Exact solution of a 2d random Ising model

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第八届国际凝聚态理论与计算材料学会议

第八届国际凝聚态理论与计算材料学会议

大会将请专家对以下领域作专题性的特邀报告:
(1). 凝聚态物理的最新进展:
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D. 玻色-爱因斯坦凝聚
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J. 半导体物理
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structure Metallic Phases in Solid Germane (GeH4) under Pressure 锗烷在
压力下的金属相
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午餐
张振宇 橡树岭国家实验室
柳百新
清华大学
林海青 香港中文大学 牛谦 美国德克萨斯大学
7 月 16 日
凝聚态理论专题邀请报告 I 主持人:谢心澄 地点:芙蓉厅
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Manipulating Magnetization States of Nanostructures Two-spin decoherence in semiconductor quantum dots
稀磁半导体(Al,Cr)N 中的氮空位与高温铁磁性的第一原理研究
蒋青 刘邦贵
吉林大学 中科院物理所
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Theoretical and experimental studies of semiconductor dilute nitrides and devices

2007 JCP Finite difference spectral approximations for the timefractional

2007 JCP Finite difference spectral approximations for the timefractional

Finite difference/spectral approximations for the time-fractional diffusion equation qYumin Lin,Chuanju Xu*School of Mathematical Sciences,Xiamen University,361005Xiamen,ChinaReceived 9October 2006;received in revised form 18January 2007;accepted 2February 2007Available online 14February 2007AbstractIn this paper,we consider the numerical resolution of a time-fractional diffusion equation,which is obtained from the standard diffusion equation by replacing the first-order time derivative with a fractional derivative (of order a ,with 06a 61).The main purpose of this work is to construct and analyze stable and high order scheme to efficiently solve the time-fractional diffusion equation.The proposed method is based on a finite difference scheme in time and Legendre spectral methods in space.Stability and convergence of the method are rigourously established.We prove that the full dis-cretization is unconditionally stable,and the numerical solution converges to the exact one with order O ðD t 2Àa þN Àm Þ,where D t ;N and m are the time step size,polynomial degree,and regularity of the exact solution respectively.Numerical experiments are carried out to support the theoretical claims.Ó2007Elsevier Inc.All rights reserved.AMS Classification:65M12;65M06;65M70;35S10Keywords:Fractional diffusion equation;Spectral approximation;Stability;Convergence1.IntroductionThe use of fractional partial differential equations (FPDEs)in mathematical models has become increas-ingly popular in recent years.Different models using FPDEs have been proposed [4,14,16],and there has been significant interest in developing numerical schemes for their solution.Roughly speaking,FPDEs can be classified into two principal kinds:space-fractional differential equation and time-fractional one.One of the simplest examples of the former is fractional order diffusion equations,which are generalizations of classical diffusion equations,treating super-diffusive flow processes.Much of0021-9991/$-see front matter Ó2007Elsevier Inc.All rights reserved.doi:10.1016/j.jcp.2007.02.001qThis work was partially supported by National NSF of China under Grant 10531080,973High Performance Scientific Computation Research Program 2005CB321703,and Program of 985Innovation Engineering on Information in Xiamen University.*Corresponding author.Tel.:+865922580713;fax:+865922580608.E-mail address:cjxu@ (C.Xu).Journal of Computational Physics 225(2007)1533–1552/locate/jcpthe work published to date has been concerned with this kind of FPDEs(see e.g.[1,4–7,13,15,20]for a non-exhaustive list of references).In this paper,we consider the time-fractional diffusion equation(TFDE),obtained from the standard dif-fusion equation by replacing thefirst-order time derivative with a fractional derivative of order a,with 06a61.Time-fractional diffusion or wave equations are derived by considering continuous time random walk problems,which are in general non-Markovian processes.The physical interpretation of the fractional derivative is that it represents a degree of memory in the diffusing material[9].These models have been inves-tigated in analytical and numerical frames by a number of authors[8,11,18,19,21].Some of these authors have tried to construct analytical solutions to problems of time-fractional differential equations.For example, Schneider and Wyss[18]and Wyss[21]considered the time-fractional diffusion-wave equations.The corre-sponding Green functions and their properties are obtained in terms of Fox functions.Gorenflo et al.[8,9] used the similarity method and the method of Laplace transform to obtain the scale-invariant solution of TFDE in terms of the wright function.A similar construction of the solution to the time-fractional advec-tion–dispersion equations or TFDE in whole-space and half-space has been given in[10,11]by using the Fou-rier–Laplace transforms.However,published papers on the numerical solution of the TFDE equations are very sparse.Liu et al.[12] use afirst-orderfinite difference scheme in both time and space directions for this equation,where some sta-bility conditions are derived.Herein,we examine a practicalfinite difference/Legendre spectral method to solve the initial-boundary value time-fractional diffusion problem on afinite domain.An approach based on the backward differentiation combined with spatial collocation method is used to obtain estimates of (2-a)-order convergence in time and exponential convergence in space.It is also shown that the time-stepping scheme is unconditionally stable for all a2½0;1 .A series of numerical examples is presented and compared with the exact solutions to support the theoretical claims.Let us emphasize that the computation of the numerical solution of time-fractional differential equations has been generally limited to simple cases(low spatial dimension or small time integration)due to the‘‘glo-bal dependence’’ually,by the definition of the fractional derivative,the solution at a time t k depends on the solutions at all previous time levels t<t k.The fact that all previous solutions have to be saved to compute the solution at the current time level would make the storage very expensive if low-order methods are employed for spatial discretization.Contrarily,use of the spectral method can relax this stor-age limit because,as compared to a low-order method,the spectral method needs fewer grid points to pro-duce highly accurate solution.This is one of main advantages of the spectral method for FPDES.Another difficult point in solving TFDE lies in the discretization of the time-fractional derivative.The fact that the time-fractional derivative uses Caputo integral makes the standard schemes and corresponding numerical analysis not applicable.One of our main goals here is to propose an approach and provide an error analysis for this problem.The outline of the paper is as follows:first,we provide in Section2an analytical solution of the TFDE in a bounded domain.Second,afinite difference scheme for temporal discretization of this problem is pro-posed in Section3,where the stability and convergence analysis is given.A detailed error analysis is car-ried out for the semi-discrete problem,showing that the temporal accuracy is of(2-a)-order.In Section4, we construct a Legendre spectral collocation method for the spatial discretization of the TFDE.Error esti-mates are provided for the full discrete problem.Finally numerical experiments are presented in Section5 which support the theoretical error estimates.Some concluding remarks are given in thefinal section.2.Analytical solution of the TFDE in a bounded domainIn this section,wefirst describe the problem of fractional differential equation studied in this paper,and present some analytical solutions which will be found helpful in the comprehension of the nature of such a problem.Let L>0;T>0;K¼ð0;LÞ,consider the time-fractional diffusion equation of the formo a uðx;tÞo t a Ào2uðx;tÞo x2¼fðx;tÞ;x2K;0<t6Tð2:1Þ1534Y.Lin,C.Xu/Journal of Computational Physics225(2007)1533–1552subject to the following initial and boundary conditions:uðx;0Þ¼gðxÞ;x2K;ð2:2Þuð0;tÞ¼uðL;tÞ¼0;06t6T;ð2:3Þwhere a is the order of the time-fractional derivative.Here,we consider the case06a61.o a uðx;tÞo t a in(2.1)isdefined as the Caputo fractional derivatives of order a[16],given byo a uðx;tÞo t a ¼1Cð1ÀaÞZ to uðx;sÞo sd sðtÀsÞa;0<a<1:ð2:4ÞWhen a¼1,Eq.(2.1)is the classical diffusion equation:o uðx;tÞo t Ào2uðx;tÞo x2¼fðx;tÞ;x2K;0<t6T;ð2:5Þwhile the case a¼0corresponds to the classical Helmholtz elliptic equation.In fact the time derivative of inte-ger order in(2.5)can be obtained by taking the limit a!1in(2.4).In the case0<a<1,the definition of the Caputo fractional derivatives uses the information of the stan-dard derivatives at all previous time levels(non-Markovian process).If f 0,then by applying thefinite sine and Laplace transforms to(2.1),the analytical solution for the problem(2.1)–(2.3)can be obtained[1]asuðx;tÞ¼2LX1n¼0E aðÀa2n2t aÞsinðanxÞZ LgðrÞsinðanrÞd r;ð2:6Þwhere a¼p andE aðzÞ¼X1m¼0z mCða mþ1Þis the Mittag–Leffler function.We list here some special Mittag–Leffler-type functions having explicit expressions as follows:E1ðÀzÞ¼eÀz;E2ðzÞ¼coshðffiffizpÞ;E12ðzÞ¼X1m¼0z mC mþ1ÀÁ¼e z2erfcðÀzÞ;where erfc(z)is the error function complement defined byerfcðzÞ¼1ffiffiffip pZ1zeÀt2d t:Although expressed in a compact form,we note that using(2.6)to compute the exact solution is gen-erally difficult(especially for large time)due to slow convergence of the series E aðzÞfor a2ð0;1Þand big z.The exact solutions for a number of a are plotted in Fig.1,showing the smoothness of the solu-tions.The regularity of these solutions can be analyzed by using some properties of the Mittag–Leffler function[2].In the analysis of the numerical method that follows,we will assume that problem(2.1)–(2.3)has a unique and sufficiently smooth solution.3.Discretization in time:afinite difference schemeIn order to simplify the notations and without lose of generality,we consider the case f 0in the scheme construction and its numerical analysis.First,we introduce afinite difference approximation to discretize the time-fractional derivative.Lett k:¼k D t,k¼0;1;...;K,where D t:¼TK is the time step.To motivate the construction of the scheme,weuse the following formulation:for all06k6KÀ1,Y.Lin,C.Xu/Journal of Computational Physics225(2007)1533–15521535o a u ðx ;t k þ1Þo t a ¼1C ð1Àa ÞX k j ¼0Z t j þ1t j o u ðx ;s Þo s d sðt k þ1Às Þa¼1C ð1Àa ÞX k j ¼0u ðx ;t j þ1ÞÀu ðx ;t j ÞD t Z t j þ1t jd s ðt k þ1Às Þa þr k þ1D t ;ð3:1Þwhere r k þ1D t is the truncation error.It can be verified that the truncation error takes the following form:r k þ1D t6c u 1C ð1Àa ÞX k j ¼0Z t j þ1t j t j þ1þt j À2s ðt k þ1Às Þa d s þO ðD t 2Þ"#;ð3:2Þwhere c u is a constant depending only on u .For the first term in RHS of (3.2),we have1C ð1Àa ÞX k j ¼0Z t j þ1t j t j þ1þt j À2sðt k þ1Às Þa d s¼À1C ð1Àa ÞX k j ¼011Àa ð2j þ1ÞD t 2Àa½ðk Àj Þ1Àa Àðk þ1Àj Þ1Àa þ1C ð1Àa ÞX k j ¼021Àa D t 2Àa ½ðj þ1Þðk Àj Þ1Àa Àj ðk þ1Àj Þ1Àaþ1C ð1Àa ÞX k j ¼02ð1Àa Þð2Àa ÞD t 2Àa ½ðk Àj Þ2Àa Àðk þ1Àj Þ2Àa ¼D t 2Àa C ð2Àa Þðk þ1Þ1Àa þ2ðk 1Àaþðk À1Þ1Àa þðk À2Þ1Àa þÁÁÁþ11Àa Þh i À2D t 2ÀaC ð3Àa Þðk þ1Þ2Àa ¼D t 2Àa C ð2Àa Þðk þ1Þ1Àa þ2ðk 1Àa þðk À1Þ1Àa þðk À2Þ1Àa þÁÁÁþ11Àa ÞÀ22Àa ðk þ1Þ2Àa!:LetS ðk Þ¼ðk þ1Þ1Àaþ2ðk 1Àa þðk À1Þ1Àaþðk À2Þ1ÀaþÁÁÁþ11Àa ÞÀ22Àaðk þ1Þ2Àa:Incidentally,we find that j S ðk Þj is bounded for all a 2½0;1 and all k P 1,as proven in the following lemma.1536Y.Lin,C.Xu /Journal of Computational Physics 225(2007)1533–1552Lemma3.1.For all a2½0;1 and all K P1,it holdsj SðKÞj6c;where c is a constant independent of a;K.Proof.First,for a¼0,a direct calculation shows SðKÞ¼0for all K P1.Now we prove the lemma for a2ð0;1 .It can be verified thatSðKÞ¼ðKþ1Þ1Àaþ2ðK1ÀaþðKÀ1Þ1ÀaþðKÀ2Þ1ÀaþÁÁÁþ11ÀaÞÀ22ÀaðKþ1Þ2Àa¼X Kk¼0a k;wherea k¼ðkþ1Þ1Àaþk1ÀaÀ22Àaððkþ1Þ2ÀaÀk2ÀaÞ:This observation leads us to prove that the series P1k¼0a k converges.It is well known that the seriesP1k¼11k bconverges for all b>1.By consequence,it suffices to prove j a k j61k1þa for big enough k.In fact we have,for k P2,j a k j¼k1Àa1þ1 k1Àaþ1À2k2Àa1þ1k2ÀaÀ1!¼k1Àa1þ1þð1ÀaÞ1kþð1ÀaÞðÀaÞ2!1k2þð1ÀaÞðÀaÞðÀaÀ1Þ3!1k3þÁÁÁÀ2k2ÀaÀ1þ1þð2ÀaÞ1kþð2ÀaÞð1ÀaÞ2!1kþð2ÀaÞð1ÀaÞðÀaÞ3!1kþð2ÀaÞð1ÀaÞðÀaÞðÀaÀ1Þ4!1kþÁÁÁ¼k1Àa12!À23!ð1ÀaÞðÀaÞ1kþ13!À24!ð1ÀaÞðÀaÞðÀaÀ1Þ1kþÁÁÁ6k1Àa 13!ð1ÀaÞa1k21þ2ðaþ1Þ41kþ3ðaþ1Þðaþ2Þ201k2þÁÁÁ613!ð1ÀaÞa1k1þa1þ1kþ1k2þÁÁÁ623!ð1ÀaÞa1k1þa61k1þa:The proof is completed.hMore precise bound of SðkÞcan be obtained by numerical computations.Indeed our numerical tests show thatÀ16SðkÞ60806a61;k¼1;2;...,as observed in Fig.2,where evolution of SðkÞas a function of k for several typical values of a is plotted in the leftfigure,while limit of SðkÞas k tends to infinity as a function of a is shown in the rightfigure.Y.Lin,C.Xu/Journal of Computational Physics225(2007)1533–15521537Using Lemma3.1,and taking into account the fact that1Cð2ÀaÞ62for all a2½0;1 ,we have1Cð1ÀaÞX kj¼0Z t jþ1t jt jþ1þt jÀ2sðt kþ1ÀsÞad s62D t2Àa:As a result,it holdsr kþ1 D t K cuD t2Àa:ð3:3ÞOn the other side,a straightforward calculation of thefirst term in RHS of(3.1)gives1Cð1ÀaÞX kj¼0uðx;t jþ1ÞÀuðx;t jÞD tZ t jþ1t jd sðt kþ1ÀsÞa¼1Cð1ÀaÞX kj¼0uðx;t jþ1ÞÀuðx;t jÞD tZ t kþ1Àjt kÀjd tt a¼1Cð1ÀaÞX kj¼0uðx;t kþ1ÀjÞÀuðx;t kÀjÞD tZ t jþ1t jd tt¼1Cð2ÀaÞX kj¼0uðx;t kþ1ÀjÞÀuðx;t kÀjÞD t aðjþ1Þ1ÀaÀj1Àah i:For the sake of simplification,let us introduce the notations b j:¼ðjþ1Þ1ÀaÀj1Àa;j¼0;1;...;k,and define the discrete fractional differential operator L atbyL a t uðx;t kþ1Þ:¼1Cð2ÀaÞX kj¼0b juðx;t kþ1ÀjÞÀuðx;t kÀjÞD t a:Then(3.1)readso a uðx;t kþ1Þo t a ¼L atuðx;t kþ1Þþr kþ1D t:ð3:4ÞUsing L at uðx;t kþ1Þas an approximation of o a uðx;t kþ1Þaleads to the followingfinite difference scheme to(2.1):L a t u kþ1ðxÞ¼o2u kþ1ðxÞo x2;k¼0;1;...;KÀ1;ð3:5Þwhere u kþ1ðxÞis an approximation to uðx;t kþ1Þ.By virtue of(3.3),this scheme is formally of(2-a)-order accu-racy.A rigorous analysis of the convergence rate will be provided later for both semi-discrete and full-discrete cases,where we will prove that the temporal accuracy of the scheme(3.5)is globally of order2-a.Scheme(3.5)can be rewritten into,with simplification by omitting the dependence of u kþ1ðxÞon x:b0u kþ1ÀCð2ÀaÞD t a o2u kþ1o x2¼b0u kÀX kj¼1b j½u kþ1ÀjÀu kÀj ¼b0u kÀX kÀ1j¼0b jþ1u kÀjþX kj¼1b j u kÀj:ð3:6ÞIt is worthwhile to noting that the second term in the RHS of(3.6)automatically vanishes when k61,while the last two terms of(3.6)vanish when k¼0.It is direct to check thatb j>0;j¼0;1;...;k;1¼b0>b1>ÁÁÁ>b k;b k!0as k!1;X k j¼0ðb jÀb jþ1Þþb kþ1¼ð1Àb1ÞþX kÀ1j¼1ðb jÀb jþ1Þþb k¼1:ð3:7ÞLet us introduce the parameter a0:a0:¼Cð2ÀaÞD t a;and note that b0¼1,then by reformulating the right-hand side of(3.6),we obtain an equivalent form to scheme(3.5):1538Y.Lin,C.Xu/Journal of Computational Physics225(2007)1533–1552u kþ1Àa0o2u kþ1o x2¼ð1Àb1Þu kþX kÀ1j¼1ðb jÀb jþ1Þu kÀjþb k u0;k P1:ð3:8ÞHere again,when k¼1scheme(3.8)becomesu2Àa0o2u2o x2¼ð1Àb1Þu1þb1u0:For the special case k¼0,that is thefirst time step,the scheme simply readsu1Àa0o2u1o x2¼u0:ð3:9ÞEqs.(3.8)and(3.9),together with the boundary conditionsu kþ1ð0Þ¼u kþ1ðLÞ¼0;k P0;ð3:10Þand the initial conditionu0ðxÞ¼gðxÞ;x2Kð3:11Þform a complete set of the semi-discrete problem.It will be useful to define the error term r kþ1byr kþ1:¼a0o a uðx;t kþ1Þo t aÀL atuðx;t kþ1Þ!:ð3:12ÞThen we have from(3.3)and(3.4)j r kþ1j¼Cð2ÀaÞD t a j r kþ1D tj6c u D t2:ð3:13ÞTo introduce the variational formulation of the problem(3.8),we define some functional spaces endowed with standard norms and inner products that will be used hereafter.H1ðKÞ:¼v2L2ðKÞ;d vd x2L2ðKÞ&';H10ðKÞ:¼v2H1ðKÞ;v jo K¼0ÈÉ;H mðKÞ:¼v2L2ðKÞ;d k vk2L2ðKÞfor all positive integer k6m&';where L2ðKÞis the space of measurable functions whose square is Lebesgue integrable in K.The inner products of L2ðKÞand H1ðKÞare defined,respectively,byðu;vÞ¼ZK uv d x;ðu;vÞ1¼ðu;vÞþd ud x;d vd xand the corresponding norms byk v k0¼ðv;vÞ1=2;k v k1¼ðv;vÞ1=21:The norm kÁkmof the space H mðKÞis defined byk v km ¼X mk¼0d k vd x k2!1=2:In this paper,instead of using the above standard H1-norm,we prefer to define kÁk1byk v k1¼k v k2þa0d ud x2!1=2:ð3:14ÞY.Lin,C.Xu/Journal of Computational Physics225(2007)1533–15521539It is well known that the standard H1-norm and the norm defined by(3.14)are equivalent,the latter will be used in what follows.The variational(weak)formulation of the Eq.(3.8)subject to the boundary condition(3.10)reads:find u kþ12H1ðKÞ,such thatðu kþ1;vÞþa0o u kþ1o x;o vo x¼ð1Àb1Þðu k;vÞþX kÀ1j¼1ðb jÀb jþ1Þðu kÀj;vÞþb kðu0;vÞ;8v2H1ðKÞ:ð3:15ÞFor this weak semi-discretized problem,we have the following stability result.Theorem3.1.The semi-discretized problem(3.15)is unconditionally stable in the sense that for all D t>0,it holdsk u kþ1k16k u0k;k¼0;1;...;KÀ1:Proof.We will prove the result by induction.First when k¼0,we haveðu1;vÞþa0o u1o x;o vo x¼ðu0;vÞ8v2H1ðKÞ:Taking v¼u1and using the inequality k v k06k v k1and Schwarz inequality,we obtain immediatelyk u1k16k u0k:Suppose now we have provenk u j k16k u0k;j¼1;2;...;k;ð3:16Þwe want to prove k u kþ1k16k u0k.Taking v¼u kþ1in(3.15)givesðu kþ1;u kþ1Þþa0o u kþ1;o u kþ1¼ð1Àb1Þðu k;u kþ1ÞþX kÀ1j¼1ðb jÀb jþ1Þðu kÀj;u kþ1Þþb kðu0;u kþ1Þ:Hence,by using(3.16),we havek u kþ1k216ð1Àb1Þk u k kk u kþ1kþX kÀ1j¼1ðb jÀb jþ1Þk u kÀj kk u kþ1kþb k k u0kk u kþ1k6½ð1Àb1ÞþX kÀ1j¼1ðb jÀb jþ1Þþb k k u0kk u kþ1k1:Finally,the last equality of(3.7)yieldsk u kþ1k16k u0k:ÃNow we carry out an error analysis for the solution of the semi-discretized problem.We denote from now by c a generic constant which may not be the same at different occurrences.Theorem3.2.Let u be the exact solution of(2.1)–(2.3),f u k g K k¼0be the time-discrete solution of(3.15)with the initial condition u0ðxÞ¼uðx;0Þ,then we have the following error estimates:(1)when06a<1,k uðt kÞÀu k k16cu;aT a D t2Àa;k¼1;2;...;K;ð3:17Þwhere c u;a:¼c u=ð1ÀaÞ,with c u:constant defined in(3.3);(2)when a!1,k uðt kÞÀu k k16cuT D t;k¼1;2;...;K:ð3:18Þ1540Y.Lin,C.Xu/Journal of Computational Physics225(2007)1533–1552Proof.(1)First consider the case06a<1.We start by proving the following estimate:k uðt jÞÀu j k16cubÀ1jÀ1D t2;j¼1;2;...;K:ð3:19ÞAs in the proof of Theorem3.1,we will use the mathematical induction.Let e k¼u x;t kðÞÀu kðxÞ.For j¼1,we have,by combining(2.1),(3.9)and(3.12),the error equation:ð e1;vÞþa0o e1o x;o vo x¼ð e0;vÞþðr1;vÞ¼ðr1;vÞ8v2H1ðKÞ:Taking v¼ e1yieldsk e1k216k r1kk e1k:This,together with(3.13),givesk uðt1ÞÀu1k16cubÀ1D t2:Therefore,(3.19)is proven for the case j¼1.Suppose now(3.19)holds for all j¼1;2;...;k,we need then to prove that it holds also for j¼kþ1.By combining(2.1),(3.12)and(3.15),we derive,8v2H1ðKÞð e kþ1;vÞþa0o e kþ1o x;o vo x¼ð1Àb1Þð e k;vÞþX kÀ1j¼1ðb jÀb jþ1Þð e kÀj;vÞþb kð e0;vÞþðr kþ1;vÞ:ð3:20ÞLet v¼ e kþ1in(3.20),thenk e kþ1k216ð1Àb1Þk e k kk e kþ1kþX kÀ1j¼1ðb jÀb jþ1Þk e kÀj kk e kþ1kþb k k e0kk e kþ1kþk r kþ1kk e kþ1k:Dividing by k e kþ1k1at both sides,using the induction assumption and the fact that bÀ1jbÀ1jþ1<1for all non-negativeinteger j,we obtaink e kþ1k16ð1Àb1ÞbÀ1kÀ1þX kÀ1j¼1ðb jÀb jþ1ÞbÀ1kÀjÀ1"#c u D t2þc u D t26ð1Àb1ÞþX kÀ1j¼1ðb jÀb jþ1Þþb k"#c u bÀ1kD t2:Using(3.7)in the above inequality givesk e kþ1k16cubÀ1kD t2:The estimate(3.19)is proved.Now,by the definition of b k,a direct computation shows thatkÀa bÀ1kÀ1¼kÀak1ÀaÀðkÀ1Þ!11Àa;as k!1;and the function/ðxÞ:¼xÀax1ÀaÀðxÀ1Þ1Àais increasing on x for all x>1since/0ðxÞ¼1xðxÀ1Þa1À1À1xaÀax!P08x>1;06a61:This means kÀa bÀ1kÀ1increasingly tends to11Àaas1<k!1.Note that kÀa bÀ1kÀ1¼1when k¼1,hence we havekÀa bÀ1kÀ1611Àa;k¼1;2;...;K:ð3:21ÞConsequently we obtain,for all k such that k D t6T,Y.Lin,C.Xu/Journal of Computational Physics225(2007)1533–15521541k uðt kÞÀu k k16cubÀ1kÀ1D t2¼c u kÀa bÀ1kÀ1k a D t26c u11Àaðk D tÞa D t2Àa6c u;a T a D t2Àa:(2)Now we consider the case a!1.Note that in this case,the estimate(3.17)has no meaning since c u;a tends to infinity as a!1.Therefore,we need to look for an estimate of other form.Taking into account the fact j D t6T for all j¼1;2;...;K,we are led to establish:k uðt jÞÀu j k16cuj D t2;j¼1;2;...;K:ð3:22ÞOnce again,we derive this estimate by induction.(3.22)is obvious for j¼1.Suppose now(3.22)holds for j¼1;2;...;k,we want to prove that it remains true for j¼kþ1.A similar procedure as in case(1)leads tok e kþ1k16ð1Àb1Þk e k kþX kÀ1j¼1ðb jÀb jþ1Þk e kÀj kþb k k e0kþk r kþ1k6ð1Àb1Þ½c u k D t2 þX kÀ1j¼1ðb jÀb jþ1Þ½c uðkÀjÞD t2 þc u D t2¼ð1Àb1Þkkþ1þX kÀ1j¼1ðb jÀb jþ1ÞkÀjkþ1þ1kþ1"#c uðkþ1ÞD t2¼ð1Àb1ÞþX kÀ1j¼1ðb jÀb jþ1ÞÀð1Àb1Þ1kþ1ÀX kÀ1j¼1ðb jÀb jþ1Þjþ1kþ1þ1kþ1"#c uðkþ1ÞD t2:ð3:23ÞIt is observed thatð1Àb1Þ1kþ1þX kÀ1j¼1ðb jÀb jþ1Þjþ1kþ1þb k P1kþ1ð1Àb1ÞþX kÀ1j¼1ðb jÀb jþ1Þþb k"#¼1kþ1;which is equivalent toÀð1Àb1Þ1kþ1ÀX kÀ1j¼1ðb jÀb jþ1Þjþ1kþ1þ1kþ16bk:Bringing this inequality into(3.23)givesk e kþ1k16ð1Àb1ÞþX kÀ1j¼1ðb jÀb jþ1Þþb k"#c uðkþ1ÞD t2¼c uðkþ1ÞD t2:Hence(3.22)is proven,i.e.(3.18)holds.The proof is completed.h4.Full discretization4.1.A Galerkin spectral method in spaceTo simplify the notations,we let K¼ðÀ1;1Þhereafter.The Galerkin spectral discretization proceeds by approximating the solution by the polynomials of high degree.To this end,we define P NðKÞthe space ofall polynomials of degree6N with respect to x.Then the discrete space,denoted by P0N ðKÞ,is defined as fol-lows:P0N ðKÞ:¼H1ðKÞ\P NðKÞ.Now consider the spectral discretization to the problem(3.15)as follows:find u kþ1N 2P0NðKÞ,such that forall v N2P0NðKÞðu kþ1N ;v NÞþa0oo xu kþ1N;oo xv N¼ð1Àb1Þðu kN;v NÞþX kÀ1j¼1ðb jÀb jþ1Þðu kÀj N;v NÞþb kðu0N;v NÞ:ð4:1ÞFor f u jN g kj¼0given,the well-posedness of the problem(4.1)is guaranteed by the well-known Lax–MilgramLemma.We are interested in this section in deriving an error estimate for the full-discrete solution f u kN g K k¼0.1542Y.Lin,C.Xu/Journal of Computational Physics225(2007)1533–1552。

Exact solution of the one-dimensional ballistic aggregation

Exact solution of the one-dimensional ballistic aggregation

a r X i v :c o n d -m a t /9808077v 1 7 A u g 1998Exact solution of the one-dimensional ballistic aggregationL.FrachebourgInstitut de Physique Th´e orique Ecole Polytechnique F´e d´e rale de LausanneCH-1015Lausanne,SwitzerlandAbstractAn exact expression for the mass distribution ρ(M,t )of the ballistic ag-gregation model in one dimension is derived in the long time regime.It is shown that it obeys scaling ρ(M,t )=t −4/3F (M/t 2/3)with a scaling function F (z )∼z −1/2for z ≪1and F (z )∼exp(−z 3/12)for z ≫1.Relevance of these results to Burgers turbulence is discussed.Ballistic aggregation provides a simple model of nonequilibrium statistical physics which is a natural version of a dissipative gas of hard spheres where particles follow the basic laws of mechanics.It consists in a one-dimensional gas of point-like massive particles which move freely until they collide.The perfectly inelastic collision of two masses conserves the total mass and momentum,while dissipation occurs as kinetic energy is loss in each collision.One can anticipate the formation of more and more massive while slower and slower aggregates.This model was introduced by Carnevale,Pomeau and Young [1]where they conjectured,based on scaling arguments and numerical simulations,an asymptotic scaling regime for the mass distribution ρ(M,t )=F (M/ M t )/ M 2t .The average mass per aggregate was supposed to grow algebraically with time as M t ∼t 2/3and the scaling function had a simple universal exponential form F (z )=exp(−z )independent of the initial ter,this conjecture was reinforced by Piasecki [2]where he solved the hierarchy of dynamicalequations governing the system inside a mean-field approximation scheme.This system,in its continuous limit,was also studied as a simplified astronomical model for the agglomeration of cosmic dust into macroscopic objects[3].In the ballistic aggregation model,the aggregates interact only through their collisions.An aggregation model where gravitational interactions are present has been studied in[4].It is important to mention the connection between this model and some solutions of the Burgers equation.At very high Reynolds number,the asymptotic solution of the Burgers equation consists of a train of shock waves.The laws of motion which govern the dynamics of these shock waves are found to be equivalent to a ballistic aggregation system(see[5]).In this letter,I verify the scaling hypothesis for the mass distribution andfind in an exact calculation an explicit form for the scaling function.It happens to be different from the conjectured simple exponential.Rather than solving the set of partial differential equations governing the evolution of the system,I exploit the fact that,once the initial state of the system is given,the dynamics is completely deterministic.Our approach will thus be based on a statistical study of the initial conditions and is largely inspired by the work of Martin and Piasecki[6].Initially,particles having all the same mass m are regularly placed on a line with the same inter-particle distance a.Initial mass density is thusρ0=m/a.The initial momentum of the thermalized particles are not correlated and are distributed according to the same Gaussian distributionφ(p)=can be determined from the initial state.I label the location of the CM at time t of the r particles located initially at(j+1)a,(j+2)a,...,(j+r)a byX r j+1(t):=12a+tt1/3ρm′(M′,P′)(3) with M′=M/t2/3,P′=P/t1/3and m′=m/t2/3.Note that,due to translational invariance, the mass distribution does not depend on X.Owing to the uncorrelated initial Gaussian distribution of the momentum,one can com-pute the densityρusing an analogy with a Brownian motion in the momentum space under particular constraints[6,7],(see Fig.(1)).Onefindsρm′(M′,P′)=J m′ −M′−P′M′ (4) where J m′(Z)is the probability for a Brownian motion P(τ)to start from P(0)=0and pass above the discrete points P(rm′)>Zrm′−(rm′)2(r≥1),and I m′(M′,P′)is the probability for a Brownian motion to start at P(0)=0,end at P(M′)=P′and over-passing the discrete points P(rm′)>(M′+P′/M′)rm′−(rm′)2(1≥r≥n).FIGURESFIG.1.The Brownian motion used in the construction of our solution.I will derive below an expression for the mass distribution in the limit m′=m/t2/3→0 which is reached either when t→∞for afixed m(asymptotic long time limit)or for any fixed time t when m→0(continuous limit).In this limit,one keeps M′and P′of order O(1).In terms of the Brownian motion introduced above,the space m′between the discrete points barrier shrinks to zero and approaches a continuous barrier which makes the problem tractable analytically.Nevertheless,the functions I and J are identically null for m′=0. One should thus keeps track of thefirst space m′(the Brownian motion will be unrestricted up to thefirst point of the barrier)and willfind a mass distribution which is an expansion in power of m′.From now on,I drop the subscript′and setρ0=1/2without loss of generality.Onefinds the dominant contribution in m:¯Im(M,P)=e−P2πe−P2∂P1∂P2K M(m,P1,M−m,P2) P1=P2=0+O(m2)(5)and¯Jm(Y)= ∞Y m−m2dP1φ(P1)lim N→∞ ∞Y Nm−(Nm)2dP2K Y(P1,m,P2,Nm) = πlim N→∞ ∞Y Nm−(Nm)2dP2∂2(Q1f′(τ1)−Q2f′(τ2)−1∂τ2−∂22f′′(τ2) G(Q1,τ1,Q2,τ2)=0(8)with G(Q1,τ,Q2,τ)=δ(Q1−Q2)and G(0,τ1,Q2,τ2)=G(Q1,τ1,0,τ2)=0.In our problem f′′(τ)=2.The equation(8)can be solved(see[7]for details)and onefindsG(Q1,τ1,Q2,τ2)= k≥1e−ωk(τ2−τ1)Ai(Q1−ωk)Ai(Q2−ωk)πe−M3/12I(M)+O(m2)(10) withI(M)= k≥1e−ωk M.(11) In the same way,I use Eqs.(6,7,9)and obtain¯Jm(Y)= πlim M→∞e(Y/2−M)3/3−(Y/2)3/3 ∞0dx e−x(Y/2−M) k≥1e−ωk M Ai(x−ωk)Using the integral representation of the sum in(12)[9],k≥1e−ωk M Ai(x−ωk)Ai(z)(13) with c>−ω1,one can exchange the integration andfind after a tedious analytical calculation[7]¯Jm(Y)= πe−(Y/2)3/3J(Y)+O(m3/2)(14) withJ(Y)=1Ai(z)(15) where c>−ω1.Now,inserting the expression for I and J in Eq.(4),one has in the original variablesρ(M,P;t)=m2t2/3 J−M M J −M M +≀ m2P2 t∼t1/3,E(t)∼t−2/3.(17)A careful integration over P[7]leads to the mass distribution,which is the main result of this letter,ρ(M,t)=1t2/3 +≀m2π2M′I(M′)H(M′)(19)whereI(M′)= k≥1e−ωk M′,H(M′)=1Ai2(z)(20)with c >−ω1.The scaling function F (M ′)is plotted on Fig.2.0.0 1.02.03.04.0M/t2/30.000.050.100.150.20t 4/3ρ(M /t 2/3)FIG.2.The rescaled mass distribution t 4/3ρ(M,t )as a function of M/t 2/3.One can compare the obtained scaling function with the conjectured one (F conj .(M ′)=exp(−M ′))[1].In particular small and large arguments present strong differences.Indeed,for M ′≪1,one get H (M ′)=1+O (M ′)while one can estimate I (M ′)using the asymptotic properties of the zeroes of the Airy function ωk =[(3πk )/2]2/3+O (k −1/3)and find I (M ′)∼(2√π5/21M′+O (√of small masses M <M 0≪t 2/3at time t is well underestimated by the conjectured formwhich leads to N (M 0,t )∼M 0/t ,while the exact solution gives N (M 0,t )∼√πM ′3/2exp(−M ′3/12).On the other end,one has I (M ′)∼exp(−ω1z )andfinallyF (M ′)=2M 1−P 2M 1−P 2M ′1−M ′1I m ′(M ′1,P ′1)I m ′(M ′2,P ′2)J m ′P ′2tπ3FM 1t 2/3(24)withF (M ′1,M ′2)=(M ′1+M ′2)M ′1M ′2I (M ′1)I (M ′2)H (M ′1+M ′2)(25)and I and H as above.This collision frequency clearly does not factorize in a product of functions of M 1and M 2,respectively.This fact invalidates the assumption on which the mass distribution was computed in[2].One can inquire about the universality of these results with respect to other initial conditions.Let usfirst consider a Poissonian distribution of the particles initial positions with an average interparticle distance a.The discrete points over which the Brownian motion should pass in the construction of our solution are still distributed on the same parabola but with irregular spacing.In the long time limit and after rescaling,the spacing between points of average a′=a/t2/3become smaller and smaller up to be,infirst order in m′, a continuum.The difference between irregular and regular spacing is thus asymptotically erased and the result Eq.(18)should be recovered in this case.A bimodal momentum distributionφ(p)=(δ(p−p0)+δ(p+p0))/2is used in the initial state in[1].I believe that this should not affect the form of the mass distribution(18)as the random walk initiated by this distribution is well approximated,in the long time limit, by the considered Brownian motion.One can define a distribution where momentum are initially correlated.In this case,one expects the scaling function to be different,at least for small M′[12].In summary,I found an exact asymptotic solution for the mass distribution of the ballistic aggregation in one dimension.Such an exact solution is not frequent in a nonequilibrium system and has permitted to verify scaling hypothesis for this system.While the average mass per aggregate was proved to behave with time as M t∼t2/3for t≫1,as expected from previous studies,the scaling function is shown here to be different from the conjectured one.This distribution also solve the shock strength distribution of the one dimensional Burgers equation in the inviscid limit with a white noise initial condition.I gratefully acknowledge numerous useful discussions with P.Martin and J.Piasecki and financial support from the Swiss National Foundation.REFERENCES[1]G.F.Carnevale,Y.Pomeau and W.R.Young,Phys.Rev.Lett.64,2913(1990).[2]J.Piasecki,Physica A190,90(1992).[3]S.F.Shandarin and Ya.B.Zeldovich,Rev.Mod.Phys.61,185(1989).[4]P.A.Martin and J.Piasecki,J.Stat.Phys.84,837(1996).[5]J.M.Burgers,The nonlinear diffusion equation,Reidel,Dordrecht(1974).[6]P.A.Martin and J.Piasecki,J.Stat.Phys.76,447(1994).[7]L.Frachebourg,P.A.Martin and J.Piasecki,in preparation.[8]M.Abramowitz and I.A.Stegun,Handbook of Mathematical Functions,Dover,New-York(1965).[9]P.Groeneboom,Probab.Th.Rel.Fields81,79(1989).[10]M.Avellaneda and W.E,Comm.Math.Phys.172,13(1995);M.Avellaneda,Comm.Math.Phys.169,45(1995).[11]S.Kida,J.Fluid Mech.93,337(1979).[12]Ya.G.Sinai,Comm.Math.Phys.148,601(1992);Z.-S.She,E.Aurell and U.Frisch,Comm.Math.Phys.148,623(1992).11。

fa-yuehwu–curriculumvitae:伍法岳–简历

fa-yuehwu–curriculumvitae:伍法岳–简历

Fa-Yueh Wu—Curriculum vitaeFa-Yueh Wu was born January1932in China.He moved to Taiwan in1949where he received a B.S.degree in Electrical Engineering from the Chinese Naval College of Technology in1954and,after serving the Navy for three years from1954to1957, a M.S.degree in physics from the National Tsing Hua University in1959.The same year,he entered Washington University in St.Louis as a physics graduate student, where he studied under the late Eugene Feenberg,working on many-body theory, a topic to which he has continued to make important contributions throughout the years. After obtaining his Ph.D.in physics in1963,he continued at Washington University as a postdoc for9months and was appointed an Assistant Professor at the Virginia Polytechnic Institute in the same year.In1967he moved to Northeastern University in Boston where he has remained until the present.Promoted to Professor in1976,he was named a University Distinguished Professor in1989and the Matthews University Distinguished Professor of Physics in1992.Professor Wu’s works in many-body theory,particularly those related to the the-ory of liquid He4and He3and the formulation of the correlated-basis wave function approach,have been in uential for years.In the late1960s,he began working in sta-tistical mechanics with a special interest in exact solutions of lattice models of phase transitions and critical phenomena.He has over200papers published in refereed scien-tiÿc journals and has authored a number of important review articles and monographs. Professor Wu’s1982review on the Potts model is a classic which has over the years drawn over1000citations.Another classic among his works is his1968joint paper with E.H.Lieb on the exact solution of the ground state of the one-dimensional Hub-bard model,a fundamental paper on strongly correlated electron systems which has drawn over1400citations.A full account of the Lieb–Wu solution is now published for theÿrst time in this Proceedings,possibly establishing a record34years time span between the publication of a Letter and the full report of a seminal research. Professor Wu has solved numerous lattice models of phase transitions.These in-clude lattice models in three dimensions and dimer models having di erent geometry and topology.He has also contributed signiÿcantly to the study of the role played by integrable models in the mathematical theory of knots and knot invariants and has written a comprehensive review on the subject.Likewise,he has made deÿnitive con-tributions in graph theory and combinatorics which clarify and elucidate the interplay of combinatorics in statistical physics.A Fellow of the American Physical Society since1972,Professor Wu served as the Program Director for the Condensed Matter Theory Program at the National Science Foundation from1983to1984.In this capacity he helped maintain the quality and viability of the Program at a time of declining funding growth.Within the scientiÿc community he has served as the editor of several physics journals,given many invited talks and organized a number of international conferences.doi:10.1016/S0378-4371(02)01801-0xvi Curriculum vitaeProfessor Wu has visited numerous universities and institutions worldwide.He was a1973Fulbright–Hays Senior Research Scholar.He has been a Visiting Professor at the Australian National University(1973,1990,1995),the University of Amsterdam (1994),the Institute-Lorentz(1980),the University of Delft(1980),the Institute of Nuclear Energy(KFA)at J u lich(1981),the University of Paris VI(1991,1996),the National Taiwan University(1984),the National Tsing Hua University(1974,1988, 1999),the Brazilian Center of Theoretical Physics(1985),the Institute of Physics of Academia Sinica,Beijing(1979),the Institute of Physics of Academia Sinica,Taipei (1990),the University of Washington(1987),and theÃEcole Polytechnique FÃe derale of Lausanne(1975,1978,1985,1988,1991).He has also been the Invited Distinguished Chair Professor of the National Science Council,Taipei(1991).He is a Guest Professor at Nankai University in Tianjin,and an Honorary Professor at the Southwest University in Chongqing and at Beijing Normal University.He is named the Outstanding Alumnus of the National Tsing Hua University in2003.Selected Publications of Fa Yueh Wu—Papers with9or more citations based on database of Science Citation Index Expanded(ISI Web of Science)in early November 2002.[1]E.Lieb,F.Y.Wu,Absence of Mott transition in an exact solution of the short-rangeone-band model in one dimension,Phys.Rev.Lett.20(1968)1445–1448,1422 citations.[2]F.Y.Wu,The Potts model,Rev.Mod.Phys.54(1982)235–268,1096citations.[3]C.Fan,F.Y.Wu,General lattice model of phase transitions,Phys.Rev.B2(1970)723–733,222citations.[4]R.J.Baxter,F.Y.Wu,Exact solution of an Ising model with three-spin interactionson a triangular lattice,Phys.Rev.Lett.31(1973)1294–1297,161citations. [5]F.Y.Wu,Ising model with four-spin interactions,Phys.Rev.B4(1971)2312–2314,135citations.[6]R.J.Baxter,S.B.Kelland,F.Y.Wu,Equivalence of the Potts model or Whit-ney polynomial with the ice-type model:a new derivation,J.Phys.A9(1976) 397–406,123citations.[7]C.Fan,F.Y.Wu,Ising model with next-neighbor interactions:some exact resultsand an approximate solution,Phys.Rev.179(1969)560–570,112citations. [8]F.Y.Wu,E.Feenberg,Theory of Fermi liquids,Phys.Rev.128(1962)943–955,106citations.[9]R.J.Baxter,F.Y.Wu,Ising model on a triangular lattice with three-spin in-teractions:I.The eigenvalue equations,Aust.J.Phys.27(1974)357–367,92 citations.[10]F.Y.Wu,Y.K.Wang,Duality transformation in a many component spin model,J.Math.Phys.17(1976)439–440,88citations.[11]F.Y.Wu,Percolation and the Potts model,J.Stat.Phys.18(1978)115–123,63citations.[12]A.Hinterman,H.Kunz,F.Y.Wu,Exact results for the Potts model in two di-mensions,J.Stat.Phys.19(1978)623–632,63citations.Curriculum vitae xvii [13]F.Y.Wu,K.Y.Lin,Two phase transitions in the Ashkin–Teller model,J.Phys.C7(1974)L181–L184,60citations.[14]F.Y.Wu,E.Feenberg,Ground state of liquid helium(Mass4),Phys.Rev.122(1961)739–742,57citations.[15]F.Y.Wu,Remarks on the modiÿed KDP model,Phys.Rev.168(1968)539–543,52citations.[16]D.H.Lee,R.G.Ca ish,J.D.Joannopoulos,F.Y.Wu,Antiferromagnetic classicalXY-model:a mean-ÿeld analysis,Phys.Rev.B29(1984)2680–2684, 44citations.[17]F.Y.Wu,Exactly soluble model of ferroelectric phase transition in two dimen-sions,Phys.Rev.Lett.18(1967)605–607,43citations.[18]F.Y.Wu,Potts model of ferromagnetism,J.Appl.Phys.55(1984)2421–2425,39citations.[19]F.Y.Wu,Knot theory and statistical mechanics,Rev.Mod.Phys.64(1992)1099–1131,39citations.[20]C.N.Chen,C.K.Hu,F.Y.Wu,Partition function zeroes of the square lattice Pottsmodel,Phys.Rev.Lett.76(1996)169–172,37citations.[21]G.Keiser,F.Y.Wu,Electron gas at metallic densities,Phys.Rev.A6(1972)2369–1377,33citations.[22]F.Y.Wu,On the Horiguchi’s solution of the Blume–Emery–Gri ths model,Phys.Lett.A116(1986)245–247,33citations.[23]F.Y.Wu,Eight-vertex model on the honeycomb lattice,J.Math.Phys.6(1974)687–691,32citations.[24]Y.K.Wang,F.Y.Wu,Multi-component spin model on the Cayley tree,J.Phys.A9(1976)593–604,31citations.[25]F.Y.Wu,M.K.Chien,Convolution approximation for the n-particle distributionfunction,J.Math.Phys.11(1970)1912–1916,30citations.[26]I.G.Enting,F.Y.Wu,Triangular lattice Potts model,J.Stat.Phys.28(1982)351–378,30citations.[27]K.Y.Lin,F.Y.Wu,Phase diagram of the antiferromagnetic triangular Ising modelwith anisotropic interactions,Z.Phys.B33(1979)181–185,29citations. [28]F.Y.Wu,Critical point of planar Potts models,J.Phys.C12(1979)645–649,28citations.[29]F.Y.Wu,Exact solution of a model of an antiferroelectric transition,Phys.Rev.183(1969)604–607,27citations.[30]C.S.Hsue,K.Y.Lin,F.Y.Wu,Staggered eight-vertex model,Phys.Rev.B12(1975)429–437,27citations.[31]F.Y.Wu,K.Y.Lin,Staggered ice-rule model—the Pfa an solution,Phys.Rev.B12(1975)419–428,25citations.[32]H.Kunz,F.Y.Wu,Site percolation as a Potts model,J.Phys.C11(1978)L1–L4,25citations.[33]F.Y.Wu,Cluster development in an N-body problem,J.Math.Phys.4(1963)1438–1443,24citations.[34]J.E.Sacco,F.Y.Wu,Thirty-two vertex model on a triangular lattice,J.Phys.A8(1975)1780–1787,24citations.[35]X.N.Wu,F.Y.Wu,The Blume–Emery–Gri ths model on the honeycomb lattice,J.Stat.Phys.50(1988)41–55,24citations.xviii Curriculum vitae[36]F.Y.Wu,G.Rollet,H.Y.Huang,J.-M.Maillard,C.K.Hu,C.N.Chen,Directedcompact lattice animals,restricted partitions of numbers,and the inÿnite-state Potts model,Phys.Rev.Lett.76(1996)173–176,24citations.[37]J.H.H.Perk,F.Y.Wu,Non-intersecting string model and graphical approach:equivalence with a Potts model,J.Stat.Phys.42(1986)727–742,22 citations.[38]F.Y.Wu,X.N.Wu,H.W.J.Bl o te,Critical frontier of the antiferromagnetic Isingmodel in a nonzero magneticÿeld:the honeycomb lattice,Phys.Rev.Lett.62 (1989)2273–2276,22citations.[39]F.Y.Wu,Exact results for a dilute Potts model,J.Stat.Phys.23(1980)773–782,21citations.[40]H.K.Sim,R.Tao,F.Y.Wu,Ground-state energy of charged quantum liquids intwo dimensions,Phys.Rev.B34(1986)7123–7128,21citations.[41]W.Kinzel,W.Selke,F.Y.Wu,A Potts model with inÿnitely degenerate groundstate,J.Phys.A14(1981)L399–L404,19citations.[42]G.O.Zimmerman,A.K.Ibrahim,F.Y.Wu,A planar classical dipolar system ona honeycomb lattice,Phys.Rev.B37(1988)2059–2065,19citations.[43]Y.Chow,F.Y.Wu,Residual entropy and validity of the third law of thermody-namics in discrete spin systems,Phys.Rev.B36(1987)285–288,18citations.[44]F.Y.Wu,Multiple density correlations in a many particle system,J.Math.Phys.12(1971)1923–1929,17citations.[45]F.Y.Wu,Ashkin–Teller model as a vertex problem,J.Math.Phys.18(1977)611–613,17citations.[46]R.K.P.Zia,F.Y.Wu,Critical point of the triangular Potts model with two-andthree-site interactions,J.Phys.A14(1981)721–727,17citations.[47]F.Y.Wu,Dilute Potts model,duality and site-bond percolation,J.Phys.A14(1981)L39–L44,17citations.[48]X.N.Wu,F.Y.Wu,Exact results for lattice models with pair and triplet interac-tions,J.Phys.A22(1989)L1031–L1035,17citations.[49]F.Y.Wu,Exact results on a general lattice statistical model,Solid State Commun.10(1972)115–117,16citations.[50]F.Y.Wu,H.E.Stanley,Domany–Kinzel model of directed percolation:formula-tion as a random-walk problem and some exact results,Phys.Rev.Lett.48(1982) 775–777,16citations.[51]J.H.H.Perk,F.Y.Wu,Graphical approach to the non-intersecting string model:star-triangle equation,inversion relation and exact solution,Physica A138(1986) 100–124,16citations.[52]F.Y.Wu,K.Y.Lin,Ising model on the Union Jack lattice as a free-Fermionmodel,J.Phys.A20(1987)5737–5740,16citations.[53]X.N.Wu,F.Y.Wu,Duality properties of a general vertex model,J.Phys.A22(1989)L55–L60,16citations.[54]F.Y.Wu,Critical behavior of two-dimensional hydrogen-bonded antiferroelectrics,Phys.Rev.Lett.22(1967)1174–1176,14citations.[55]F.Y.Wu,Number of spanning trees on a lattice,J.Phys.A10(1977)L113–L115,14citations.[56]J.R.Banavar,F.Y.Wu,Antiferromagnetic Potts model with competing interac-tions,Phys.Rev.B29(1984)1511–1513,13citations.Curriculum vitae xix [57]F.Y.Wu,Exact solution of a triangular Ising model in a nonzero magneticÿeld,J.Stat.Phys.40(1985)613–620,12citations.[58]F.Y.Wu,Spontaneous magnetization of the three-spin Ising model on the UnionJack lattice,J.Phys.C8(1975)2262–2266,11citations.[59]F.Y.Wu,Solution of an Ising model with two-and four-spin interactions,Phys.Lett.A38(1972)77–78,11citations.[60]F.Y.Wu,Two-dimensional Ising model with crossing and four-spin interactionsand a magneticÿeld i kT=2,J.Stat.Phys.44(1986)455–463,11citations. [61]F.Y.Wu,H.T.Tan,E.Feenberg,Necessary conditions on radial distributionsfunctions,J.Math.Phys.8(1967)864–869,10citations.[62]F.Y.Wu,Critical behavior of hydrogen-bonded ferroelectrics,Phys.Rev.Lett.24(1970)1476–1478,10citations.[63]K.G.Chen,H.H.Chen,C.S.Hsue,F.Y.Wu,Planar classical Heisenberg modelwith biquadratic interactions,Physica A87(1977)629–632,10citations. [64]F.Y.Wu,Phase diagram of a spin-one Ising system,Chin.J.Phys.16(1978)153–156,10citations.[65]S.Sarbach,F.Y.Wu,Exact results on the random Potts model,Z.Phys.B44(1981)309–316,10citations.[66]F.Y.Wu,Eight-vertex model and Ising model in a nonzero magneticÿeld on thehoneycomb lattice,J.Phys.A23(1990)375–378,10citations.[67]C.K.Hu,C.N.Chen,F.Y.Wu,Histogram Monte-Carlo renormalization group:applications to the site percolation,J.Stat.Phys.82(1996)1199–1206, 10citations.[68]W.T.Lu,F.Y.Wu,Dimer statistics on a M o bius strip and the Klein bottle,Phys.Lett.A259(1999)108–114,10citations.[69]H.J.Brascamp,H.Kunz,F.Y.Wu,Some rigorous results for the vertex model instatistical mechanics,J.Math.Phys.14(1973)1927–1932,9citations. [70]X.N.Wu,F.Y.Wu,Critical line of the square-lattice Ising model,Phys.Lett.A144(1990)123–126,9citations.[71]L.H.Gwa,F.Y.Wu,Critical surface of the Blume–Emery–Gri ths model on thehoneycomb lattice,Phys.Rev.B43(1991)13755–13777,9citations.[72]F.Y.Wu,H.Y.Huang,Exact solution of a vertex model in d dimensions,Lett.Math.Phys.29(1993)205–213,9citations.[73]H.Y.Huang,F.Y.Wu,H.Kunz,D.Kim,Interacting dimers on the honeycomblattice:an exact solution of theÿve-vertex model,Physica A228(1996)1–32, 9citations.[74]F.Y.Wu,Duality relations for Potts correlation functions,Phys.Lett.A228(1997)43–47,9citations.[75]R.Shrock,F.Y.Wu,Spanning trees on graphs and lattices in d dimensions,J.Phys.A33(2000)3881–3902,9citations.[76]W.J.Tzeng,F.Y.Wu,Spanning trees on hypercubic lattices and non-orientablesurfaces,Appl.Math.Lett.13(2000)19–25,9citations.。

手性与对称性

手性与对称性

Chapter5Chiral Dynamics5.1What is spontaneous symmetry breaking?Symmetries and their breakings are important part of modern physics.Spacetime symmetry and its supersymmetric extensions are the basis for building quantumfield theories.Internal symmetries, such as isospin(proton and neutron,up and down quark symmetry),flavor,color etc.,form the fundamental structure of the standard model.On the other hand,studying symmetry breakings is as interesting as studying symmetries themselves.As far as we know,there are three ways to break a symmetry:explicit breaking,spontaneous breaking,andfinally anomalous breaking.In this part of the lectures we will concern ourselves with thefirst two types of breakings of the so-called chiral symmetry,the exact meaning of which will become clear later.We will come to the anomalous symmetry breaking towards the end of the course.In quantum mechnics,a symmetry of a hamiltonian is usually reflected in its energy spectrum. For instance,the rotational symmetry of a three-dimensional system often leads to a2ℓ+1-fold degeneracy of the spectrum.This standard realization of a symmetry is called Wigner-Weyl mode. On the other hand,in the late50’s Nambu and Goldstone discovered a new way through which a symmetry of a system can manifest itself:spontaneous breaking of the symmetry.This realization of a symmetry is called Nambu-Goldstone mode.To understand the Nambu-Goldstone realization of a symmetry,let us recall a related problem in statistical mechanics:second-order phase transitions.We have many examples of the second-order phase transitions in which a continuous change of order parameters happens.Consider a piece of magnetic material.Its hamiltonian is certainly rotationally symmetric and therefore normally one would expect its ground state wave function is also rotationally symmetric.This apparently is not the case below a certain critical temperature at which a spontaneous magnetization occurs. The magnitization vector points to a certain direction in space,and hence the rotational symmetry is lost.We say in this case that the rotational symmetry is spontaneously broken.Likewise,for a conductor below a certain temperature,the electromagnetic U(1)symmetry is spontaneously broken and the wavefunction of the Cooper pairs developes certain classical value.A useful mathematical formulation of the SSB is the concept of the effective action.Let us introduce thisfirst.Consider a scalarfield theory with lagrangian density L(φ).We define the green’s function8182CHAPTER5.CHIRAL DYNAMICS functional or generating functional Z(j)asZ(j)=∞i=0i n[Dφ]e i d4x L(x).(5.2)We define the connected green’s function G(n)c throughW(j)=∞i=1i nδj(x),(5.4)from which one can solve j(x)as a functional ofφ(x).Perform now the Legendre transformation,Γ(φ)= W− d4xj(x)φ(x) |j=j(φ)(5.5) ThenΓ(φ)is the generating functional for the one-particle irreducible Green’s functionsΓ(n)(x1,···,x n),Γ(φ)= n=11δφ(x).(5.7)Effective action can be computed through the shift offield in the lagrangianφ→φ+φc,and calculating the1PI contribution to the effective W.There are two popular usage of the effective action formalism:First,the effective action containsall the1PI which are the target for renormalization study.The renormalization condition can5.1.WHAT IS SPONTANEOUS SYMMETRY BREAKING?83 easily expressed in terms of1PI,like the mass of the particles and coupling constants.Moreover, the symmetry of these1PI can be expressed in terms of the Ward-Takahashi identities which can be summarized in terms of a simple equation for the effective action.This equation can be used to prove the Goldstone theorem.Second,the effective action can be used as a thermodynamic function with natural variableφc which diagnoses the phase structure of the system.For instance, according to Colemann-Weinberg,the natural phase of the massless scalar electrodynamics is the Higgs phase in which the vector and scalar particles aquire mass through radiative corrections. Another use of the effective action is in cosmology.The spontanous symmetry breaking happens only if there is a degeneracy in the vacuum.This degeneracy can arise from certain symmetry of the original lagrangian.Consider a symmetry transformation offields,φi(x)→φ′i(x)= j L ijφj(x),(5.8)here we have assumed multiplefields with i=1,...,n.If the action and measure are both invariant, then the effective action is invariant under a similar transformation of the classicalfieldsΓ[φ]=Γ[Lφ].(5.9) As we mentioned before,the vaccum state is a solution¯φof−Γ[φ]at its minimum.If the solution is invariant L¯φ=¯φ,i.e.the vacuum is invariant under the symmetry transformation,the vacuum is unique.On the other hand,if L¯φ=¯φ,the solution is not.Then we have many degenerate vacua which are all physically equivalent.By choosing a particular barφas the true vaccum,we have a spontaneous symmetry breaking.According to the above discussion,the key condition for SSB is there are multiple,equivalent vacua.Although it is easy tofind ground state degeneracies in the classical systems,in quantum systems it is difficult to have multiple vacuum.For instance,in a potential with a double well,the ground state is a non-degenerate symmetrical state.In other words,the real vacuum is a linear combination of the various classical vacua.The same thing happens for a rotationally symmetric system in which the ground state has J=0,i.e.,allθangles are equally probable.There are special cases in quantum mechanics in which the ground state may be degenerate. For instace,in an atom with a ground state J=0,the state can be prepared in the eigenstates of J2and J z.However,there is no SSB because the states of different J z are not equivalent vacua in the sense that they blong to the same Hilbert space and are easily connected through a transitions operators.Therefore,the spontaneous symmetry breaking happens only if the volume of the system is approaching infinity and the transition rate between the degenerate states goes to zero.In this case,it turns out that the vacuum states are not representations of the symmetry generators. Rather they are eigenstates of the conjugating coordinate operators and are superposition of states with symmetry quantum numbers.Any perturbation which causes the transition between different vacua have exponentially small matrix elements.On the other hand,the diagonal matrix elements of the perturbation is much larger than the off-diagonal matrix elements.In other words,the vacuum states are those with definite¯φ,or in the rotationally symmetric system,definiteθ.So in the limit of infinit volume,the states with definite¯φbecome the exact vacua.It can be shows that with local hamiltonian and operators,different vacua obey the super-selection rule.Assume the degenerate vacua are|v i andv i|v j =δij(5.10)84CHAPTER5.CHIRAL DYNAMICS By considering the matrix element of v i|A( x)B(0)|v j in the limit of x→∞,it can be shownu i|A(0)|u j =δij a i.(5.11) Therefore the local operators have nofinite matrix elements between different vacuum states. 5.1.1SSB and Space(-time)DimensionsIn afinite quantum mechanical system,there is no SSB.For discrete symmetry,such as Z2symmetry (σi→−σi)in the Ising model,it cannot be broken in one-dimensional(0+1)system.This is known in1938to Peierls.But,it can be broken in two-dimensional(1+1)system.For example, the Onsagar solution contains a spontaneous magnetization for a two-dimensional Ising model.For continuous symmetry,it cannot be spontaneously broken in two-dimensional system.This is called the Mermin-Wagner-Coleman theorem.For example,the classical Heisenberg model consists of interactions of spins living on a n-dimensional sphere.The system has O(n)symmetry.This model has spontaneous symmetry breaking only in3D.To see the MWC theorem,let’s assume there is a SSB in2D.Then we have massless Goldstone bosons.The correlation of these massless Goldstone bosons reads0|φ(x)φ(0)|0 = d2k2πk1cos(k1x1)e ik1x0(5.12)which is hopelessly infrared divergent.This strongfluctation will destroy any long-range order. In a two-dimensional classical Heisenberg model,an disordered phase has as much weight as an ordered one.5.2SSB of the continuous symmetry and Goldstone TheoremIn the case of the spontaneous breaking of a continuous symmetry,a theorem can be proved.The theorem says that the spectrum of physical particles must contain one particle of zero mass and spin for each broken symmetry generator.Those particles are called Goldstone bosons.Consider an infinitesimal transformationφi→φi+iǫa(t aφ)i.(5.13) The same transformation leaves the effective action invariantijd4xδΓ∂φit a ijφj=0,(5.15)This relation is true independent ofφ.Differentiate the above equation with respect toφk and take φ=¯φin a vacuum,∂2V(φ)5.2.SSB OF THE CONTINUOUS SYMMETRY AND GOLDSTONE THEOREM85According to the definition of the effective potential,we have∂2V (φ)2∂µφi ∂µφi −14(φi φi )2(5.19)In the tree approximation Γ=V 3L ,we haveV =14(φi φi )2(5.20)If M 2is negative,we have¯φi ¯φi =−M 2/g(5.21)We can choose a solution as ¯φi =(0, 0∂φi ∂φj |φ=¯φ=2g ¯φi ¯φj =(0,...,0,2|M 2|)(5.22)Thus the last particle now has mass √86CHAPTER5.CHIRAL DYNAMICS we have the effective classical hamiltonianH eff= N1∂φi 1···φi N (5.27)From equations derived earlier,it is easy to see that the amplitude for a zero-momentum Goldstone boson disappearing into the vacuum is zero.The amplitude for a zero-momentum goldstone boson to make transition to another boson is zero.Finally,the amplitude for three massless Goldstone bosons to make transtion is zero.This is in fact true to all orders.Let us consider now the interactions of Goldstone bosons with other massive particles.The following approach assumes exact symmetry.To calculate the process ofα→β+B a,we start from the matrix element with the corresponding conserved currentβ|Jµa|α .(5.28) The current supports a momentum transfer q=pα−pβ.Clearly the most important contributionto matrix element comes from the Goldstone boson pole which has the following structureiF qµMβB,αFqµNµβ+J,α.(5.30)This is a form of Ward identity.If Nµhas no pole,then the process of emitting a Goldstone boson vanishes as q→0.This is called the Adler zero.The most important contribution in the regular term comes from the Feynman diagrams in which J acting on the external line.In this case,there is a heavy-particle pole which enhance the contribution.The pole contribution can often be calculated or extracted from experimental data,from example,the nucleon pole contribution is related to the neutron beta decay constant g A.Knowing g A,we can calculate the meson-nucleon interaction as we shall do in the next section.The above result can also be derived from a theory with explicit breaking of the symmetry.This approach is called PCAC.In this case,the masses of the Goldstone bosons are not exactly zero, butfinite.They are called pseudo-Goldstone bosons.Let us consider the SSB of an approximate symmetry.In this case,the vacuum is no longer degenerate,and strictly speaking,there is no spontaneous symmetry breaking.This is very much like a magnet in an external magneticfield(first order phase transition).In the following we would like tofind the constraint on the vacuum from the symmetry breaking effects;we also want to derive the masses of the pseudo-Goldstone bosons.5.3.PION AS GOLDSTONE BOSON,PCAC87Now the effective potential has two terms V(φ)=V0(φ)+V1(φ).The real solution isφ=φ0+φ1 which is no longer degenerate.The condition onφ0andφ1is contained in the expanded version of ∂V(φ)/∂φi|φ=¯φ=0∂2V0=0(5.31)∂φiUsing the equation we found early,we have∂V1(φ0)(t aφ0)i(5.33)∂φi∂φjwhich vanish to the zeroth order.To the frist order,wefindM2ab=− cd F−1ac F−1bd 0|[T a,[T b,H1]]|0 (5.34) where T a is the quantum generator of the symmetry group.5.3pion as goldstone boson,PCACOne of the most interesting examples of SSB is exhibited by fundamental strong interactions:quan-tum chromodynamics.Consider the QCD lagrangian.The only parameters with mass dimension are quark masses.For ordinary matter,we just consider up and down quarkflavors.The QCD scale ΛQCD is about200MeV,which is much larger than the up and down quark masses(5to9MeV). Therefore,to a good approximation,we can negelect the quark masses in the QCD lagrangian. Then the QCD lagrangian has the U(2)×U(2)chiral symmetry.Recall the chiral projection operators P L=(1−γ5)/2and P R=(1+γ5)/2,whereγ5is diag (-1,1),which project out the left-handed and right-handed quarkfields,ψL,R=P L,Rψ.(5.35) Then the QCD lagrangian we can be written in terms ofL=ψR(i D)ψR−188CHAPTER5.CHIRAL DYNAMICS where U L,R are unitary matrices in the two-dimensionalflavor space.Since U(2)=U(1)×SU(2),we have two U(1)symmtries.From now on,we focus on the two SU(2)symmetries,leaving the U(1) symmetries to later discussion.According to Noether’s theorem,the SU L(2)×SU R(2)chiral symmetry leads to the the following conserved currents,jµL,R=¯ψL,R t aγµψL,R,(5.38) where t a=τa/2andτa is the usual Pauli matrices.We have the vector and axial vector currents from the linear combinations,j aµV=¯ψt aγµψ=jµL+jµRj bµA=¯ψt aγµγ5ψ=jµR−jµL.(5.39) From the above currents,we can define the charges Q a and Q a5in the usual way.And it is easy to see that the charges obey the following algebra:[Q a,Q b]=iǫabc Q c;[Q5a,Q b]=iǫabc Q5c;[Q5a,Q5b]=iǫabc Q c.(5.40)From the above,wefind that Q a forms a subgroup of the chiral symmetry group and is called the isospin group.From the experimental hadron spectrum,wefind that the isospin subgroup is realized in Wigner-Weyl mode.For instance,the pion comes in with three charge states and near degenerate mass.The proton and neutron also have nearly degenerate mass.However,the spectrum does not show the full chiral symmetry.For instance,the three pion states do not form an irreducible reps of the chiral group.Together a scalar particleσ,they form(1/2,1/2)reps. Therefore,if the chiral symmetry is realized fully in Wigner-Weyl mode,there must be a scalar particle with the same mass as the pion.We do not see such a particle in Nature.Thus,the chiral group SU L(2)×SU(2)R must break spontaneously to the isospin subgroup SU(2).Thus the QCD vacuum|0 satisfiesQ a|0 =0,Q5a|0 =0.(5.41) According to Goldstone’s theorem,there are three massless spin-0pseudo-scalar bosons.They are pseudoscalars because Q5a changes sign under parity transformation.Of course,in the real world,we don’t have massless pseudoscalars.We have pions.The pion masses are indeed much smaller than a typical hadron mass.For instance,the rho meson has mass 770MeV.The nucleon mass is940MeV.And the pion mass is140MeV.The pions are called pseudo-Goldstone bosons because the chiral symmetry is not exact.It is broken by thefinite up and down quark masses.H1=m u¯u u+m d¯dd.(5.42) If we write u in terms of left and right-handedfields,we haveH1=m u(¯u L u R+¯u R u L)+m d(¯d L d R+¯d R d L).(5.43)Therefore the left and right-handedfields are now coupled through the mass terms.The mass operator transforms as the components of(1/2,1/2)representations of the chiral group.Using the relation we found earlier,we can calculate the pion mass,m2π=−(m u+m d) 0|¯u u+¯dd|0 /f2π(5.44)5.3.PION AS GOLDSTONE BOSON,PCAC89 where 0|¯u u+¯dd|0 is the chiral condensate.Since¯u u is a part of the representation(1/2,1/2),it vacuum expectation value vanishes ordinarily because of the chiral symmetry.However,it has a vacuum expectation value because of the vacuum is no longer chirally symmetric(chiral singlet). In fact,the vacuum contains all(k,k)type of representations because the vacuum has zero isospin. Any chiral tensor of type(k,k)has non-zero vacuum expectation value.The pion decay constant fπis defined from0|jµa(x)|πb =ipµδab fπe−ip·x.(5.45) It can be measured from the semi-leptonic weak decayπ+→µ+νµrateG2F m2µf2π(m2π−m2µ)2Γ=U(p′)t a[g A(q2)γµγ5+g p(q2)qµγ5]U(p),(5.48) where q=p−p′and U’s are the on-shell Dirac spinors of the nucleon states.Multiplying qµto both sides of the equation and using current conservation and Direc equation(p−M)U(p)=0, we have−2Mg A(q2)+q2g P(q2)=0.(5.49) g A(q2)in the limit of q2→0is just the neutron decay constant(the axial current is part of the weak interaction current)and has been measured accuratelyg A(0)=1.257.(5.50) Thus according to the above equation g P(q)must have a pole in1/q2.This pole corresponds to the intermediate massless pion contribution to the interaction between the the axial current and the nucleon.If we introduce the pion-nucleon interaction vertex gπNN¯Niγ5τa Nπa,the contribution to the axial current matrix element is(ifπqµ).(5.51)i2gπNNq2In the limit of q2→0,wefind the following celebrated Goldberger-Treiman relationg A(0)M=gπNN fπ.(5.52) Using gπNN from experimental data(g2πNN/4π=14.6),wefind that the above relation is obeyed at better than10%level.90CHAPTER5.CHIRAL DYNAMICS According to the recipe derived from the previous section,we calculate the interactions between the soft pion and the nucleon system as follows.First use a vertex iqµ/fπconnecting the Goldstone boson to the axial current.Then the non-singular part of the axial current interaction with the nu-cleon is approximated through the g Aγµγ5vertex.This yields the effective pion-nucleon interaction vertex i qγ5/fπ.This is a peudo-vector interaction.Another way to study the interactions among the pions and with other particles is through what is called the PCAC(partially-conserved axial-vector current),in which we assume there is a small explicit symmetry breaking through nonvanishing quark masses.Applying the derivative operator to the current matrix between the vacuum and the pion,we have0|∂µjµa|πb =m2πδab fπ.(5.53) The right-hand side is proportional to the pion mass squared.This motivates the assumption that∂µj aµ=m2πfππa,(5.54)whereπa is a pion interpolatingfield.Of course,the above relation is in some sense empty because any pseudo-scalar operator can be used as an interpolatingfield for pion.The content of the PCAC is that axial current at zero momentum transfer(this is the place where we know how to calculate the matrix element)is dominated by the pion contribution at q2=m2π.In other words, the variation of the matrix elements of the axial current from q2=0to m2πis smooth.In fact,we can derive the Goldberger-Treiman relation using PCAC andfind now one has to use g A(0)instead of g A(m2π).The content of PCAC is that the variation of this small.Therefore,when the pion energy is small,we can calculate using PCAC.PCAC can be used to study the multi-pion interactions.For instance,consider the amplitudeT abµν= d4xe iqx H(p2)|T A aµ(x)A bν(0)|H(p1) (5.55) Applying differentical operators to the above quantity,we derive a Ward ing PCAC, one can calculate the pion-nucleon scattering amplitude at low-energy.However,it turns out that it is much easier to get the predictions using the low-energy effective theory.5.4the linearσmodelMany of the essential physics exhibited in spontaneous breaking of the chiral symmetry can be illustrated by a simple phenomenological model.This is very similar to the Ginsburg-Landau theory for second-order phase transitions.This model isfirst introduced by Gell-Mann and Levy, and is called the linearσmodel.The lagrangian is,L=L S+cσ,L S=¯ψ[i∂+g(σ+i π·τγ5)]ψ+12(σ2+ π2)−λ5.5.EFFECTIVE FIELD THEORY:CHIRAL PERTURBATION THEORY WITH PIONS91 term cσ,the lagrangian is clearly symmetric under the chiral SU L(2)×SU R(2),and the correspond-ing vector and axial vector current isτajµa=¯ψγµψ+(σ∂µπa−πa∂µσ)(5.57)2After introducing the symmetry breaking term,the axial vector current is no longer conserved.We have instead∂µA aµ=−cπa(5.58) according to the equation of motion.The above has the form of PCAC.Whenµ2<0,the spontaneous symmetry breaking happens.The potential has its minimum not atπa=σ=0but atπ2+σ2=v2,where v2=−µ2/λ.Thus,the shape of the potential is a Mexican hat.There are infinite many degenerate minima.We need to choose a particular direction as our vacuum state.If we want to keep the isospin group intact,we takeσ =v.(5.59) The pion excitation corresponds to the motion along the minima and therefore has zero energy unless the wavelength isfinite.Theσmass corresponds to the curvature in theσdirection and is 2λv2.The nucleon also get its mass from spontaneous symmetry breaking and is−gv.From the PCAC,wefind that fπ=−v.When the symmetry breaking term is introduced,the Mexican hat is tilted.In this case,the minimum of the potential is unique and the pion excitations do have mass.5.5effectivefield theory:Chiral Perturbation theory with pionsCurrent algebra and Ward identity approach were popular in the60’s for calculating Goldstone boson interactions.However,they are tedious.In1967,Weinberg used the nonlinearly-transformed effective lagrangian to study the Goldstone boson interactions.This is the precursor of effective field theory approach which is popular today.The key observation is that when the Goldstone boson energy is small,the coupling is weak. Therefore their interactions must be calculable in perturbation theory.However,in the strong interactions,we also have the usual QCD or hadron(rho meson or nucleon)mass scale.The physics at these two different scales have to be separated before one can apply chiral perturbation theory.The physics at QCD or hadron mass scale can be parametrized in terms of various low-enegy constants which can be determined from experimental data.Through a particular model,we demonstrate the separation of physics through nonlinear trans-formations.Wefirst perform a symmetry transformation at every point of the spacetime to get rid of the Goldstone boson degrees of freedom.We then re-introduce them through the spacetime-dependent symmetry transformation.When the Goldstone-bosonfields are constant,the transfor-mation is the usual chiral tranformation;and the Goldstone bosonfields disappear.Therefore,in the new lagrangian,the Goldstone boson interaction must have derivative-type interactions.Consider the linear sigma model.Let us introduce a(1/2,1/2)2×2matrixU=σ+i π·τ(5.60)92CHAPTER5.CHIRAL DYNAMICSUnder the chiral transformation,we haveU→U L UU†R(5.61) We can write the linear sigma model asL=14Tr[UU†]−λπ2+σ2.We reintroduce back the goldstone boson by parametrizing the U including the axial transformation parameters,U=σe i πa(x)·τa/fπ(5.64) whereπa=fπθa A is now the Goldstone bosonfield.For the convenience,we call the exponential factorΣ.Now substituting U=σΣinto the original lagrangian,we get,L=14σ2Tr[∂µΣ∂µΣ†]−14σ4.(5.65) Now the Goldstone bosonfields contain derivatives and therefore the above lagrangian will pro-duce appropriate Goldstone boson interactions.Since theσparticle has a typical hadronic mass, its effects can be integrated out completely and theσis then replaced by its expectation value. Therefore,the effective intereaction lagrangian for pion is justL(2)ππ=f25.5.EFFECTIVE FIELD THEORY:CHIRAL PERTURBATION THEORY WITH PIONS93 Using L=I− i V i+1,we haveν= i V i(d i−2)+2L+2.(5.69)Therefore the lowest power of Q in any pion process is2.We can use the above leading order lagrangian to calculate the interactions between the pions. Expand in1/fπto to the second order,we have[(∂µ π· π)2− π2(∂µ π)2]+...(5.70) L(2)ππ=16f2πThe second term can be used to calculate the S-matrix element between pion scattering.Assume the incoming pions with momenta p A and p B and isospin indices a and b and the outgoing pions with momenta p C and p D and isospin indices c and d.We have the following leading-order invariant amplitude(S=1−iM),M=−f−2π(δabδcd s+δacδbd t+δadδbc u)(5.71) where s=(p A+p b)2,t=(p A−p C)2and u=(p A−p D)2are called Mandelstam variables.5.5.1Scalar and Pseudoscalar SourcesWe can include the quark mass effects at this order.The quark mass term transforms like(1/2,1/2) under chiral transformations.In general,let us introduce s and p source in the QCD lagrangianL sp=−¯ψs(x)ψ+¯ψiγ5p(x)ψ=−¯ψR(s+ip)ψL−¯ψL(s−ip)ψR(5.72) Call s−ip=χand s+ip=χ†.Then the interaction is invariant ifχ→LχR;χ†→Rχ†L†(5.73) Without the p source,χ∼χ†∼s∼m q,which counts as second order in momentum.The effective lagrangian then containχas a O(p2)external source.The lowest order isL(2m)ππ=B Tr(Σχ†+Σ†χ).(5.74) When expanded to the leading order,the above gives the pion mass contribution if B=f2π/4and χ=m2π.The next-order contribution ism2π94CHAPTER5.CHIRAL DYNAMICSAt the threshold where s=4m2π,t=u=0,we haveM=−m2πf−2π[3δabδcd−δacδbd−δadδbc].(5.77) The scattering amplitude f=−M/8π√16f4π −1µ2−1µ2−1µ2 −14c2(t2+u2) +crossing(5.78)where c1and c2are constants which must be determined from experimental data.In fact,there are also pion mass contribution at this order which we will not go into.The p4-order mass term include the followingL4Tr(DµΣ†DµΣ)Tr(χ†Σ+χΣ†)+L5Tr(DµΣ†DµΣ)(χ†Σ+χΣ†)+L6(Tr(χ†Σ+χΣ†))2+L7(Tr(χ†Σ−χΣ†))2+L8Tr(χ†Σχ†Σ+χΣ†χΣ†)+H2Tr(χ†χ)(5.79) where H2is pointless because there is no meson depedence.5.5.2Electromagnetic and Axial InteractionsWhen there are electromagnetic and weak interactions with the Goldstone boson system,we need to construct a gauge theory in which the effective theory is gauge invariant under gauge transfor-mations.Introduce the the following coupling the QCD lagrangianL=¯ψ(γµvµ(x)+γµγ5aµ(x))ψ=¯ψLγµ(vµ−aµ)ψL+¯ψRγµ(vµ+aµ)ψR(5.80) If vµand aµare gaugefields,under gauge transformation,they must transform in the following way,vµ−aµ→L(vµ−aµ)L†+iL∂µL†vµ+aµ→R(vµ−aµ)R†+iR∂µR†(5.81) The above equation means that these gaugefields have to appear together withΣin the following formDµΣ=∂µΣ−i(v−a)µΣ+iΣ(v+a)µ(5.82)5.6.BANKS-CASHER FORMULA AND VAFA-WITTEN THEOREM95 Then all the partial derivatives will be replaced by the above covariant derivatives.For example,consider the electromagnetic interaction of the pions.In this case,we replace vµ=−ie(τ3/2+1/6)Aµwhere e is the charge of a proton andτ3is the isospin and1/6is the hypercharge.Then the partial derivative becomes,DµΣ=∂µΣ+ieAµ[τ3∂x1+∂A2∂x3+∂A496CHAPTER5.CHIRAL DYNAMICS The electricfield E in the Euclidean space is the imaginary of that in the Minkowski space and so E2→−E2,and FµνFµν=−2(E2−B2)→2(B2+E2)=FµνFµν.We also define the Euclidean version of theγmatrix withγE4=γ0andγE i=−iγi and the commutators now become{γEµ,γEν}=2δµν(5.91) The newγmatrices are hermitian.The QCD lagrangian is nowL QCD=−4FµνFµν (5.92)Notice thatγµDµis now an antihermitian operator.We can define the Euclidean L to absorb the minus sign.Consider now the exponential factor exp(iS)in the path integral.After rotation,the integral d4x becomes−i d4x.The−i here cancels the i in front of the iS and define the Eulidean action asS E=− d4x L(5.93) Therefore the integration meansure becomes exp(−S E)Let us see how the spontaneous symmetry breaking takes place in QCD.To this goal,we need to introduce an explicit breaking of the symmetry.For example,we give a small mass to quarks. Consider the expectation value of ¯u u .We writeV4d4x u(x)¯u(x)=− [DA]e−S Y M Det(D+M)1D+m u].(5.94)where Tr is over spatial,color,and spin indices.Now consider the eigenstates of D.Because it is an anti-hermitian operator,we haveD|λ =iλ|λ ,(5.95) whereλis real.The different|λ are orthogonal and therefore we haveTr[1iλi+m u.(5.96)On the other hand,we have Tr(D+M)=Tr(−D+M)because(γ5)2=1.We get thenTr 1iλi+m u+1m2u+λ2i(5.97)Intrduce now aδ(λ−λi)and integration overλ.We have then¯u u =−dλρ(λ)m uZV4 [DA]exp(−S Y M)Det(D+M)i2δ(λ−λi)(5.99)。

三维简单正交晶格伊辛(Ising)模型精确解猜想

三维简单正交晶格伊辛(Ising)模型精确解猜想

三维简单正交晶格伊辛(Ising)模型精确解的猜想伊辛(Ising)模型是一个最简单的模型可以提供非常丰富的物理内容,可以被用来帮助我们发现物理世界的原则。

它不仅可以用来描述晶体的磁性,还可以用来描述非常广泛的现象,如合金中的有序-无序转变、液氦到超流态的转变、液体的冻结和蒸发、晶格气体、玻璃物质的性质、森林火灾、城市交通、蛋白质分子进入它们的活性形式的折叠等。

科学家对伊辛模型的广泛兴趣还源于它是描述相互作用的粒子(或原子或自旋)最简单的模型。

它可以用来测试研究相互作用的粒子在多体系统(特别是理解在临界点及其附近的合作现象和临界行为)任何近似方法的理想工具。

进一步说,三维伊辛模型可以研究从无限大温度到绝对零度相互作用的粒子(或原子或自旋) 系统的演变过程,如果将热力学中的温度作为动力学中时间来考量,它不仅可以理解热力学平衡的无限系统,如一个磁铁,还可以帮助理解我们的宇宙。

另外,平衡相变的理论可以用来研究连续的量子相变、基本粒子的超弦理论、在动力学系统到混沌的转变、系统偏离平衡的长时间行为和动力学临界行为等。

由于伊辛模型中的粒子(或原子或自旋)具有两种可能的状态(自旋向上或向下),它实际上可以对应黑白、上下、左右、前后、是非、正负……原则上,伊辛模型可以描述所有具有两种可能的状态的多体系统,描述两种极端条件间的相互竞争。

尽管伊辛模型是一个最简单的物理模型,目前仅有一维和二维的精确解。

Ising 在1925年解出的精确解表明一维伊辛模型中没有相变发生。

Onsager 于1944年获得二维伊辛模型的配分函数和比热的精确解,为统计物理领域的一个重大进展。

杨振宁于1952年求出二维伊辛模型的自发磁化强度。

二维正方伊辛模型的居里温度精确地存在于122−==−c K c e x 即1/K c = 2.26918531……。

二维伊辛模型的临界指数为α = 0, β = 1/8, γ = 7/4, δ = 15, η = 1/4 和 ν = 1。

Exact Solutions of the Generalized Equal Width Wave Equation

Exact Solutions of the Generalized Equal Width Wave Equation
+∞ −∞
(u )2 dξ = k2 , as ξ −→ +∞ ,
(13)
By substituting (14) into (13) and using the relation (11), we obtain the analytical expression of the following important square integral,
2
Derivation of the Exact Solutions
We concentrate on finding an exact solitary wave solution of the form u(x, t) = u(x − x0 − Ct) . (3)
This corresponds to a traveling-wave propagating with steady celerity C . We are interested in solutions depending only on the moving coordinate ξ = x − x0 − Ct as, u(x, t) = u(x − x0 − Ct) ≡ u(ξ ) . (4) Substituting into (2), the function u(ξ ) satisfies a third order nonlinear ordinary differential equation (ODE), −Cu + aup u − δu + µCu =0, (5)
Abstract. The equal width wave (EW) equation is a model partial differential equation for the simulation of one-dimensional wave propagation in nonlinear media with dispersion processes. The EW-Burgers equation models the propagation of nonlinear and dispersive waves with certain dissipative effects. In this work, we derive exact solitary wave solutions for the general form of the EW equation and the generalized EW-Burgers equation with nonlinear terms of any order. We also derive analytical expressions of three invariants of motion for solitary wave solutions of the generalized EW equation.

2025届高考英语二轮专题复习与测试专题强化练三推理判断题__观点态度类

2025届高考英语二轮专题复习与测试专题强化练三推理判断题__观点态度类

专题强化练(三) 推理推断题——观点看法类A(2024·广州市高三调研测试)Our planet quakes thousands of times a year,but we still can't predict exactly when and where earthquakes will strike.What if animals' odd behaviors could warn us?Researchers have reviewed hundreds of reports on pre­packed abnormal animal behaviors,but more were just anecdotes.Geologist Jim Berkland counted newspaper ads looking for runaway cats and dogs.On October 13,1989,he told a newspaper reporter a big quake would strike in a week.Four days later,the Loma Prieta earthquake hit! But the scientific community still rejected Berkland's theory.He didn't document every prediction,so nobody could measure his accuracy rate.Actual scientific evidence has to be repeatable.And a connection between a cause and an effect has to be shown to be stronger than random chance through careful experimentation and data collection.California researchers in the 1970s happened to have built controlled habitats to monitor the wheel­running activity of pocket mice.These habitats happened to be in an active earthquake area.Then the 1971 San Fernando Earthquake struck nearby.The researchers checked their data and found no big changes in how long the animals ran in their wheels or stayed underground before the earthquake activity.What might the next experiment show?Researchers from 150 universities worldwide are working on a new study called the ICARUS project.The project tracks many small animal species such as birds,bats,and turtles for the purpose of scientific research.One group of researchers are looking for possible connections between animal behaviors and earthquakes.If they find a reliable connection,this could save hundreds of thousands of human lives.ICARUS aims to power an app that will give people hours to get to safety.However,not everyone is hopeful.Geologist Wendy Bohon said that ICARUS is doing some “cool things”,but she knows animal behaviors are hard to pin down.“My cat could act crazy before an earthquake,”she says.“But it also acts crazy if somebody uses the can opener.”【语篇解读】本文是一篇说明文。

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a r X i v :c o n d -m a t /9705161v 1 [c o n d -m a t .d i s -n n ] 16 M a y 1997EXACT SOLUTION OF A 2D RANDOM ISING MODELMaurizio Serva Dipartimento di Matematica,Universit`a dell’Aquila and I.N.F.M.I-67010Coppito,L’Aquila,Italy ABSTRACT The model considered is a d =2layered random Ising system on a square lattice with nearest neighbours interaction.It is assumed that all the vertical couplings are equal and take the positive value J while the horizontal couplings are quenched random variables which are equal in the same row but can take the two possible values J and J −K in different rows.The exact solution is obtained in the limit case K →∞for any distribution of the horizontal couplings.The model which corresponds to this limit can be seen as an ordinary Ising system where the spins of some rows,chosen at random,are frozen in an antiferromagnetic order.No phase transition is found if the horizontal couplings are independent random variables while for correlated disorder one finds a low temperature phase with some glassy properties.PACS NUMBERS:05.50.+q,02.50.-rIsing spin glasses have been solved exactly in their meanfield version[1,2]while as far as I know no exact solutions are available atfinite dimensionality d≥2.Indeed, in presence of disorder even a d=1system with magneticfield is a very complicated problem[3]and compact exact solutions can be found only in special cases[4].This is frustrating since it is not always clear if the qualitative results of a meanfield approximation are shared by thefinite dimension model.In this paper I am far from answering this problem,nevertheless I exactly solve a class of d=2layered random Ising systems which in some conditions have a low temperature phase.The nature of this non-ferromagnetic low temperature phase is still unclear to me,but there are some indications that it shares some of the properties of a glassy phase.The models I consider are defined as follows:the interaction is effective only between nearest neighbours on a square lattice;all the vertical couplings are equal while the horizontal couplings are quenched variables which are equal in the same row but can take different values in different rows;the vertical couplings take the positive value J while the horizontal couplings J i can take the two possible values J and J−K with K→∞.These models have frustration since the product of the signs of the coupling around a plaquette can be negative.Different distributions of the horizontal couplings correspond to different models of the class;in the simplest case the J i are independent random variables and take the value J with probability1−p and J−K with probability p.Layered Ising models of this type have beenfirst considered by B.M.McCoy and T.T.Wu[5,6]for the non frustrated case which is used for studying the effect of quenched randomness on the ferro-para transition.These authors deal with the determinant which occurs in the Pfaffian approach and while they do not provide an explicit exact solution of the problem they are able to show that the free energy has aninfinitely differentiable singularity at the yered models with frustration have been studied by R.Shankar and Ganpathy Murthy[7],not only their topic but also their approach is the same of this work since they deal with the row to row transfer matrices.They do notfind out an exact solution,nevertheless they map the problem into a collection of d=1randomfield Ising systems from which they can extract a lot of informations.In particular they provide evidence for the existence of a low temperature phase.Let me now state more precisely the problem.Assume that N=LM is the number of spins,L is the number of rows and M the number of columns,the hamiltonian can be written asH N=− ij(Jσi,jσi+1,j+J iσi,jσi,j+1)(1) where the J i are the horizontal couplings whose value only depend on the row i and not on the column j.One can write J i=J−ηi K where the quenched variablesηi can take the value0and1according to a given distribution.In the independent case ηi=0with probability1−p andηi=1with probability p.The partition function is Z N= {σ}exp{ ijβ(Jσi,jσi+1,j+Jσi,jσi,j+1−ηi K(1+σi,jσi,j+1))}(2) where the constant term ijηi K has been added to the hamiltonian in order to avoid divergences in the K→∞limit.After having definedΓ≡Jβand performed the limit K→∞one obtainsZ N= {σ} ij exp{Γσi,jσi+1,j+Γσi,jσi,j+1} 1−1+σi,jσi,j+1contribution to the partition function.It is now clear that(3)defines a class of Ising model with both vertical and horizontal couplings equal to J and with the spins of some rows frozen in an antiferromagnetic order.The frustration comes out from the fact that the tendency to the ferromagnetic alinement due to the positive couplings is in competition with the tendency to the antiferromagnetic alinement induced by the frozen spins on the unfrozen ones.A similar problem,where the spin are randomly frozen in a random direction has been solved in d=1in[4],and studied in d=2at zero temperature in[8].The advantage of considering layered disorder is that one can apply a standard diagonalization method[7,9],and reduce the problem to the evaluation of the trace of products of random matrices.Following the same steps of[7,9]one easilyfinds the free energyf=−J2πΓ π0γ(q,Γ)dq(4)whereγ(q,Γ)=limL→∞12log(tanhΓ).The trace of a product of random matrices is easily accessible via computer simulation but it cannot be,in general,exactly computed.In the present case,nevertheless,following a similar method as in [4],it is possible to find out the compact analytical result.Consider a given realization of the quenched variables ηi and look at the product of matrices in (5).Since T i (q,Γ)=E i ·T (q,Γ)that product reduces to a product of matrices T (q,Γ)and up projectors τ+.The first and the second τ+will be separated by l 1matrices T (q,Γ),the second and the third by l 2matrices T (q,Γ),and so on.The l n are random variable which can take the values 1,2,....whose distribution can be easily found out once the distribution of the ηi is given.The order number n goes from 1to n f =L/¯l ,in fact,one must have n f n =1l n =L sothat n f n =1l n /n f ≡¯l =L/n f .With the help of these considerations one can rewrite(5)asγ(q,Γ)=lim L →∞1L L/¯l n =1log[T (q,Γ)l n ]11(8)where [T (q,Γ)l n ]11is the up left entry of T (q,Γ)l n .If P (l )is the probability that two successive rows of infinitely negative couplings are separated by l rows of finitepositive couplings than ¯l ≡ ∞l =1l P (l )andγ(q,Γ)=∞ l =11sinh 2Γ−cos q (11)andcos φ=cosh 2Γ(cos q −sinh 2Γ)2(12)Using(10)it is immediate to obtain[T(q,Γ)l]11=cosh(lǫ)+cosφsinh(lǫ)(13) Finally:f=−J2πΓ¯l∞l=1P(l) π0log(cosh(lǫ)+cosφsinh(lǫ))dq(14)whereǫandφare given in(11)and(12).The probability P(l)for the simplest choice of independentηi is P(l)=p(1−p)l−1 and¯l=1/p.In this case one can prove that the system has no phase transition,except for p=0where it trivially reduces to the ordinary Ising model.In Fig.1it is shown the specific heat C in correspondence of different values of p;one can notice that the logarithmic divergence is smoothed showing the absence of transition.Nevertheless, the model is frustrated and its zero temperature properties are not completely trivial. One can compute the T=0energy f0end entropy s0andfindsf0=−2J(1−p)2(15)s0=Jp2(1−p)log √2 (16) s0is not vanishing for p=0,1showing an exponential degeneration of the ground state due to the frustration of the model.Since the transition disappears for p=0the role of p reminds that of a magneticfield which also suppresses the transition.The analogue of the spontaneous magnetization is obtained in the limit p→0asf′≡ ∂f2πΓ π0log 1+cosφdTis not as shown in Fig.2where one can see a logarithmic divergence at T c(the Onsager critical temperature).The circumstance that a phase transition can be found only at p=0suggests to look more carefully at the model around this value.If one chooses p=α/L one has a vanishing p in the thermodynamic limit and the free energy is the same of that of the standard Ising model.Nevertheless,one has a randomfinite number of frozen rows.This number is Poisson distributed with intensityαand it is different for different realizations of the disorder(no self-averaging).The distance between two given frozen rows is also a random number of order of L and it also varies from a realization to another.Thefinal result is that the frozen rows separate a random number of regions of random size of order N whose magnetization at T≤T c is±m(T) independently one from the other(m(T)is the Onsager spontaneous magnetization at temperature T).As a consequence of this fact,the whole system can be in all the states corresponding to all the possible combinations of magnetization of each region. In conclusion,one has the same free energy of a standard Ising system but a number of pure states each of them corresponding to a different local magnetization.The situation is completely analogous to that studied in[10]for a diluted d=1model at zero temperature.Following the same line of[10]it is easy to compute the overlap probability,in particular for largeαone hasP(q)≃12πtexp{−q2be much more separated than in the independent case.This task can be accomplished with the choice P(l)=a/l3(a is the normalization constant)which replaces the exponential distribution P(l)=p(1−p)l−1of the independent case.By substituting this expression in(14)one can easily compute the free energy and look at the eventual divergences.In spite of the fact that the free energy is now different from that of the standard Ising model one stillfinds a phase transition at the Onsager temperature. Nevertheless this phase transition does not correspond to a divergence in the specific heat,but in its derivative dCReferences[1]D.Sherrington and S.Kirkpatrick,Phys.Rev.Lett.32,(1975),1792[2]M.Mezard,G.Parisi and M.Virasoro,Spin glass theory and beyond,WorldScientific Singapore1988[3]G.Paladin and M.Serva,Phys.Rev.Lett,69,(1992),706[4]G.Grinstein and D.Mukamel,Phys.Rev.B27,(1983),4503[5]B.M.McCoy and T.T.Wu,Phys.Rev.76,(1968),631[6]B.M.McCoy,Phys.Rev.B.2,(1970),2795[7]R.Shankar and Ganpathy Murthy,Phys.Rev.B36,(1987),536[8]B.Derrida and Y.Shnidman,J.Phisique Lett.45,(1984),L-507[9]T.D.Schultz,D.C.Mattis and E.H.Lieb Rev.Mod.Phys.36,(1964),856[10]A.Crisanti,G.Paladin,M.Serva and A.Vulpiani,Journal de Physique13,(1993),1993Figure CaptionsFig.1Specific heat C as function of the temperature T.The dotted line corresponds to the Ising model(p=0),the full line to p=0.1and the dashed line to p=0.2Fig.2Temperature derivative d f′∂p p=0as function of TFig.3Temperature derivative dC。

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