excited in the experimentally allowed parameter domain, when two and three-body interactions are respectively repulsive and attractive. These solutions are obtained for non-zero chemical potential, unlike their unstable real counterparts which exist in the limit of vanishing $\mu$. The dark solitons travel with constant speed, which is quite different from the Lieb mode, where profiles with different speeds, bounded above by sound velocity can exist for specified interaction strengths.
cond-mat.other
complex localized stable solitons characterized by a power law behaviour are found for a quasionedimensional boseeinstein condensate near feshbach resonance both dark and bright solitons can be excited in the experimentally allowed parameter domain when two and threebody interactions are respectively repulsive and attractive these solutions are obtained for nonzero chemical potential unlike their unstable real counterparts which exist in the limit of vanishing mu the dark solitons travel with constant speed which is quite different from the lieb mode where profiles with different speeds bounded above by sound velocity can exist for specified interaction strengths
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708.3647
Sub-Threshold Field Emission from Thin Silicon Membranes
We report on strongly enhanced electron multiplication in thin silicon membranes. The device is configured as a transmission-type membrane for electron multiplication. A sub-threshold electric field applied on the emission side of the membrane enhances the number of electrons emitted by two orders of magnitude. This enhancement stems from field emitted electrons stimulated by the incident particles, which suggests that stacks of silicon membranes can form ultra-sensitive electron multipliers.
cond-mat.mes-hall
we report on strongly enhanced electron multiplication in thin silicon membranes the device is configured as a transmissiontype membrane for electron multiplication a subthreshold electric field applied on the emission side of the membrane enhances the number of electrons emitted by two orders of magnitude this enhancement stems from field emitted electrons stimulated by the incident particles which suggests that stacks of silicon membranes can form ultrasensitive electron multipliers
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708.3648
Evidence of a Broad Relativistic Iron Line from the Neutron Star Low-Mass X-ray Binary Serpens X-1
We report on an analysis of XMM-Newton data from the neutron star low mass X-ray binary (LMXB) Serpens X-1 (Ser X-1). Spectral analysis of EPIC PN data indicates that the previously known broad iron K$\alpha$ emission line from this source has a significantly skewed structure with a moderately extended red wing. The asymmetric shape of the line is well described with the laor and diskline models in XSPEC and strongly supports an inner accretion disk origin of the line. To our knowledge this is the first strong evidence of a relativistic line in a neutron star LMXB. This finding suggests that the broad lines seen in other neutron star LMXBs likely originate from the inner disk as well. Detailed study of such lines opens up a new way to probe neutron star parameters and their strong gravitational fields. The red wing of the iron line from Ser X-1 is not as broad as that observed from some black hole systems. This is not unreasonable for a neutron star system, as the accretion disk has to terminate at or before the hard stellar surface. Finally, the inferred source inclination angle in the approximate range 40 degree to 60 degree is consistent with the lack of dips and eclipses from Ser X-1.
astro-ph
we report on an analysis of xmmnewton data from the neutron star low mass xray binary lmxb serpens x1 ser x1 spectral analysis of epic pn data indicates that the previously known broad iron kalpha emission line from this source has a significantly skewed structure with a moderately extended red wing the asymmetric shape of the line is well described with the laor and diskline models in xspec and strongly supports an inner accretion disk origin of the line to our knowledge this is the first strong evidence of a relativistic line in a neutron star lmxb this finding suggests that the broad lines seen in other neutron star lmxbs likely originate from the inner disk as well detailed study of such lines opens up a new way to probe neutron star parameters and their strong gravitational fields the red wing of the iron line from ser x1 is not as broad as that observed from some black hole systems this is not unreasonable for a neutron star system as the accretion disk has to terminate at or before the hard stellar surface finally the inferred source inclination angle in the approximate range 40 degree to 60 degree is consistent with the lack of dips and eclipses from ser x1
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