Sigma-model symmetry in orientifold models

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XANES理论

XANES理论

量子力学其中一个最突出的成就就是严格求解了氢原子的薛定谔方程,从 而对氢原子光谱和性质给出了相当满意的说明。
通过对氢原子薛定谔方程的求解,我们可以给出原子的轨道表达式,这是 我们了解和研究复杂原子及分子结构的基础。
轨道
表达式
角度部分表达式
s
px py pz dx2-y2 dz2 dxy dxz dyz
北京同步辐射装置XANES谱讲习班,2010年6月7-8日
Atomic Orbitals: A Review
d z2
d x2−y2
d xy
d yz
d xz
北京同步辐射装置XANES谱讲习班,2010年6月7-8日
例如,如果激发的内层电子是1s轨道上的电子,那么它的 初态波函数φi为偶函数,由于中间的偶极跃迁操作算符r 具有奇函数性质,因此只有当这个激发的电子的末态波函 数φf具有奇函数性质时,这个积分才不等于零。
对于单重态到三重态的跃迁,假设初态波函数 ϕkϕkαβ 为其中α和 β表示自
旋相反的自旋函数;终态波函数为 在跃迁矩阵元中将包含
ϕkϕ jα 2
或者
ϕkϕ jβ 2

∫ αβ dσ
其中dσ 为自旋坐标中的体积元。根据自旋波函数的正交性,这个积分为零,
因此单重态到三重态的跃迁是禁阻的。 而在单重态到单重态或者三重态到三重态的跃迁中,因为
但是,芯态激发的电子并不能跃迁到 所有的未占据轨道,也就是说,芯态 电子吸收一定能量的X射线光子后跃 迁到未占据轨道具有一定的选择性。
北京同步辐射装置XANES谱讲习班,2010年6月7-8日
这种选择性体现在吸收截面计算中的跃迁矩阵元中,
< φi | rK ⋅ εG | φ f >

Skyrmion

Skyrmion

SkyrmionIn particle theory,the skyrmion (/ˈskɜrmi.ɒn/)is a hy-pothetical particle related originally [1]to baryons .It was described by Tony Skyrme and consists of a quantum su-perposition of baryons and resonance states.[2]Skyrmions as topological objects are also important in solid state physics ,especially in the emerging technology of spintronics .A two-dimensional magnetic skyrmion ,as a topological object,is formed,e.g.,from a 3D effective-spin “hedgehog”(in the field of micromagnetics :out of a so-called "Bloch point "singularity of homotopy degree +1)by a stereographic projection ,whereby the positive north-pole spin is mapped onto a far-offedge circle of a 2D-disk,while the negative south-pole spin is mapped onto the center of the disk.1Mathematical definitionIn field theory,skyrmions are homotopically non-trivial classical solutions of a nonlinear sigma model with a non-trivial target manifold topology –hence,they are topological solitons .An example occurs in chiral models [3]of mesons,where the target manifold is a homogeneous space of the structure group (SU (N )L ×SU (N )RSU (N )diag)where SU (N )L and SU (N )R are the left and right parts of the SU (N )matrix,and SU (N ) ₐ is the diagonal subgroup .If spacetime has the topology S 3×R ,then classical con-figurations can be classified by an integral winding num-ber [4]because the third homotopy groupπ3(SU (N )L ×SU (N )R SU (N )diag ∼=SU (N ))is equivalent to the ring of integers,with the congruence sign referring to homeomorphism .A topological term can be added to the chiral Lagrangian,whose integral depends only upon the homotopy class ;this results in superselection sectors in the quantised model .A skyrmion can be approximated by a soliton of the Sine-Gordon equation ;after quantisation by the Bethe ansatz or otherwise,it turns into a fermion inter-acting according to the massive Thirring model .Skyrmions have been reported,but not conclu-sively proven,to be in Bose-Einstein condensates ,[5]superconductors ,[6]thin magnetic films [7]and also chiral nematic liquid crystals .[8]2Skyrmions in an emerging tech-nologyOne particular form of the skyrmions is found in mag-netic materials that break the inversion symmetry and where the Dzyaloshinskii-Moriya interaction plays an im-portant role.They form “domains”as small as a 1nm (e.g.in Fe on Ir(111)[9]).The small size of mag-netic skyrmions makes them a good candidate for fu-ture data storage solutions.Physicists at the University of Hamburg have managed to read and write skyrmions using scanning tunneling microscopy.[10]The topological charge,representing the existence and non-existence of skyrmions,can represent the bit states “1”and “0”.3References[1]At later stages the model was also related to mesons .[2]Wong,Stephen (2002).“What exactly is a Skyrmion?".arXiv :hep-ph/0202250[hep/ph ].[3]Chiral models stress the difference between “left-handedness”and “right-handedness”.[4]The same classification applies to the mentioned effective-spin “hedgehog”singularity":spin upwards at the north-pole,but downward at the southpole.See also Döring,W.(1968).“Point Singularities in Mi-cromagnetism”.Journal of Applied Physics 39(2):1006.Bibcode :1968JAP....39.1006D .doi :10.1063/1.1656144.[5]Al Khawaja,Usama;Stoof,Henk (2001).“Skyrmionsin a ferromagnetic Bose–Einstein condensate”.Nature 411(6840):918–20.Bibcode :2001Natur.411..918A .doi :10.1038/35082010.PMID 11418849.[6]Baskaran,G.(2011).“Possibility of Skyrmion Superconductivity in Doped Antiferromagnet K$_2$Fe$_4$Se$_5$".arXiv :1108.3562[cond-mat.supr-con ].[7]Kiselev,N.S.;Bogdanov,A.N.;Schäfer,R.;Rößler,U.K.(2011).“Chiral skyrmions in thin magnetic films:New objects for magnetic storage technologies?".Journal of Physics D:Applied Physics 44(39):392001.arXiv :1102.2726.Bibcode :2011JPhD...44M2001K .doi :10.1088/0022-3727/44/39/392001.[8]Fukuda,J.-I.;Žumer,S.(2011).“Quasi-two-dimensional Skyrmion lattices in a chiralnematic liquid crystal”.Nature Communica-tions 2:246.Bibcode :2011NatCo...2E.246F .doi :10.1038/ncomms1250.PMID 21427717.123REFERENCES [9]Heinze,Stefan;Von Bergmann,Kirsten;Menzel,Matthias;Brede,Jens;Kubetzka,André;Wiesen-danger,Roland;Bihlmayer,Gustav;Blügel,Ste-fan(2011).“Spontaneous atomic-scale magneticskyrmion lattice in two dimensions”.Nature Physics7(9):713–718.Bibcode:2011NatPh...7..713H.doi:10.1038/y summary(Jul31,2011).[10]Romming,N.;Hanneken, C.;Menzel,M.;Bickel,J. E.;Wolter, B.;Von Bergmann,K.;Kubet-zka, A.;Wiesendanger,R.(2013).“Writing andDeleting Single Magnetic Skyrmions”.Science341(6146):636–9.Bibcode:2013Sci...341..636R.doi:10.1126/ysummary–(Aug8,2013).3 4Text and image sources,contributors,and licenses4.1Text•Skyrmion Source:/wiki/Skyrmion?oldid=637550141Contributors:Michael Hardy,Charles Matthews,Phys, Icairns,Lumidek,Pjacobi,Jag123,Fwb22,Rjwilmsi,Conscious,Wikid77,Headbomb,Lincoln F.Stern,Tarotcards,KylieTastic,Pix-elBot,Doprendek,Addbot,Luckas-bot,Yobot,Citation bot,Obersachsebot,Omnipaedista,Citation bot1,Merongb10,Meier99,Korepin, EmausBot,JSquish,ZéroBot,StringTheory11,AManWithNoPlan,Isocliff,Parcly Taxel,Bibcode Bot,BattyBot,ChrisGualtieri,Andy-howlett,1andreasse,Nicohoho,NorskMaelstrom,Noah Van Horne and Anonymous:74.2Images•File:Portal-puzzle.svg Source:/wikipedia/en/f/fd/Portal-puzzle.svg License:Public domain Contributors:?Original artist:?4.3Content license•Creative Commons Attribution-Share Alike3.0。

基于混沌模拟退火法的非线性马斯京根模型参数率定方法

基于混沌模拟退火法的非线性马斯京根模型参数率定方法

P ARAM E TER l T眦
- oN ETHoD I 1 I oF NoNLI NEAR U KI M S NG UM oDEL M
BS ED AS oN CHAo s—・ndJ A E ANNEA NG 【 H oD . S 【I Ic l 1D LI lI i
基 于 混 沌 模 拟 退 火 法 的 非 线 性 马 斯 京 根 模 型 参 数 率 定 方 法
程银 才 , 左 欣
( 山东农业 大学水利土木 3程学院 , - 山东 泰安 2 1 1 ) 7 0 8
摘要 : 文在分析一些 已有 的马斯京 根模 型参数率定方法 不足之 处 的基 础上 , 出 了一种基 于混沌 模拟退 火法 的 本 提 非线性马斯京 根模 型率 定的新方法 , 同其 它方法相 比 , 该法具有求解精度高 、 计算速度 快 以及适 应性强 的特点 。最
Ab t a t On t e b sso n l ssmeh d t e o a a tre t t n o s i g m d l h sp p rp e e t s r c : h a i f ay i t o fp rmee si i fMu k n u mo e ,t i a e r s n a h ma o a n w meh d o a a tr e t t n o s i g m d lb s d o h o e t o fp r mee si i fMu k n u mo e a e n c a s—smu a e n e l g me h d B o ma o i l td a n a i t o . y c m- n p r g wi h t e t o s h to a h r c e s c f ih p e iin ,f s p e n o s b l y a i t t e oh rmeh d ,t e meh d h s c aa tr t so r c s n h i i hg o a ts e a d s e u a i t . d d i

Chiral symmetry breaking in the Wegner-Houghton approach

Chiral symmetry breaking in the Wegner-Houghton approach

a rXiv:h ep-ph/6169v115J un21Chiral symmetry breaking in the Wegner-Houghton RG approach A.Bonanno a and D.Zappal`a b ∗a Osservatorio Astrofisico di Catania,Via S.Sofia 58,I-95125,Catania INFN,Sezione di Catania,Corso Italia 57,I-95129,Catania b INFN,Sezione di Catania and Dip.to di Fisica e Astronomia,Universit`a di Catania,Corso Italia 57,I-95129,Catania,Italy The Wegner-Houghton formulation of the exact renormalization group evolution equa-tion is used in order to study the chiral symmetry breaking of the linear σ-model coupled to an isospin doublet of quarks.A numerical investigation for a particular truncation of the equation which includes the scalar field renormalization function is presented.1.INTRODUCTION The full understanding of the phase structure of QCD as the theory of strong inter-actions has become an important issue since the discovery of asymptotic freedom.The possibility that high temperature QCD could show different properties from the theory at zero temperature has been addressed already in [1].New features are also predicted for the theory at very high and intermediate baryon density [2],[3,4].An essential role is played by the Chiral Symmetry which is supposed to be broken by the vacuum structure of the theory.Thus,before considering the high temperaturephase transition with the Chiral Symmetry restoration,one has to deal with the problem of determining a nonzero order parameter which indicates the Chiral Symmetry Breaking (CSB)at zero temperature and density.A strong simplification is obtained by considering the effective theory described by a linear σmodel of scalar mesons coupled to an isospin multiplet of fermions with the same chiral symmetry group of the original action.Then CSB corresponds to a mexican hat-shaped effective potential and the order parameter is identified with the vacuum expectation value (VEV)of one of the scalar fields.The infrared (IR)properties of a field theory such as the vacuum structure,can be analysed by means of the wilsonian renormalization group which generates a sequence of effective actions defined at some momentum scale k ,starting from the original action,by integrating out in the latter all the modes with frequency higher than k .This leads to the construction of a differential flow equation for the k -dependent action,generally known as Exact Renormalization Group Equation (ERGE).In the past years many analytical and numerical approaches to the ERGE,applied to various theories,have been developed.Two recent extensive reviews of this topic are [5,6]and a detailed ERGE analysis of the Chiral Phase Transition can be found in [7–10].2Here we shall consider just the simple case of the CSB at zero temperature employing the sharp cut-offversion of the ERGE,namely the Wegner-Hougton equation[11].The cut-offdependence of the ERGE for the O(4)linearσ-model has been addressed in[12]where, however only theflow of the scalar potential is considered while the Yukawa coupling is keptfixed.In addition to the Yukawa couplingflow,we are particularly interested in the behavior of thefield renormalization.In fact,if our model is really an effective theory which,at some scale,can naturally replace the original QCD action,then at this scale one expects the formation of the mesonic bound states characterized by a very small wave function renormalization function.The reduction of QCD to the quark-meson action has been analysed before and a review of it is given in[10].As expected the value of the scalar field renormalization is vanishingly small at the mesonic bound state formation scale which is found between0.60and0.63GeV.Then,theflow of thefield renormalization deserves particular attention.2.ANALYSIS AND RESULTSThe explicit form of the euclidean action at a scale k is(ρ≡σ2+ π2)S k= d4x z l k2∂µ π∂µ π+U k(ρ)+N c c¯ψc(iγ·∂+g kσ+ig kγ5 π τ)ψc (1)ψc is aflavor doublet and the summation over the index c is extended to N c colors.No CSB fermion mass term is included and the action is fully invariant under chiral trans-formations.The presence of CSB depends on the shape of the O(4)symmetric potential U k in the limit k→0.z l k and z t k are theσandπrenormalization functions.As long as U k has zero vacuum expectation value(VEV),we choose the following parametriza-tion U k=(1/2)m2kρ+(λk/24)ρ2and consider theflow of the two parameters m2k andλk neglecting all the irrelevant operators that could be generated during theflow.In the presence of a nonvanishing VEV¯ρk,according to[12],we reparametrize the potential in terms of¯ρk andλk,recalling that m2k can be expressed in term of these two parameters through the minimum condition.The purpose of this double choice is practical,we take the couple of parameters which corresponds to the simplest set offlow equations.The Wegner-Houghton equation can be reduced to a set of coupled ordinary differential equations for the k dependent parameters in(1),i.e.g k,z l k,z t k,λk and m2k or¯ρk.In particular the equations for the parameters in the potential are deduced in[12],and the one for g k can be obtained by an analogous procedure.The equations for z l k,z t k, (which coincide as long as¯ρk=0,according to the chiral simmetry)are deduced following the procedure formulated in[13]and already implemented in[14].In the following,the derivatives of z l k and z t k w.r.t.thefields,which are supposed to be small,are neglected. The pion decay constant and the constituent fermion mass are two IR constraints for our equations.In fact,in the limit k→0we have√¯ρk≡M→M q∼0.3GeV,as initial conditions for the equations.If we start, according to[10],theflow at the UV scale k=0.6GeV with a convex potential(m2k>0), then at a certain scale Kχ,m2k becomes negative generating a nonzero¯ρk.In the following the three remaining initial conditions imposed are¯ρk=0at the CSB scale Kχand a particular value for z l k at the UV scale(the symmetry requires z l k=z t k at the UV scale).30.300.400.500.60k (GeV)0.000.200.400.60(G e V )M f mm Figure 1.RG flow with two different setsof initial conditions (see text).For thesetwo sets,the quark mass M and the de-cay constant f are displayed below K χ=0.43GeV ,and the scalar mass m above K χ.0.3700.3900.4100.430Κχ −6.0−5.0−4.0−3.0−2.0−1.00.0∆ (%)Figure 2.100×∆(see text)vs.K χ(GeV)for two different values of M q .M q =0.30GeV (solid)and M q =0.33GeV (dashed).Figure 1shows,above K χ(fixed at the value K χ=0.43GeV),the flow of the scalar mass m (the subscript k is omitted)for two different initial values of z l (=z t )and,below K χ,the corresponding f and M .The curves for f and M in the two cases are almost superposed indicating insensitivity to the UV condition on z l .The value of K χis suggested by an IR stability criterion.In order to use a particular value of quark mass,M q ,as the initial condition for the running quantity M defined above,M must be practically flat around k =M q .The same criterion should apply to f πbut,since f πis smaller than M q ,we find that f at the scale k =f πis already a stable parameter.After fixing the IR condition M (k =M q −ǫ)=M q with ǫ=0.03GeV,we have considered the ratio ∆=(M (k =M q )−M q )/M q ,plotted vs.K χin Figure 2for two different values of M q .The stability requirement indicates that K χshould not be smaller than ∼0.4Gev.In Figures 3and 4the other running parameters are displayed for the same two initial values of z l that have been used in Figure 1.It should be noted the small running of g and λ,in the range of k considered,and their large values which are clearly nonperturbative.As shown in Figure 4,when going from the UV to the IR scale,the field renormalizations grow and,below K χ,z l and z t increase differently.Since reasonably we expect,for the pion physics at scales around k =0.3GeV,field renormalization functions close to the unity,we must require very small values at k =ly we used z l =z t =0.1and z l =z t =0.01in the two cases here considered in Figures 1,3,4.Higher curves for m,λ,g correspond to the former case,lower curves to the latter.The approximation here employed for the ERGE has been sufficient for exploring a nonperturbative region (note that,as explained in [10],the renormalized couplings which include the field renormalization effect,are larger than those in Figure 3)and it has40.300.400.500.60k (GeV)0.00.51.01.5zlztFigure 3.Flow of z l (solid)and z t (dashed)for two different sets of initial data (seetext).z l and z t coincide above K χ=0.43.0.300.400.500.60k (GeV)0.05.010.0gλ/24Figure 4.Flow of the scaled scalar quartic coupling λ/24(solid)and of the Yukawa coupling g (dashed)for two different setsof initial data (see text).yielded a very small (vanishing)scalar field renormalization around 0.6GeV.We hope to extend our analysis to the finite temperature case.REFERENCES1.J.C.Collins and M.J.Perry,Phys.Rev.Lett.34(1975)1353.2.D.Bailin and A.Love,Phys.Rep.107(1984)325.3.M.Alford,K.Rajagopal and F.Wilczek,Phys.Lett.422B (1998)247.4.R.Rapp,T.Shafer,E.V.Shuryak and M.Velkovsky,Phys.Rev.Lett.81(1998)53.5.C.Bagnuls and C.Bervillier,Exact renormalization group equations.An introductory review,Preprint e-Print Arch.:hep-th/0002034,Feb 2000.6.J.Berges,N.Tetradis,C.Wetterich,Nonperturbative renormalization flow in quan-tum field theory and statistical physics,Preprint MIT-CTP-2980,HD-THEP-00-26,e-Print Arch.:hep-ph/0005122,May 2000.Submitted to Phys.Rep.7.J.Berges,N.Tetradis and C.Wetterich,Phys.Rev.Lett.77(1996)873.8. D.-U.Jungnickel and C.Wetterich,Phys.Rev.D53(1996)5142.9.J.Berges,D.-U.Jungnickel and C.Wetterich,Phys.Rev.D59(1999)034010.10.J.Berges,QCD in extreme conditions and the wilsonian exact renormalization group,Preprint MIT-CTP-2829,e-Print Arch.:hep-ph/9902419.11.F.J.Wegner and A.Houghton,Phys.Rev.A8(1972)401.12.G.Papp,B.J.Schaefer,H.J.Pirner and J.Wambach,Phys.Rev.D61(2000)096002.13.C.Fraser,Z.Phys.C28(1985)101.14.A.Bonanno and D.Zappal`a ,Phys.Rev.D56(1997)3759.。

Pion and Eta Strings

Pion and Eta Strings

a r X i v :h e p -p h /9711452v 1 24 N o v 1997November 1997Pion and Eta StringsXinmin Zhang 1,Tao Huang 1and Robert H.Brandenberger 21Institute of High Energy Physics,Academia Sinica,Beijing 100039,China 2Department of Physics,Brown University,Providence,IR 02912,USA ABSTRACT In this paper we construct a string-like classical solution,the pion-string,in the linear sigma model.We then study the stability of the pion-string,and find that it is unstable in the parameter space allowed experimentally.We also speculate on the existance of an unstable eta-string,associated with spontaneous breakdown of the anomalous U A (1)symmetry in QCD at high temperatures.The implications of the pion and eta strings for cosmology and heavy ion collisions are briefly mentioned.BROWN-HET-1103Strings,as classical solutions in theories with spontaneously broken symmetries,play an important role in both particle physics and cosmology.Thus it is of crucial importance to know if strings can exist in realistic models of strong and electroweak interactions.Recently, in an inspiring paper,Vachaspati[1]showed that string-like structures exist in the standard model of electroweak theory.In this paper,we will consider strings in models with spon-taneously broken chiral symmetry of QCD.First of all,we explicitly construct a classical solution,the pion string,in the linear sigma model,and then argue for the existence of an eta string at high tempratures.In recent years,the SU L(2)×SU R(2)∼O(4)linear sigma-model has been often used as a model of hadron dynamics for chiral symmetry breaking in QCD,in particular in studies of the physics associated with the chiral phase transition[2]and of the disoriented chiral condensates[3]in heavy ion collisions.The lagrangian density of this model isL=12(∂µ π)2−λ√√2)2.(4)During chiral symmetry breaking,thefieldφtakes on a nonvanishing vacuum expectation value,which breaks SU L(2)×SU R(2)down to SU L+R(2).This results in a massive sigma and three massless Goldstone bosons.In addition,we will demonstrate below that there is a static unstable string-like solution,the pion-string.For static configurations in eq.(4),the energy functional is given byE= d3x ▽φ∗ ▽φ+ ▽π+ ▽π−+λ(π+π−+φ∗φ−f2π2)φ,(6)▽2π+=2λ(π+π−+φ∗φ−f2πThe pion string solution extremising the energy functional in eq.(5)is given byφ=fπ2ρ(r)e inθ,(8)π±=0,(9)where the coordinates r andθare polar coordinates in the x−y plane,and the integer n is the winding number.In the following discusion,we will restrict ourselves to n=1.Substituting(8)into(6),we obtain the equation of motion forρ(r),1∂r (r∂r2ρ(r)=λf2π(ρ2−1)ρ(r).(10)The boundary conditions forρ(r)arer→0,ρ(r)→0;(11)r→∞,ρ(r)→1.(12)In principle,ρ(r)can be determined numerically by solving Eq.(10)with boundary con-ditions in(11)and(12).But it is simpler to adopt a variational approach.Following the method of Hill,Hodges and Turner[5],we make an ansatz of the following form:ρ(r)=(1−e−µr),(13)whereµis a variational parameter.Adopting expression(13)as a variational ansatz,it follows that the energy per unit lengthof the string isE(pion−string)=1289µ2,(14)where Iθ(µ,R)= ∞0dr∂µ|R→∞=1144f2π.(16)Substituting(16)into(14),the mass of the pion-string per unit length isE(pion−string)= 34+ln(µR) πf2π.(17) The pion-string is not topologically stable,since anyfield configuration can be contin-uously deformed to the vacuum.To study the stability of the pion-string,we consider infinitesimal perturbations of thefieldπ±and check if the variation in the energy is positive or negative.Discarding terms of cubic and higher orders inπ±,wefindE=E(pion−string)+δE,(18) whereδE= d3x ▽π+ ▽π−+λf2π(ρ2−1)π+π− .(19) Following Ref.[4],we consider an expansion of theπ±fields in Fourier modes,π+=χm(r)e imθ.(20) Inserting the expressions for the m-th mode ofπ±in eq.(19)givesδE= 2πrdr (∂χm r2χ2m+λf2π(ρ2−1)χ2m ,(21) where thefirst term(the kinetic energy part)and the second term are always positive,but the third term,the potential energy,is negative.Notice that the second term gives the smallest contribution to the positive energy inδE for m=0,so we will focus on m=0.Definingξ=fπr,χ=fπR,and setting m=0,δE becomes:δE=2πf2π ξdξ(∂Rξ∂∂ξ)+λ(ρ2−1).(24)The question of stability of the pion-string reduces to checking if the eigenvalues of the oper-atorˆO in its spectrum are negative,subject to the eigenfunction R satisfying the boundary conditions R(ξ→0)→constant,and R(ξ→∞)→0.To simplify the analysis,we take a variational approach,making use of an ansatz of the form[5],R=σ0e−κξ(1+κξ+κ1ξ2+κ2ξ3),(25)whereσ0,κ,κ1,κ2are dimensionless variational parameters.This ansatz has the correct short-distance limit andκ−1represents the size of theπ±condensate on the pion-string. By inserting(25)into(23)it is obvious that the negative term wins out ifλ≥1.This implies that the pion-string is unstable in the parameter space allowed experimentally(λ∼10−20[2]).It can be shown by numerical analysis thatδE is positive only for very small values ofλ(λ≤10−8),and hence the pion-string is only stable for these values.In the early universe and in heavy-ion collisions,pion strings are expected to be produced and to subsequently decay.Their lifetime can be estimated by considering their interactions with the surrounding plasma.Based on a naive dimensional analysis,their lifetimeτshould be proportional to the inverse of the corresponding temperature.For strongly interacting theory such as the linear sigma model studied here,we expect thatτ=O(1)T−1,where T is the temperature at the time when the chiral symmetry of QCD is restored.Before concluding,let us speculate about the existence of an unstableηstring.In QCD, in the limit of massless quarks,there is an additional U A(1)chiral symmetry.This chiral symmetry,when broken by the quark condensate,predicts the existence of a goldstone boson. There is no such a light meson,however.This is resolved by the Adler-Bell-Jackiw U A(1) anomaly together with the properties of non-trival vacuum structure of non-abelian gauge theory,in particular QCD.The U A(1)symmetry is badly broken by instanton effects at zero temperature.As the density of matter and/or the temperature increases,it is expected that the instan-ton effects will rapidly disappear[6],and one thus has an additional U A(1)symmetry(besides SU L(2)×SU R(2))at the transition temperature of the QCD chiral symmetry.When the U A(1)symmetry is broken spontaneously by the quark condensate,a topological string,the η-string,results.Differing from the pion-string,theη-string is topologically stable at high temperatures,but will decay as the temperature decreases.Theη-string can form during the chiral phase transition of QCD.In the setting of cosmology,it will exist during a specific epoch below the QCD chiral symmetry breaking temperature during the evolution of the universe.In the context of heavy-ion collisions,it will exist in the plasma created by the collision during a period shortly after the cooling of the interaction region below the sym-metry breaking scale.The strings then become unstable as the temperature decreases and when the instanton effects become substantial.AcknowledgementsWe thank Jin Hong-Ying and Cao Jiun-Jer for discussions and help in the numerical calculation.This work was supported in part by National Natural Science Foundation of China and by the U.S.Department of Energy under Contract DE-FG0291ER40688.References[1]T.Vachapati,Phys.Rev.Lett.68,1977(1992);Nucl.Phys.B397,648(1993).[2]For example,see,R.D.Pisarski,”Applications of Chiral Symmetry”(hep-ph/9503330).[3]K.Rajagopal and F.Wilczek,Nucl.Phys.B379,395(1993);B404,577(1993).[4]M.James,L.Perivolaropoulos,and T.Vachaspati,Nucl.Phys.B395,534(1993).[5]C.T.Hill,H.M.Hodges and M.Turner,Phys.Rev.D37,263(1988).[6]R.D.Pisarski and F.Wilczek,Phys.Rev.D29,338(1984);E.Shuryak,Comm.Nucl.Part.Phys.21,235(1994),and refs therein;J.Kapusta,D.Kharzeev and L.McLerran,Phys.Rev.D53,5028(1996).。

data-quality

Making the most of your observations – data quality Of symmetry, scaling and mergingCharles Ballard (original by Johan Turkenburg,alterations by Andrey Lebedev and CharlesBallard)As progress more information is available1. Include all data2. Resolution cutoff3. Exclude batches4. Review symmetryDepends on the question you ask What to look out for, depends on what you need (user perspective):▪Native data▪Atomic resolution▪Anomalous data▪(Putative) complexIn general, look at results (map, structure solution)Why you should review data quality! Opportunity to assess experiment, and prepare forstructure solution and refinementAssessment of experiment, data qualityAssessment of resulting data, statistical properties – intensity distributions Tables and GraphsR-factorsCC½ Pearson's CorrelationCoefficientIn practice:Divide (equivalent) observations in two random sets, and calculate CC1/2Works on unmerged data.Accuracy and Precision Inaccurate but precise Accurate but not preciseVsSigma (σ)As in all experiments, observations have a σ (standard deviation)From integration programs – not always very good.Corrected by looking at spread of equivalent observations around the mean. Effected by multiplicity.Measure precision.Sigma correctionThe error estimate from the integration program (poisson or guassian less background) is generally too small. A “corrected” value may be estimated by increasing it for large intensities such that the mean scatter of scaled intensities equals σ'(I), in all intensity ranges.σ'(|h|)2 = Sdfac2 [ σ2 +SdB<Ih> + (SdAdd<Ih|>)2]I/sig(I) vs resolutionIntegrationUnit cell needed, lattice ‘optional’Integration uses a unit cell (and depending on program it may add constraints on the parameters based on crystal lattice) and missets to determine where the spots are that need to be integrated.Only shape of unit cell (crystal system) is known, not point or space group!Can use DIALS, XDS, HKL, etc.We then have a set of observations, these need to be scaled and merged.Determine spacegroupPointless in CCP4, xscale in xds.From the cell dimensions, determine the maximum possible lattice symmetry, with some tolerance (ignores input symmetry).For eash possible rotation operator, score potentially related observation pairs for agreement (CC and R-factor)Score all possible combinations of operators to determine the point group (PGs from the maximum down to P1).Score axial systematic absences to detect screw axes, hence space group (NB sometimes these are unobserved, or ambiguous).Pointless in CCP4, xscale in xds.Rotational symmetry encoded indiffraction pattern Intensities obey rotational symmetryandSymmetry determined from intensitiesPointless output in ccp4i2 data reduction task or via xia2Important tables and graphs for a P62?2?datasetView down 6-foldAlways worth checking in hklview ordials.reciprocal_lattice_viewer toconfirmLayer k=1Table of CC for symmetry relatedreflectionsCC and R-factor withconfidence level indicated*** confident** reasonably confident* not confidentShould compare levels of CCs andR-factors for operators associatedwith space group.Plot of systematic absences along 6-fold (c-axis) 00ll=6l=12Pointless result P63Deposited structure P61Look at individual operators, compare agreement ●because we compare within dataset, Rmerge is ok to use●Example: P3112 or P31●Compare Rmerge for 3-fold and 2-folds●Pointless gives P3112 as most likely spacegroupPseudo (incorrect) symmetryAlternative settings (indexing)If the true point group is a lower symmetry than the lattice group, alternative valid, but non-equivalent indexing schemes are available. These are related by symmetry operations present in the lattice group but not in the point group.●In space group P3 (or P31) there are 4 different schemes:●(h,k,l), (-h,-k,l), (k,h,-l) or (-k,-h,-l)Note: this is also the case where merohedral twinning is possibleCCPI2 output says: “You will have to resolve the enantiomorphic ambiguity later”This occurs for e.g.:●P61 / P65●P62 / P64●P41 / P43Enantiomorphic Space GroupsExample 41 and 43Space Group CheckThe space group is a hypothesis until the structure has been solved and refined. Checking the space group:●Molecular replacement in all space groups with same point group (balbes, and phaser do this)●Refinement in lower space groups, even P1 (zanuda will do this, but does not remerge the data – see ccp4online).ScalingAimless in CCP4, xscale in xds.Why needed? Decay, beam instability, shutter (not any more), detector dead time, detector characteristics, illuminated volume (beam smaller than crystal), absorption, etc.(simple) two parameter scale model: k & B.Maximise effectiveness:●High multiplicity●Low (enough) dose●Multiple settings (especially for low symmetry)●Low background scatter and good centringDiffraction, fall off with resolutionTypical imageSpot intensity andbackground drop as movefrom beam centre to theimage edges, and hencewith resolution. This canbe modelled with B.ResolutionI n t e n s i t y Simple illustration of why scaling is needed.Time of sweep, need to put all observations on commonscale (k)Scales and B-factor vs BatchScales vs. rotation range (batch)B-factor vs rotation range (batch)Scales and B-factor for decayingScales vs. rotation range (batch)B-factor vs rotation range (batch)MergingMultiple observations, because there are symmetry equivalents, or you have collected many degrees of data, or both.Determine mean for every reflection, reject outliers.More useful plots to monitor state of dataeg Rmerge vs batch (film, image)Analysis vs batchRmerge vs batch consistent. This is good.Rmerge vs batch increases for later images. Radiation damage?Must always be prepared to reject images. Often a trade of with completeness.Look at analysis against batchBad patches and anisotropy (disorder) often correlated, rejecting the worst part of dataset often leads to incomplete data.Rejecting Images and CompletenessCumulative completenessThe useful resolution of the data depends on what the data is to be used for. On square detectors integrate into corners ●Traditionally <I/sigI> > 3 (none ML stats)●Aimless suggests <CC 1/2> > 0.3●EM uses <CC 1/2> > 0.14●ML techniques down weight poor data.Resolution cut-offCC 1/2vs resolutionTwo other indicators of an overly optimistic resolution are the●Moments plots●Will see break down of expectedbehaviour, eg acentric 2nd moment >> 2●Wilson plot (see later)●Often see observed data is deviatessignificantly above ideal plotResolution cut-offSecond moment vs resolutionEffect of removing poor dataCC1/2, scaling, L-test and moments 1/2, scaling, L-test and moments after.Diffraction fall-off with resolution.ln(<F2obs >) = -2Bsin2θ/λ2..k.ln(<F2ref>)The “global temperature” effect on thedata. <F2ref> can be atomic scatteringfactors, or experimentally derivedscattering (cf BEST)●Provides absolute scale and isotropicthermal parametersGood wilson plot, but still deviates at lowresolutionexpected values.●Ice rings●Integration into noiseThe computed B-factor can be used togive an alternative resolution estimate.The optical resolution, a measure of theuseful data range.v. bad wilson plot, missing low resolution andflat at high resolutionAnisotropyDiffraction falls with resolutionincrease, but not necessarily in anisotropic manner.Aimless Anisotropic CC1/2Dials reciprocal_lattice_viewerAnisotropy – other ways to seeData reduction warnings.Anisotropy matrix, directional B-valuesDirectional intensity vs resolution plot●Low level anisotropy will have little effect ●Intermediate level can lead to density sausages – density poorly resolved in one or more directions ●Anisotropic correction ●Shown to work for MR (in programs)●Not applied in refinement (I/sigI has all information)●Useful tool staraniso from global phasing ●Non-spherical truncations ●Highly anisotropic●Very difficult to handle Anisotropy – merged data Anisotropy – effectAnisotropy – effectAnisotropy – merged dataTwinningTwo or more crystals of the same species joined together in different orientations.I 1+2 = αI1+ (1-α)I2α is the twin fractionThe twin law (twin operator) is the operator between the conjoined crystals, effectively an additional symmetry operator.●This type of twinning cannot be NOT recognised by inspection of the images●All spots overlap with related spots from another individual crystal ●Detection requires analysis of intensity statistics●Significant effect on model if ignored in refinement●Point group, and consequently space group determination may be a problem=lattice in orientation 1lattice in orientation 2≠crystal in orientation 1crystal in orientation 2+=Twinned crystal crystal in orientation 1crystal in orientation 2Merohedral twinTwin law: Symmetry operator of the crystal system, but not the crystal‘s point groupPseudo-Merohedral twinTwin law: Belongs to a higher crystal system than the structure.Twintwo-fold axisCrystallographic two-fold axisUnit cellTwinned crystalIndividual crystal 1Individual crystal 2Example: P2, β = 90Twin two-fold axisCrystallographic two-fold axisIntensities from individual crystal 1Intensities fromindividual crystal 2Partial twin (individual crystal of different size)Perfect twin (individual crystal of equal size)hlk=0P121, β = 90fewer weak reflectionsAnisotropy – effect Anisotropy – merged data Twinning Analysis•Presence:–intensity statistics•Space group symmetry of a single domain:–structure solutionPerfect twinning by(pseudo)merohedryP222P211P121P112Anisotropy – effectAnisotropy – merged dataTwinning Analysis - L-test J 1J 2L = | J 1 – J 2 | / ( J 1 + J 2 )L-test is designed to be suitable for most of cases- reflections close to each other in reciprocal space - with and without pseudo-translation (offset)- isotropic and anisotropic dataAnisotropy – effectAnisotropy – merged data Theoretical distribution of L-test P (L )L 0.00.5 1.00.00.51.0Single crystal0.00.51.00.00.51.0L P (L)Partial twinP (L )0.00.5 1.00.00.51.0LPerfect twinAnisotropy – effectAnisotropy – merged data Twinning Analysis - H-test J 1J 2H = | J 1 – J 2 | / ( J 1 + J 2 )H-test: reflections J 1 and J 2 related by the twin operatorCumulative distribution for H-test Anisotropy – merged dataAnisotropy – effect Array H-test: (for acentric reflection)Cumulative probability distribution:0 H<0{N(H) = H/(1-2α) 0≤H≤1-2α1 H>1-2αNote: rotation parallel to twinningaxes causes the distribution to bediferent, by further mixing ofintensitiesAnisotropy – effectAnisotropy – merged data Twinning and space groups Twinning by(pseudo)merohedry is impossible432622234226323222421Twinning by merohedry ●higher lattice symmetry is determined by crystal symmetryTwinning by pseudomerohedry ●specialised unit cell parameterssupergroup (lattice)subgroup (crystal)Anisotropy – effectCCP4i2 twinning testsAnisotropy – merged dataThe data reduction task runsseveral twinning tests includingthe L-test, H-test, moments, andML-Britton test.●These give an indication thatthe intensity statistics areconsistent with twinning.Anisotropy – effectAnisotropy – merged data Refinement of twinned data Model error R -f a c t o r0.60.50.40.30.20.10.00.0 1.00.80.60.40.2Model error0.60.50.40.30.20.10.00.01.00.80.60.40.2Twinned crystalSingle crystalOnOnOffOff。

Conditionalindependence

Conditional independenceThese are two examples illustrating conditional independence. Each cell represents a possible outcome. The events R, B and Y are represented by the areas shaded red, blue and yellow respectively. And the probabilities of these events are shaded areas with respect to the total area. In both examples R and B are conditionally independent given Y because: \Pr(R \cap B \mid Y) = \Pr(R \mid Y)\Pr(B \mid Y)\,To see that this is the case,one needs to realise that Pr(R ∩ B | Y) is the probability of an overlap of R and B in the Y area. Since, in the picture on the left, there are two squares where R and B overlap within the Y area, and the Y area has twelve squares, Pr(R ∩ B | Y) = \tfrac{2}{12} =\tfrac{1}{6}. Similarly, Pr(R | Y) = \tfrac{4}{12} = \tfrac{1}{3} and Pr(B | Y) =\tfrac{6}{12} = \tfrac{1}{2}.but not conditionally independent given not Ybecause:\Pr(R \cap B \mid \text{not } Y) \not= \Pr(R \mid \mbox{not } Y)\Pr(B \mid\text{not } Y).\,In probability theory, two events R andB are conditionally independentgiven a third event Y precisely if theoccurrence or non-occurrence of R andthe occurrence or non-occurrence of Bare independent events in theirconditional probability distributiongiven Y . In other words, R and B areconditionally independent if and onlyif, given knowledge of whether Yoccurs, knowledge of whether R occursprovides no information on thelikelihood of B occurring, andknowledge of whether B occursprovides no information on thelikehood of R occurring.In the standard notation of probabilitytheory, R and B are conditionallyindependent given Yif and only ifor equivalently,Two random variables X and Y are conditionally independent given a third random variable Z if and only if they are independent in their conditional probability distribution given Z . That is, X and Y are conditionally independent given Z if and only if, given any value of Z , the probability distribution of X is the same for all values of Y and the probability distribution of Y is the same for all values of X .Two events R and B are conditionally independentgiven a σ-algebra Σ ifwhere denotes the conditional expectation of the indicator function of the event , , given the sigma algebra. That is,Two random variables X and Y are conditionally independent given a σ-algebra Σ if the above equation holds for all R in σ(X ) and B in σ(Y ).Two random variables X and Y are conditionally independent given a random variable W if they are independent given σ(W ): the σ-algebra generated by W. This is commonly written:This is read "X is independent of Y, given W"; the conditioning applies to the whole statement: "(X is independentof Y) given W".If W assumes a countable set of values, this is equivalent to the conditional independence of X and Y for the events of the form [W = w]. Conditional independence of more than two events, or of more than two random variables, is defined analogously.The following two examples show that X⊥Y neither implies nor is implied by X⊥Y | W. First, suppose W is 0 with probability 0.5 and 1 otherwise. When W = 0 take X and Y to be independent, each having the value 0 with probability 0.99, the value 1 otherwise. When W = 1, X and Y are again independent, but this time they take the value 1 with probability 0.99. Then X⊥Y | W. But X and Y are dependent, because Pr(X = 0) < Pr(X = 0|Y = 0). This is because Pr(X = 0) = 0.5, but if Y = 0 then it's very likely that W = 0 and thus that X = 0 as well, so Pr(X = 0|Y = 0) > 0.5. For the second example, suppose X⊥Y, each taking the values 0 and 1 with probability 0.5. Let W be the product X×Y. Then when W = 0, Pr(X = 0) = 2/3, but Pr(X = 0|Y = 0) = 1/2, so X ⊥ Y | W is false. This also an example of Explaining Away. See Kevin Murphy's tutorial [2] where X and Y take the values "brainy" and "sporty".Uses in Bayesian statisticsLet p be the proportion of voters who will vote "yes" in an upcoming referendum. In taking an opinion poll, one chooses n voters randomly from the population. For i = 1, ..., n, let Xi= 1 or 0 according as the i th chosen voter will or will not vote "yes".In a frequentist approach to statistical inference one would not attribute any probability distribution to p (unless the probabilities could be somehow interpreted as relative frequencies of occurrence of some event or as proportions ofsome population) and one would say that X1, ..., Xnare independent random variables.By contrast, in a Bayesian approach to statistical inference, one would assign a probability distribution to p regardless of the non-existence of any such "frequency" interpretation, and one would construe the probabilities as degrees of belief that p is in any interval to which a probability is assigned. In that model, the random variablesX 1, ..., Xnare not independent, but they are conditionally independent given the value of p. In particular, if a largenumber of the X s are observed to be equal to 1, that would imply a high conditional probability, given that observation, that p is near 1, and thus a high conditional probability, given that observation, that the next X to be observed will be equal to 1.Rules of conditional independenceA set of rules governing statements of conditional independence have been derived from the basic definition.[3][4] Note: since these implications hold for any probability space, they will still hold if considers a sub-universe by conditioning everything on another variable, say K. For example, would also mean that.Note: below, the comma can be read as , and thus can be visualized as a Venn Diagram.SymmetryDecompositionProof:•(meaning of )•(ignore variable by integrating it out)•repeat proof to show independence of X and B .Weak unionContractionContraction-weak-union-decomposition Putting the above three together, we have:IntersectionIf the probabilities of X, A, B are all positive, then the following also holds:References [1]To see that this is the case, one needs to realise that Pr(R ∩ B | Y ) is the probability of an overlap of R and B in the Y area. Since, in the pictureon the left, there are two squares where R and B overlap within the Y area, and the Y area has twelve squares, Pr(R ∩ B | Y ) == .Similarly, Pr(R | Y ) = = and Pr(B | Y ) = = .[2]http://people.cs.ubc.ca/~murphyk/Bayes/bnintro.html[3]Dawid, A. P. (1979). "Conditional Independence in Statistical Theory". Journal of the Royal Statistical Society Series B 41 (1): 1–31.MR0535541. JSTOR 2984718.[4]J Pearl, Causality: Models, Reasoning, and Inference, 2000, Cambridge University PressArticle Sources and Contributors4Article Sources and ContributorsConditional independence Source: /w/index.php?oldid=418113252 Contributors: 3mta3, Alansohn, AzaToth, Brighterorange, Btyner, Cesarth, Charles Matthews,Circeus, Citrus Lover, DGJM, Ddxc, Dominus, Duoduoduo, Epachamo, Fresheneesz, Gareth Owen, Giftlite, Jeff G., Mackseem, Melcombe, Michael Hardy, Ms2ger, Mtcv, Nasz, Neilc,Ninjagecko, Ogai, Oleg Alexandrov, Pr.elvis, Qwfp, Redrocket, Rkashuba, Splat2010, Tsirel, 31 anonymous editsImage Sources, Licenses and ContributorsImage:Conditional independence.svg Source: /w/index.php?title=File:Conditional_independence.svg License: Creative Commons Attribution-Sharealike 3.0,2.5,2.0,1.0 Contributors: Original uploader was AzaToth at en.wikipedia Later version(s) were uploaded by Ddxc at en.wikipedia.LicenseCreative Commons Attribution-Share Alike 3.0 Unported/licenses/by-sa/3.0/。

杨振宁诺贝尔奖演讲词

C H E N N I N G Y A N GThe law of parity conservation and othersymmetry laws of physicsNobel Lecture, December 11, 1957It is a pleasure and a great privilege to have this opportunity to discuss with you the question of parity conservation and other symmetry laws. We shall be concerned first with the general aspects of the role of the symmetry laws in physics; second, with the development that led to the disproof of parity conservation; and last, with a discussion of some other symmetry laws which physicists have learned through experience, but which do not yet together form an integral and conceptually simple pattern. The interesting and very exciting developments since parity conservation was disproved, will be cov-ered by Dr. Lee in his lecture1.IThe existence of symmetry laws is in full accordance with our daily ex-perience. The simplest of these symmetries, the isotropy and homogeneity of space, are concepts that date back to the early history of human thought. The invariance of physical laws under a coordinate transformation of uni-form velocity, also known as the invariance under Galilean transformations, is a more sophisticated symmetry that was early recognized, and formed one of the corner-stones of Newtonian mechanics. Consequences of these sym-metry principles were greatly exploited by physicists of the past centuries and gave rise to many important results. A good example in this direction is the theorem that in an isotropic solid there are only two elastic constants. Another type of consequences of the symmetry laws relates to the con-servation laws. It is common knowledge today that in general a symmetry principle (or equivalently an invariance principle) generates a conservation law. For example, the invariance of physical laws under space displacement has as a consequence the conservation of momentum, the invariance under space rotation has as a consequence the conservation of angular momentum. While the importance of these conservation laws was fully understood, their close relationship with the symmetry laws seemed not to have been clearly recognized until the beginning of the twentieth century2. (Cf. Fig. 1.)3941957C.N.Y A N GFig. 1 .With the advent of special and general relativity, the symmetry laws gained new importance. Their connection with the dynamic laws of physics takes on a much more integrated and interdependent relationship than in classical mechanics, where logically the symmetry laws were only conse-quences of the dynamical laws that by chance possess the symmetries. Also in the relativity theories the realm of the symmetry laws was greatly en-riched to include invariances that were by no means apparent from daily experience. Their validity rather was deduced from, or was later confirmed by complicated experimentation. Let me emphasize that the conceptual sim-plicity and intrinsic beauty of the symmetries that so evolve from complex experiments are for the physicists great sources of encouragement. One learns to hope that Nature possesses an order that one may aspire to comprehend. It was, however, not until the development of quantum mechanics that the use of the symmetry principles began to permeate into the very language of physics. The quantum numbers that designate the states of a system are often identical with those that represent the symmetries of the system. It in-deed is scarcely possible to overemphasize the role played by the symmetry principles in quantum mechanics. To quote two examples: The general struc-ture of the Periodic Table is essentially a direct consequence of the isotropy of Coulomb’s law. The existence of the antiparticles - namely the positron, the antiproton, and the antineutron - were theoretically anticipated as con-sequences of the symmetry of physical laws with respect to Lorentz trans-formations. In both cases Nature seems to take advantage of the simple mathematical representations of the symmetry laws. When one pauses to consider the elegance and the beautiful perfection of the mathematical rea-soning involved and contrast it with the complex and far-reaching physicalP A R I T Y C O N S E R V A T I O N A N D O T H E R S Y M M E T R Y L A W S395 consequences, a deep sense of respect for the power of the symmetry laws never fails to develop.One of the symmetry principles, the symmetry between the left and the right, is as old as human civilization. The question whether Nature exhibits such symmetry was debated at length by philosophers of the pasts. Of course, in daily life, left and right are quite distinct from each other. Our hearts, for example, are on our left sides. The language that people use both in the orient and the occident, carries even a connotation that right is good and left is evil. However, the laws of physics have always shown complete symmetry between the left and the right, the asymmetry in daily life being attributed to the accidental asymmetry of the environment, or initial conditions in organic life. To illustrate the point, we mention that if there existed a mirror-image man with his heart on his right side, his internal organs reversed com-pared to ours, and in fact his body molecules, for example sugar molecules, the mirror image of ours, and if he ate the mirror image of the food that we eat, then according to the laws of physics, he should function as well as we do. The law of right-left symmetry was used in classical physics, but was not of any great practical importance there. One reason for this derives from the fact that right-left symmetry is a discrete symmetry, unlike rotational sym-metry which is continuous. Whereas the continuous symmetries always lead to conservation laws in classical mechanics, a discrete symmetry does not. With the introduction of quantum mechanics, however, this difference between the discrete and continuous symmetries disappears. The law of right-left symmetry then leads also to a conservation law: the conservation of parity. The discovery of this conservation law dates back to 1924 when Laporte4 found that energy levels in complex atoms can be classified into « gestriche-ne » and « ungestrichene » types, or in more recent language, even and odd levels. In transitions between these levels during which one photon is emitted or absorbed, Laporte found that the level always changes from even to odd or vice versa. Anticipating later developments, we remark that the evenness or oddness of the levels was later referred to as the parity of the levels. Even levels are defined to have parity +1,odd levels parity -1. One also defines the photon emitted or absorbed in the usual atomic transitions to have odd parity. Laporte’s rule can then be formulated as the statement that in an atomic transition with the emission of a photon, the parity of the initial state is equal to the total parity of the final state, i.e. the product of the parities of the final atomic state and the photon emitted. In other words, parity is conserved, or unchanged, in the transition.3961957 C. N. YANGIn 1927 Wigners took the critical and profound step to prove that the empirical rule of Laporte is a consequence of the reflection invariance, or right-left symmetry, of the electromagnetic forces in the atom. This fun-damental idea was rapidly absorbed into the language of physics. Since right-left symmetry was unquestioned also in other interactions, the idea was fur-ther taken over into new domains as the subject matter of physics extended into nuclear reactions,puzzle developed in the last few years. Before explaining the meaning of this puzzle it is best to go a little bit into a classification of the forces that act between subatomic particles, a classification which the physicists have learned through experience to use in the last 50 years. We list the four classes of interactions below. The strength of these interactions is indicated in the column on the right.The strongest interactions are the nuclear interactions which include the forces that bind nuclei together and the interaction between the nuclei and theP A R I T Y C O N S E R V A T I O N A N D O T H E R S Y M M E T R Y L A W S397 this century in the β-radioactivity of nuclei, a phenomena which especially in the last 25 years has been extensively studied experimentally. With the discovery of decays and µ capture it was noticed independently6 by Klein, by Tiomno and Wheeler, and by Lee, Rosenbluth and me, that these interactions have roughly the same strengths as β-interactions. They are called weak interactions, and in the last few years their rank has been con-stantly added to through the discovery of many other weak interactions responsible for the decay of the strange particles. The consistent and striking pattern of their almost uniform strength remains today one of the most tan-talizing phenomena - a topic which we shall come back to later. About the last class of forces, the gravitational forces, we need only mention that in atomic and nuclear interactions they are so weak as to be completely neg-ligible in all the observations with existing techniques.Now to return to theand τ mesonssome information about the spins and parities of the τ andmeson must have the total parity, or in other words, the product parity, of two π mesons,which is even (i.e. = +1). Similarly, the τ meson must have the total parity of three π mesons, which is odd. Actually because of the relative motion of the π mesons the argument was not as simple and unambiguous as we just discussed. To render the ar-gument conclusive and definitive it was necessary to study experimentally the momentum and angular distribution of the π mesons. Such studies were made in many laboratories, and by the spring of 1956 the accumulated ex-perimental data seemed to unambiguously indicate, along the lines of rea-soning discussed above, thatϑ and τ do not have the same parity, and con-sequently are not the same particle. This conclusion, however, was in marked contradiction with other experimental results which also became definite at about the same time. The contradiction was known as the ϑ-τ puzzle and was widely discussed. To recapture the atmosphere of that time allow me to quote a paragraph concerning the conclusion that3981957C.N.Y A N Gparticle from a report entitled « Present Knowledge about the New Par-ticles » which I gave at the International Conference on Theoretical Physics8 in Seattle, in September 1956.« However it will not do to jump to hasty conclusions. This is because ex-perimentally the K mesons (i.e. τ and ϑ) seem all to have the same masses and the same lifetimes. The masses are known to an accuracy of, say, from 2 to 10electron masses, or a fraction of a percent, and the lifetimes are known to an accuracy of, say, 20 percent. Since particles which have different spin and parity values, and which have strong interactions with the nucleons and pions, are not expected to have identical masses and lifetimes, one is forced to keep the question open whether the inference mentioned above that the are not the same particle is conclusive. Parenthetically, I might addthat the inference would certainly have been regarded as conclusive, and in fact more well-founded than many inferences in physics, had it not been for the anomaly of mass and lifetime degeneracies. »The situation that the physicist found himself in at that time has been likened to a man in a dark room groping for an outlet. He is aware of the fact that in some direction there must be a door which would lead him out of his predicament. But in which direction?That direction turned out to lie in the faultiness of the law of parity con-servation for the weak interactions. But to uproot an accepted concept one must first demonstrate why the previous evidence in its favor were insuffi-cient. Dr. Lee and I9 examined this question in detail, and in May 1956 we came to the following conclusions: (A) Past experiments on the weak inter-actions had actually no bearing on the question of parity conservation. (B) In the strong interactions, i.e. interactions of classes 1and 2 discussed above, there were indeed many experiments that established parity conservation to a high degree of accuracy, but not to a sufficiently high degree to be able to reveal the effects of a lack of parity conservation in the weak interactions. The fact that parity conservation in the weak interactions was believed for so long without experimental support was very startling. But what was more startling was the prospect that a space-time symmetry law which the phys-icists have learned so well may be violated. This prospect did not appeal to us. Rather we were, so to speak, driven to it through frustration with the various other efforts at understanding theP A R I T Y C O N S E R V A T I O N A N D O T H E R S Y M M E T R Y L A W S399 an approximate symmetry law was, however, not expected of the sym-metries related to space and time. In fact one is tempted to speculate, now that parity conservation is found to be violated in the weak interactions, whether in the description of such phenomena the usual concept of space and time is adequate. At the end of our discussion we shall have the occasion to come back to a closely related topic.Why was it so that among the multitude of experiments onThis experiment was first performed in the latter half of 1956 and finished early this year by Wu, Ambler, Hayward, Hoppes, and Hudson12. The actual experimental setup was very involved, because to eliminate disturbing out-side influences the experiment had to be done at very low temperatures. The technique of combining β-decay measurement with low temperature ap-paratus was unknown before and constituted a major difficulty which was successfully solved by these authors. To their courage and their skill, phys-icists owe the exciting and clarifying developments concerning parity con-servation in the past year.of cobalt. Very rapidly after these results were made known, many experi-ments were performed which further demonstrated the violation of parity conservation in various weak interactions. In his lecturer Dr. Lee will discuss these interesting and important developments.I I IThe breakdown of parity conservation brings into focus a number of ques-tions concerning symmetry laws in physics which we shall now briefly dis-cuss in general terms:(A) As Dr. Lee1 will discuss, the experiment of Wu, Ambler, and their collaborators also proves13,14 that charge conjugation invariance15 is violated forP A R I T Y C O N S E R V A T I O N A N D O T H E R S Y M M E T R Y L A W S401 The three discrete invariances - reflection invariance, charge conjugation invariance, and time reversal invariance - are connected by an important theorem17 called the CPT theorem. Through the use of this theorem one can prove13 a number of general results concerning the experimental manifesta-tions of the possible violations of the three symmetries in the weak inter-actions.Of particular interest is the possibility that time reversal invariance in the weak interactions may turn out to be intact. If this is the case, it follows from the CPT theorem that although parity conservation breaks down, right-left symmetry will still hold if18 one switches all particles into antiparticles in taking a mirror image.In terms of Fig. 2 this means that if one changes all the matter that composes the apparatus at the right into anti-matter, the meter reading would become the same for the two sides if time reversal invariance holds. It is important to notice that in the usual definition of re-flection, the electric field is a vector and the magnetic field a pseudovector while in this changed definition their transformation properties are switched. The transformation properties of the electric charge and the magnetic charge are also interchanged. It would be interesting to speculate on the possible relationship between the nonconservation of parity and the symmetrical or unsymmetrical role played by the electric and magnetic fields.The question of the validity of the continuous space time symmetry laws has been discussed to some extent in the past year. There is good evidence that these symmetry laws do not break down in the weak interactions. (B) Another symmetry law that has been widely discussed is that giving rise to the conservation of isotopic spin19. In recent years the use of this sym-metry law has produced a remarkable empirical order among the phenom-ena concerning the strange particles20.It is however certainly the least under-stood of all the symmetry laws. Unlike Lorentz invariance or reflection invariance, it is not a « geometrical » symmetry law relating to space time invariance properties. Unlike charge conjugation invariance21 it does not seem to originate from the algebraic property of the complex numbers that occurs in quantum mechanics. In these respects it resembles the conservation laws of charge and heavy particles. These latter laws, however, are exact while the conservation of isotopic spin is violated upon the introduction of electromagnetic interactions and weak interactions. An understanding of the origin of the conservation of isotopic spin and how to integrate it with the other symmetry laws is undoubtedly one of the outstanding problems in high-energy physics today.4021957 C.N.Y A N G(C) We have mentioned before that all the different varieties of weak interactions share the property of having very closely identical strengths. The experimental work on parity nonconservation in the past year reveals that they very likely also share the property of not respecting parity conservation and charge conjugation invariance. They therefore serve to differentiate be-tween right and left once one fixes one’s definition of matter vs. anti-mat-ter. One could also use the weak interactions to differentiate between matter and anti-matter once one chooses a definition of right vs. left. If time rever-sal invariance is violated, the weak interactions may even serve to differen-tiate simultaneously right from left, and matter from anti-matter. One senses herein that maybe the origin of the weak interactions is intimately tied in with the question of the differentiability of left from right, and of matter from anti-matter.1. T. D. Lee, Nobel Lecture, this volume, p. 406.2.For references to these developments see E. P. Wigner, Proc. Am. Phil. Soc., 93(1949) 521.3. Cf. the interesting discussion on bilateral symmetry by H. Weyl, Symmetry, Prince-ton University Press, 1952.4. O. Laporte, Z.Physik, 23 (1924) 135.5. E. P. Wigner, Z. Physik, 43 (1927) 624.6. O. Klein, Nature, 161 (1948) 897; J. Tiomno and J. A. Wheeler, Rev.Mod. Phys.,21 (1949) 144;T. D. Lee, M. Rosenbluth, and C. N. Yang, Phys. Rev., 75 (1949)905.7. R. Dalitz, Phil. Mag., 44 (1953) 1068; E. Fabri, Nuovo Cimento, II(1954) 479.8. C. N. Yang, Rev. Mod. Phys., 29 (1957) 231.9. T. D. Lee and C. N. Yang, Phys. Rev., 104 (1956) 254.10. T. D. Lee and J. Orear, Phys. Rev., 100 (1955) 932;T. D. Lee and C. N. Yang,Phys. Rev., 102 (1956) 290; M. Gell-Mann, (unpublished); R. Weinstein, (private communication) ; a general discussion of these ideas can be found in the Proceedings of the Rochester Conference, April 1956, Session VIII, Interscience, New York, 1957.11. C. N. Yang and J. Tiomno, Phys. Rev., 79 (1950) 495.12. C. S. Wu, E. Ambler, R. W. Hayward, D. D. Hoppes, and R. P. Hudson, Phys.Rev.,105 (1957) 1413.13. T. D. Lee, R. Oehme, and C. N. Yang, Phys. Rev., 106 (1957) 340.14. B. L. Ioffe, L. B. Okun, and A. P. Rudik, J.E.T.P. (U.S.S.R.), 32 (1957) 396.English translation in Soviet Phys. ]ETP, 5 (1957) 328.15. Charge conjugation invariance is very intimately tied with the hole theory inter-pretation of Dirac’s equation. The development of the latter originated with P. A.M. Dirac, Proc. Roy. Soc. London, A126 (1930) 360; J. R. Oppenheimer, Phys. Rev.,P A R I T Y C O N S E R V A T I O N A N D O T H E R S Y M M E T R Y L A W S40335 (1930) 562 and H. Weyl, Gruppentheorie und Quantenmechanik, 2nd ed., 1931,p. 234. An account of these developments is found in P. A. M. Dirac, Proc. Roy.S O c. London, A133(1931) 60. Detailed formalism and application of charge con-jugation invariance started with H. A. Kramers, Proc. Acad. Sci. Amsterdam, 40 (1937) 814and W. Furry, Phys. Rev., 51 (1937) 125.16.E. P. Wigner, Nachr. Akad. Wiss. Goettingen, Math.-Physik., 1932, p. 546.Thispaper explains in terms of time reversal invariance the earlier work of H. Kramers, Proc. Acad. Sci. Amsterdam, 33 (1930) 959.17.J. Schwinger, Phys. Rev., 91 (1953) 720, 723;G. Lüders, Kgl. Danske Videnskab.au‘s article in Niels Bohr and the Selskab., Mat.-Fys. Medd., 28, No. 5 (1954);W. P liDevelopment of Physics, Pergamon Press, London, 1955. See also Ref. 21.18.This possibility was discussed by T. D. Lee and C. N. Yang and reported by C. N.Yang at the International Conference on Theoretical Physics in Seattle in Septem-ber 1956. (See Ref. 8.) Its relation with the CPT theorem was also reported in the same conference in one of the discussion sessions. The speculation was later pub-lished in T. D. Lee and C. N. Yang, Phys. Rev., 105(1957) 1671. Independently the possibility has been advanced as the correct one by L. Landau, J.E.T.P.(U.S.S.R.), 32 (1957) 405. An English translation of Landau’s article appeared in Soviet Phys. JETP, 5 (1957) 336.19. The concept of a total isotopic spin quantum number was first discussed by B.Cassen and E. U. Condon, Phys. Rev., 50(1936) 846and E. P. Wigner, Phys. Rev., 51(1937) 106.The physical basis derived from the equivalence of p-p and n-p forces, pointed out by G. Breit, E. U. Condon, and R. D. Present, Phys. Rev., 50 (1936) 825. The isotopic spin was introduced earlier as a formal mathematical parameter by W. Heisenberg, Z. Physik, 77 (1932) I.20.A. Pais, Phys. Rev., 86 (1952) 663, introduced the idea of associated production ofstrange particles. An explanation of this phenomenon in terms of isotopic spin conservation was pointed out by M. Gell-Mann, Phys. Rev., 92 (1953) 833and by K. Nishijima, Progr. Theoret. Phys. (Kyoto), 12 (1954) 107.These latter authors also showed that isotopic spin conservation leads to a convenient quantum number called strangeness.21.R. Jost, Helv. Phys. Acta, 30 (1957) 409.。

R软件包‘tpn’的中文名称:截断正态模型和扩展软件包说明书

Package‘tpn’December11,2023Type PackageTitle Truncated Positive Normal Model and ExtensionsVersion1.8Date2023-12-11Author Diego Gallardo[aut,cre],Hector J.Gomez[aut],Yolanda M.Gomez[aut]Maintainer Diego Gallardo<********************>Description Provide data generation and estimation tools for the truncated positive normal(tpn) model discussed in Gomez,Olmos,Varela and Bolfarine(2018)<doi:10.1007/s11766-018-3354-x>,the slash tpn distribution discussed in Gomez,Gallardo and Santoro(2021)<doi:10.3390/sym13112164>,the bimodal tpn distributiondiscussed in Gomez et al.(2022)<doi:10.3390/sym14040665>and theflexible tpn model. Depends R(>=4.0.0)Imports pracma,skewMLRM,moments,VGAM,RBE3License GPL(>=2)NeedsCompilation noRepository CRANDate/Publication2023-12-1104:30:05UTCR topics documented:btpn (2)choose.fts (3)est.btpn (4)est.fts (6)est.stpn (7)est.tpn (8)est.utpn (9)fts (11)stpn (12)tpn (13)utpn (15)12btpnIndex17 btpn Bimodal truncated positive normalDescriptionDensity,distribution function and random generation for the bimodal truncated positive normal (btpn)discussed in Gomez et al.(2022).Usagedbtpn(x,sigma,lambda,eta,log=FALSE)pbtpn(x,sigma,lambda,eta,lower.tail=TRUE,log=FALSE)rbtpn(n,sigma,lambda,eta)Argumentsx vector of quantilesn number of observationssigma scale parameter for the distributionlambda shape parameter for the distributioneta shape parameter for the distributionlog logical;if TRUE,probabilities p are given as log(p).lower.tail logical;if TRUE(default),probabilities are P[X<=x]otherwise,P[X>x].DetailsRandom generation is based on the stochastic representation of the model,i.e.,the product betweena tpn(see Gomez et al.2018)and a dichotomous variable assuming values−(1+ )and1− withprobabilities(1+ )/2and(1− )/2,respectively.Valuedbtpn gives the density,pbtpn gives the distribution function and rbtpn generates random deviates.The length of the result is determined by n for rbtpn,and is the maximum of the lengths of the numerical arguments for the other functions.The numerical arguments other than n are recycled to the length of the result.Only thefirst elements of the logical arguments are used.A variable have btpn distribution with parametersσ>0,λ∈R andη∈R if its probability densityfunction can be written asf(y;σ,λ,q)=φxσ(1+ )+λ2σΦ(λ),y<0,choose.fts3 andf(y;σ,λ,q)=φxσ(1− )−λ2σΦ(λ),y≥0,where =η/1+η2andφ(·)andΦ(·)denote the probability density function and the cumulativedistribution function for the standard normal distribution,respectively.Author(s)Gallardo,D.I.,Gomez,H.J.and Gomez,Y.M.ReferencesGomez,H.J.,Caimanque,W.,Gomez,Y.M.,Magalhaes,T.M.,Concha,M.,Gallardo,D.I.(2022) Bimodal Truncation Positive Normal Distribution.Symmetry,14,665.Gomez,H.J.,Olmos,N.M.,Varela,H.,Bolfarine,H.(2018).Inference for a truncated positive normal distribution.Applied Mathemetical Journal of Chinese Universities,33,163-176. Examplesdbtpn(c(1,2),sigma=1,lambda=-1,eta=2)pbtpn(c(1,2),sigma=1,lambda=-1,eta=2)rbtpn(n=10,sigma=1,lambda=-1,eta=2)choose.fts Choose a distribution in theflexible truncated positive class of modelsDescriptionProvide model selection for a given data set in theflexible truncated positive class of modelsUsagechoose.fts(y,criteria="AIC")Argumentsy positive vector of responsescriteria model criteria for the selection:AIC(default)or BIC.DetailsThe functionfits the truncated positive normal,truncated positive laplace,truncated positive Cauchy and truncated positive logistic models and select the model which provides the lower criteria(AIC or BIC).ValueA list with the following componentsAIC a vector with the AIC for the different truncated positivefitted models:normal, laplace,cauchy and logistic.selected the selected modelestimate the estimated for sigma and lambda and the respective standard errors(s.e.) conv the code related to the convergence for the optim function.0if the convergence was attached.logLik log-likelihood function evaluated in the estimated parameters.AIC Akaike’s criterion.BIC Schwartz’s criterion.Author(s)Gallardo,D.I.,Gomez,H.J.and Gomez,Y.M.ReferencesGomez,H.J.,Gomez,H.W.,Santoro,K.I.,Venegas,O.,Gallardo,D.I.(2022).A Family of Trunca-tion Positive Distributions.Submitted.Gomez,H.J.,Olmos,N.M.,Varela,H.,Bolfarine,H.(2018).Inference for a truncated positive normal distribution.Applied Mathemetical Journal of Chinese Universities,33,163-176. Examplesset.seed(2021)y=rfts(n=100,sigma=10,lambda=1,dist="logis")choose.fts(y)est.btpn Parameter estimation for the btpn modelDescriptionPerform the parameter estimation for the bimodal truncated positive normal(btpn)discussed in Gomez et al.(2022).Estimated errors are computed based on the hessian matrix.Usageest.btpn(y)Argumentsy the response vector.All the values must be positive.DetailsA variable have btpn distribution with parametersσ>0,λ∈R andη∈R if its probability densityfunction can be written asf(y;σ,λ,q)=φxσ(1+ )+λ2σΦ(λ),y<0,andf(y;σ,λ,q)=φxσ(1− )−λ2σΦ(λ),y≥0,where =η/1+η2andφ(·)andΦ(·)denote the probability density function and the cumulativedistribution function for the standard normal distribution,respectively.ValueA list with the following componentsestimate A matrix with the estimates and standard errorsiter Iterations in which the convergence were attached.logLik log-likelihood function evaluated in the estimated parameters.AIC Akaike’s criterion.BIC Schwartz’s criterion.NoteA warning is presented if the estimated hessian matrix is not invertible.Author(s)Gallardo,D.I.,Gomez,H.J.and Gomez,Y.M.ReferencesGomez,H.J.,Caimanque,W.,Gomez,Y.M.,Magalhaes,T.M.,Concha,M.,Gallardo,D.I.(2022) Bimodal Truncation Positive Normal Distribution.Symmetry,14,665.Examplesset.seed(2021)y=rbtpn(n=100,sigma=10,lambda=1,eta=1.5)est.btpn(y)6est.fts est.fts Parameter estimation for the ftp class of distributionsDescriptionPerform the parameter estimation for the Flexible truncated positive(fts)class discussed in Gomez et al.(2022)based on maximum likelihood estimation.Estimated errors are computed based on the hessian matrix.Usageest.fts(y,dist="norm")Argumentsy the response vector.All the values must be positive.dist standard symmetrical distribution.Avaliable options:norm(default),logis, cauchy and laplace.DetailsA variable has fts distribution with parametersσ>0andλ∈R if its probability density functioncan be written asf(y;σ,λ,q)=g0(yσ−λ)σG0(λ),y>0,where g0(·)and G0(·)denote the pdf and cdf for the specified distribution.The case where g0(·) and G0(·)are from the standard normal model is known as the truncated positive normal model discussed in Gomez et al.(2018).ValueA list with the following componentsestimate A matrix with the estimates and standard errorsdist distribution specifiedconv the code related to the convergence for the optim function.0if the convergence was attached.logLik log-likelihood function evaluated in the estimated parameters.AIC Akaike’s criterion.BIC Schwartz’s criterion.NoteA warning is presented if the estimated hessian matrix is not invertible.Author(s)Gallardo,D.I.and Gomez,H.J.ReferencesGomez,H.J.,Gomez,H.W.,Santoro,K.I.,Venegas,O.,Gallardo,D.I.(2022).A Family of Trunca-tion Positive Distributions.Submitted.Gomez,H.J.,Olmos,N.M.,Varela,H.,Bolfarine,H.(2018).Inference for a truncated positive normal distribution.Applied Mathemetical Journal of Chinese Universities,33,163-176. Examplesset.seed(2021)y=rfts(n=100,sigma=10,lambda=1,dist="logis")est.fts(y,dist="logis")est.stpn Parameter estimation for the stpn modelDescriptionPerform the parameter estimation for the slash truncated positive normal(stpn)discussed in Gomez, Gallardo and Santoro(2021)based on the EM algorithm.Estimated errors are computed based on the Louis method to approximate the hessian matrix.Usageest.stpn(y,sigma0=NULL,lambda0=NULL,q0=NULL,prec=0.001,max.iter=1000)Argumentsy the response vector.All the values must be positive.sigma0,lambda0,q0initial values for the EM algorithm for sigma,lambda and q.If they are omitted,by default sigma0is defined as the root of the mean of the y^2,lambda as0andq as3.prec the precision defined for each parameter.By default is0.001.max.iter the maximum iterations for the EM algorithm.By default is1000.DetailsA variable has stpn distribution with parametersσ>0,λ∈R and q>0if its probability densityfunction can be written as1t1/qσφ(yt1/qσ−λ)dt,y>0,f(y;σ,λ,q)=whereφ(·)denotes the density function for the standard normal distribution.ValueA list with the following componentsestimate A matrix with the estimates and standard errorsiter Iterations in which the convergence were attached.logLik log-likelihood function evaluated in the estimated parameters.AIC Akaike’s criterion.BIC Schwartz’s criterion.NoteA warning is presented if the estimated hessian matrix is not invertible.Author(s)Gallardo,D.I.and Gomez,H.J.ReferencesGomez,H.,Gallardo,D.I.,Santoro,K.(2021)Slash Truncation Positive Normal Distribution:with application using the EM algorithm.Symmetry,13,2164.Examplesset.seed(2021)y=rstpn(n=100,sigma=10,lambda=1,q=2)est.stpn(y)est.tpn Parameter estimation for the tpnDescriptionPerform the parameter estimation for the truncated positive normal(tpn)discussed in Gomez et al.(2018)based on maximum likelihood estimation.Estimated errors are computed based on the hessian matrix.Usageest.tpn(y)Argumentsy the response vector.All the values must be positive.DetailsA variable have tpn distribution with parametersσ>0andλ∈R if its probability density functioncan be written asf(y;σ,λ,q)=φyσ−λσΦ(λ),y>0,whereφ(·)andΦ(·)denote the density and cumultative distribution functions for the standard nor-mal distribution.ValueA list with the following componentsestimate A matrix with the estimates and standard errorslogLik log-likelihood function evaluated in the estimated parameters.AIC Akaike’s criterion.BIC Schwartz’s criterion.NoteA warning is presented if the estimated hessian matrix is not invertible.Author(s)Gallardo,D.I.and Gomez,H.J.ReferencesGomez,H.J.,Olmos,N.M.,Varela,H.,Bolfarine,H.(2018).Inference for a truncated positive normal distribution.Applied Mathemetical Journal of Chinese Universities,33,163-176. Examplesset.seed(2021)y=rtpn(n=100,sigma=10,lambda=1)est.tpn(y)est.utpn Parameter estimation for the utpn modelDescriptionPerform the parameter estimation for the unit truncated positive normal(utpn)type1,2,3or4, parameterized in terms of the quantile based on maximum likelihood estimation.Estimated errors are computed based on the hessian matrix.Usageest.utpn(y,x=NULL,type=1,link="logit",q=0.5)Argumentsy the response vector.All the values must be positive.x the covariates vector.type to distinguish the type of the utpn model:1(default),2,3or4.link link function to be used for the covariates:logit(default).q quantile of the distribution to be modelled.ValueA list with the following componentsestimate A matrix with the estimates and standard errorslogLik log-likelihood function evaluated in the estimated parameters.AIC Akaike’s criterion.BIC Schwartz’s criterion.NoteA warning is presented if the estimated hessian matrix is not invertible.Author(s)Gallardo,D.I.ReferencesGomez,H.J.,Olmos,N.M.,Varela,H.,Bolfarine,H.(2018).Inference for a truncated positive normal distribution.Applied Mathemetical Journal of Chinese Universities,33,163-176. Examplesset.seed(2021)y=rutpn(n=100,sigma=10,lambda=1)est.utpn(y)fts11 fts Flexible truncated positive normalDescriptionDensity,distribution function and random generation for theflexible truncated positive(ftp)class discussed in Gomez et al.(2022).Usagedfts(x,sigma,lambda,dist="norm",log=FALSE)pfts(x,sigma,lambda,dist="norm",lower.tail=TRUE,log.p=FALSE)qfts(p,sigma,lambda,dist="norm")rfts(n,sigma,lambda,dist="norm")Argumentsx vector of quantilesp vector of probabilitiesn number of observationssigma scale parameter for the distributionlambda shape parameter for the distributiondist standard symmetrical distribution.Avaliable options:norm(default),logis, cauchy and laplace.log,log.p logical;if TRUE,probabilities p are given as log(p).lower.tail logical;if TRUE(default),probabilities are P[X<=x]otherwise,P[X>x]. DetailsRandom generation is based on the inverse transformation method.Valuedfts gives the density,pfts gives the distribution function,qfts gives the quantile function and rfts generates random deviates.The length of the result is determined by n for rbtpn,and is the maximum of the lengths of the numerical arguments for the other functions.The numerical arguments other than n are recycled to the length of the result.Only thefirst elements of the logical arguments are used.A variable have fts distribution with parametersσ>0andλ∈R if its probability density functioncan be written asf(y;σ,λ,q)=g0(yσ−λ)σG0(λ),y>0,where g0(·)and G0(·)denote the pdf and cdf for the specified distribution.The case where g0(·) and G0(·)are from the standard normal model is known as the truncated positive normal model discussed in Gomez et al.(2018).12stpnAuthor(s)Gallardo,D.I.,Gomez,H.J.and Gomez,Y.M.ReferencesGomez,H.J.,Gomez,H.W.,Santoro,K.I.,Venegas,O.,Gallardo,D.I.(2022).A Family of Trunca-tion Positive Distributions.Submitted.Gomez,H.J.,Olmos,N.M.,Varela,H.,Bolfarine,H.(2018).Inference for a truncated positive normal distribution.Applied Mathemetical Journal of Chinese Universities,33,163-176. Examplesdfts(c(1,2),sigma=1,lambda=1,dist="logis")pfts(c(1,2),sigma=1,lambda=1,dist="logis")rfts(n=10,sigma=1,lambda=1,dist="logis")stpn Slash truncated positive normalDescriptionDensity,distribution function and random generation for the slash truncated positive normal(stpn) discussed in Gomez,Gallardo and Santoro(2021).Usagedstpn(x,sigma,lambda,q,log=FALSE)pstpn(x,sigma,lambda,q,lower.tail=TRUE,log=FALSE)rstpn(n,sigma,lambda,q)Argumentsx vector of quantilesn number of observationssigma scale parameter for the distributionlambda shape parameter for the distributionq shape parameter for the distributionlog logical;if TRUE,probabilities p are given as log(p).lower.tail logical;if TRUE(default),probabilities are P[X<=x]otherwise,P[X>x].DetailsRandom generation is based on the stochastic representation of the model,i.e.,the quotient betweena tpn(see Gomez et al.2018)and a beta random variable.tpn13 Valuedstpn gives the density,pstpn gives the distribution function and rstpn generates random deviates.The length of the result is determined by n for rstpn,and is the maximum of the lengths of the numerical arguments for the other functions.The numerical arguments other than n are recycled to the length of the result.Only thefirst elements of the logical arguments are used.A variable has stpn distribution with parametersσ>0,λ∈R and q>0if its probability densityfunction can be written as1f(y;σ,λ,q)=t1/qσφ(yt1/qσ−λ)dt,y>0,whereφ(·)denotes the density function for the standard normal distribution.Author(s)Gallardo,D.I.and Gomez,H.J.ReferencesGomez,H.,Gallardo,D.I.,Santoro,K.(2021)Slash Truncation Positive Normal Distribution:with application using the EM algorithm.Symmetry,13,2164.Gomez,H.J.,Olmos,N.M.,Varela,H.,Bolfarine,H.(2018).Inference for a truncated positive normal distribution.Applied Mathemetical Journal of Chinese Universities,33,163-176.Examplesdstpn(c(1,2),sigma=1,lambda=-1,q=2)pstpn(c(1,2),sigma=1,lambda=-1,q=2)rstpn(n=10,sigma=1,lambda=-1,q=2)tpn Truncated positive normalDescriptionDensity,distribution function and random generation for the slash truncated positive normal(stpn) discussed in Gomez,Gallardo and Santoro(2021).Usagedtpn(x,sigma,lambda,log=FALSE)ptpn(x,sigma,lambda,lower.tail=TRUE,log=FALSE)rtpn(n,sigma,lambda)14tpn Argumentsx vector of quantilesn number of observationssigma scale parameter for the distributionlambda shape parameter for the distributionlog logical;if TRUE,probabilities p are given as log(p).lower.tail logical;if TRUE(default),probabilities are P[X<=x]otherwise,P[X>x].DetailsRandom generation is based on the inverse transformation method.Valuedtpn gives the density,ptpn gives the distribution function and rtpn generates random deviates.The length of the result is determined by n for rtpn,and is the maximum of the lengths of the numerical arguments for the other functions.The numerical arguments other than n are recycled to the length of the result.Only thefirst elements of the logical arguments are used.A variable have tpn distribution with parametersσ>0andλ∈R if its probability density functioncan be written asf(y;σ,λ,q)=φyσ−λσΦ(λ),y>0,whereφ(·)andΦ(·)denote the density and cumultative distribution functions for the standard nor-mal distribution.Author(s)Gallardo,D.I.and Gomez,H.J.ReferencesGomez,H.J.,Olmos,N.M.,Varela,H.,Bolfarine,H.(2018).Inference for a truncated positive normal distribution.Applied Mathemetical Journal of Chinese Universities,33,163-176. Examplesdtpn(c(1,2),sigma=1,lambda=-1)ptpn(c(1,2),sigma=1,lambda=-1)rtpn(n=10,sigma=1,lambda=-1)utpn15 utpn Truncated positive normalDescriptionDensity,distribution function and random generation for the unit truncated positive normal(utpn) type1or2discussed in Gomez,Gallardo and Santoro(2021).Usagedutpn(x,sigma=1,lambda=0,type=1,log=FALSE)putpn(x,sigma=1,lambda=0,type=1,lower.tail=TRUE,log=FALSE)qutpn(p,sigma=1,lambda=0,type=1)rutpn(n,sigma=1,lambda=0,type=1)Argumentsx vector of quantilesn number of observationsp vector of probabilitiessigma scale parameter for the distributionlambda shape parameter for the distributiontype to distinguish the type of the utpn model:1(default)or2.log logical;if TRUE,probabilities p are given as log(p).lower.tail logical;if TRUE(default),probabilities are P[X<=x]otherwise,P[X>x].DetailsRandom generation is based on the inverse transformation method.Valuedutpn gives the density,putpn gives the distribution function,qutpn provides the quantile function and rutpn generates random deviates.The length of the result is determined by n for rtpn,and is the maximum of the lengths of the numerical arguments for the other functions.The numerical arguments other than n are recycled to the length of the result.Only thefirst elements of the logical arguments are used.A variable has utpn distribution with scale parameterσ>0and shape parameterλ∈R if itsprobability density function can be written asf(y;σ,λ)=φ1−yσy−λσy2Φ(λ),y>0,(type1),16utpnf(y;σ,λ)=φyσ(1−y)−λσ(1−y)2Φ(λ),y>0,(type2),f(y;σ,λ)=φlog(y)σ+λσyΦ(λ),y>0,(type3),f(y;σ,λ)=φlog(1−y)σ+λσ(1−y)Φ(λ),y>0,(type4),whereφ(·)andΦ(·)denote the density and cumulative distribution functions for the standard nor-mal distribution.Author(s)Gallardo,D.I.ReferencesGomez,H.J.,Olmos,N.M.,Varela,H.,Bolfarine,H.(2018).Inference for a truncated positive normal distribution.Applied Mathemetical Journal of Chinese Universities,33,163-176. Examplesdutpn(c(0.1,0.2),sigma=1,lambda=-1)putpn(c(0.1,0.2),sigma=1,lambda=-1)rutpn(n=10,sigma=1,lambda=-1)Indexbtpn,2choose.fts,3dbtpn(btpn),2dfts(fts),11dstpn(stpn),12dtpn(tpn),13dutpn(utpn),15est.btpn,4est.fts,6est.stpn,7est.tpn,8est.utpn,9fts,11pbtpn(btpn),2pfts(fts),11pstpn(stpn),12ptpn(tpn),13putpn(utpn),15qfts(fts),11qutpn(utpn),15rbtpn(btpn),2rfts(fts),11rstpn(stpn),12rtpn(tpn),13rutpn(utpn),15stpn,12tpn,13utpn,1517。

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ar X i v :h e p -t h /0006201v 3 6 S e p 2000Preprint typeset in JHEP style.-HYPER VERSIONClaudio A.Scrucca Sektion Physik,Ludwig Maximilian Universit¨a t M¨u nchen Theresienstrasse 37,80333Munich,Germany Claudio.Scrucca@physik.uni-muenchen.de Marco Serone Department of Mathematics,University of Amsterdam Plantage Muidergracht 24,1018TV Amsterdam,The Netherlands;Spinoza Institute,University of Utrecht Leuvenlaan 4,3584CE Utrecht,The Netherlands serone@wins.uva.nl Abstract:We investigate in the simplest compact D =4N =1Type IIB ori-entifold models the sigma-model symmetry suggested by the proposed duality of these models to heterotic orbifold vacua.This symmetry is known to be present at the classical level,and is associated to a composite connection involving untwisted moduli in the low-energy supergravity theory.In order to study possible anomaliesarising at the quantum level,we compute potentially anomalous one-loop amplitudes involving gluons,gravitons and composite connections.We argue that the effective vertex operator associated to the composite connection has the same form as that for a geometric deformation of the orbifold.Assuming this,we are able to compute the complete anomaly polynomial,and find that all the anomalies are canceled through a Green-Schwarz mechanism mediated by twisted RR axions,as previously conjec-tured.Some questions about the field theory interpretation of our results remain open.Keywords:D-branes,orientifolds,anomalies.1.IntroductionRecently,renewed interest has been devoted to orientifold vacua of Type IIB string theory,constructed by projecting out a standard toroidal compactification by the combined action of a discrete spacetime orbifold symmetry G and the world-sheetparityΩ[1,2,3,4].These unoriented string theories contain both open and closed strings,and constitute the perhaps most important and concrete example of mod-els in which gauge interactions are localized on D-branes[5].They are therefore the natural arena for the realization of the“brane-world”scenario.Furthermore, this kind of models have proven to offer surprisingly attractive possibilities from a phenomenological point of view(see for instance[6,7]).In the following,we will be concerned with compact D=4N=1Type IIB orientifold models[8,9,10,11,12].These vacua represent a simple and tractable pro-totype of more general and possibly non-supersymmetric orientifold models.Some of them are also phenomenologically appealing and constitute a viable alternative to their more traditional heterotic analogues.In fact,a weak-weak Type IIB-heterotic duality has been conjectured[8,10,12,13]for several pairs of vacua1.In particular, Z N orientifolds with N odd do contain D9-branes but no D5-branes,and could be dual to the corresponding perturbative Z N heterotic orbifold.Models with N even do instead contain both D9-branes and D5-branes,and could be dual to heterotic orb-ifolds with a perturbative sector corresponding to D9-branes and a non-perturbative instantonic sector corresponding to D5-branes[13].At the classical level,evidence for the duality is suggested by the almost per-fect matching of the low-energy spectra and the fact that the orientifold models seem to possess the same classical symmetries as their heterotic companions[20].In particular,they both possess a so-called“sigma-model”symmetry2,naturally emerg-ing from N=1supergravity.More precisely,this symmetry consists of SL(2,R) transformations for the untwisted T i moduli and the other chiral superfields,im-plemented as the combination of a K¨a hler transformation and a reparametrization of the scalar K¨a hler manifold.On the heterotic side,a discrete SL(2,Z)subgroup of these transformations is known to correspond to the well-known T-duality sym-metry,valid to all orders of string perturbation theory,and is therefore expected to be exact.On the orientifold side,instead,sigma-model transformations do not seem to correspond to any known underlying string symmetry,and it is not clear whether the symmetry is exact.At the quantum level,the comparison becomes much more involved and several subtleties arise.In particular,it has been argued in[21]that the one-loop corrected gauge couplings in orientifold models seem to be incompatible with any duality map(see also[22]for further discussion).Thereis however an important issue which can be addressed even without knowing the detailed duality map:whether or not the classical sigma-model symmetry is anoma-lous at the quantum level.The latter continuous symmetry is indeed associated to a composite connection in the low-energy effective supergravity theory,and acts as chiral rotations on all the fermions.There are therefore anomalous triangular dia-grams involving gluons,gravitons and composite connections,leading in general to a non-vanishing one-loop anomaly.On the heterotic side,this one-loop anomaly is canceled by a universal tree-level Green-Schwarz(GS)mechanism mediated by the dilaton[23,24],and the appearance of the appropriate GS term has been explicitly checked through a string theory computation[25].On the orientifold side,it was proposed in[20]that a similar GS mechanism involving both the dilaton and twisted RR axions could cancel the anomalies.This observation was motivated by the fac-torizability of mixed sigma-gauge anomalies computed from the low-energy spectra. However,it was subsequently argued in[22]that requiring a similar mechanism also for mixed sigma-gravitational anomalies would lead to an apparent contradiction with the known results for gauge-gravitational anomaly cancellation[27].The question of whether the sigma-model symmetry is anomalous or not in orientifold models is therefore still unclear and of extreme relevance for their duality to heterotic theories. Note however that even if the presence of anomalies would pose serious problems to the duality,it would not be fatal for the consistency of the orientifold models in themselves3.The aim of this paper is to study the cancellation of all possible(pure or mixed) sigma-gauge-gravitational anomalies in orientifold models through a string theory computation.Such an analysis is interesting by itself even beyond the context of Type IIB-heterotic duality,since it can provide useful informations about the low-energy effective action.For instance,the GS couplings that will be derived are related by supersymmetry to other couplings in the Lagrangian and determine under suitable assumptions the gauge kinetic functions and the Fayet-Iliopoulos terms.For simplicity,the analysis will be restricted to the models with N odd.These are indeed simpler than models with N even for a variety of reasons;in particular,they do not present threshold corrections[21].The only consistent models with N odd are theZ3and the Z7models.We follow the strategy developed in[26,27]for standard gauge-gravitational anomalies,and compute both the quantum anomaly and the classical inflow in all possible channels.By factorization,it is then possible to extract all the anomalous couplings for D-branes andfixed-points present in each model,and the GS term given by their sum.A major ingredient of our computation is an effective vertex operator for the composite sigma-model connection,which results from a pair of untwisted K¨a hler moduli.We provide arguments that such a vertex is in fact the same as that of an“internal graviton”associated to a deformation of the K¨a hler structure of the orbifold respecting its rigid complex-structure.This suggests that there is a close relation between sigma-model symmetry and invariance under reparametrizations of the internal part of the spacetime manifold.In particular,potential anomalies in these symmetries seem to coincide.Assuming the relation above to be valid and using this common vertex,we are able to compute the complete anomaly polynomial as a function of the gauge,gravitational and sigma-model curvatures.Wefind that all the anomalies are canceled through a GS mechanism mediated by twisted RR axions only,extending the results of[27]for gauge-gravitational anomalies.The dilaton does not play any role in the anomaly cancellation mechanism,contrarily to what proposed in[20]and in agreement with[22].The results of our string computation disagree with thefield theory analysis of [22]on a crucial sign in the contribution of the twisted modulini to the one-loop sigma-gravitational anomaly.Contrary to what assumed in[22],it seems that these twisted closed string states must have a non-vanishing“effective”modular weight, that is responsible for the full cancellation of all the anomalies.Although we do not have yet a complete understanding of thefield theory interpretation of our results and their implications on the low-energy effective action,we believe that they rise some questions about the actual form of the K¨a hler potential for twistedfields.As far as we know,this potential has not yet been unambiguously determined.The only available proposal about its form is that of[28],and it was indeed assumed in[22].However,this potential implies vanishing modular weight for twistedfields, in apparent contradiction with our results,at least if one does not include possible tree-level corrections to it induced by the GS mechanism.Whether our string results might be explained by taking into account the GS terms in the potential proposed in[28],or they imply a different form for the K¨a hler potential of twistedfields,has still to be understood[29].Independently of their actualfield theory explanation,we think that our results provide strong evidence for the occurrence of this cancellation mechanism,generaliz-ing it moreover to all the other types of anomalies,like in particular pure sigma-model anomalies.Unfortunately,although we provide several convincing arguments on the correctness of the effective vertex operator for the composite sigma-model connec-tion,a rigorous proof is missing.Therefore,the only safe statement that we are in position to make is that the associated symmetry is preserved at the one-loop level thanks to a generalized GS mechanism.Whether or not this is really the sigma-model symmetry remains strictly speaking to be proven,although we believe that it is quite unlikely that this is not the case since all the anomalies we compute have precisely the structure expected for sigma-gauge-gravitational anomalies.Notice also that thanks to the alternative interpretation of this vertex as an internal graviton,these canceled anomalies can be inequivocably interpreted as relative to internal reparametrizations. As such,they admit a topological interpretation in terms of equivariant indices of the spin and signature complexes,and it is possible to verify the results obtained through the direct string computation by applying suitable index theorems,as we will see.The structure of the paper is the following.In Section2,we briefly review the notion of sigma-model symmetry.In Section3,we set up the general strategy of the string computation and propose a possible path-integral derivation of the effective vertex for the composite connection.In Section4we perform the string computation on the four surfaces appearing at the one-loop order.In Section5,we reproduce the same results from a mathematical point of view as topological indices. In Section6,we discuss in more detail the obtained quantum anomalies and perform the factorization of the classical inflow to get all the RR anomalous couplings and the total GS term.In Section7,we discuss possiblefield-theory interpretations of our results and their implications.Finally,we give conclusions in Section8.In Appendix A,we report useful conventions aboutϑ-functions.In Appendix B,we discuss the cancellation of anomalies in Type IIB string theory(this completes the analysis in[26]).Finally,Appendix C contains some useful details about the string computation.2.Sigma-model symmetryIn this section,we briefly review some well-known facts about the sigma-model sym-metry,and discuss its potential anomalies in D=4,N=1supergravity models. These general concepts are useful for the considerations that will follow,in particular in Section7.The scalar manifold M of any generic D=4N=1supergravity model is known to be a K¨a hler manifold,described by a K¨a hler potential K.At the classical level the Lagrangian presents two distinct symmetries(beside possible local gauge symmetries):•K¨a hler symmetry,under which the K¨a hler potential transforms as4κ2K(ΦM,¯ΦM)→κ2K(ΦM,¯ΦM)+F(ΦM)+¯F(¯ΦM).(2.1)•Global isometries of M,under whichφM→φ′M(φN).(2.2)HereΦM andφM denote all the chiral multiplets in the model and their lowest components,F(Φ)is a generic chiral superfield,andκ2is Newton’s gravitational constant.The fermionsψM in the chiral multipletΦM transform also under(2.1) and(2.2).Correspondingly,the fermionic kinetic terms contain a covariant derivative involving the following“K¨a hler”and“isometry”connections[30]:A(K)µ=−i4The Lagrangian is invariant under(2.1)if also the superpotential W transforms as W→e−F W. Since W is irrelevant in the considerations that will follow,we will neglect it.orientifolds we want to analyze,i.e.the Z3and the Z7model(see[8,9,10]for more details on these string vacua).The massless closed string spectrum of these models contain the gravitational multiplet,a universal chiral multiplet S,three chiral multiplets T i corresponding to the(complexified)K¨a hler deformations of the three internal two-tori5,and a given number of chiral multiplets Mαarising from the twisted sectors of the orbifold.The open string spectrum(from D9branes only in these models)contains vector multiplets and three groups of charged chiral multiplets C a.In order to distinguish the different coordinates of M,we use the index M= (i,a,α)for T i,C a and Mαrespectively.As we will see in next sections,the dilaton field S does not participate at all to the GS mechanism canceling the anomalies,and is inert under any gauge,diffeomorphism or sigma-model transformations.Up to quadratic order in the chargedfields,the total K¨a hler potential of these orientifolds is believed to be[20]6:κ2K tot(ΦM,¯ΦM)=−ln(S+¯S)−3i=1ln(T i+¯T i)+3 i=1δa i¯C a C aic i T i+d i,(2.6)C a→δa i5Actually,additional“off-diagonal”untwisted moduli survive the orientifold projection in the special Z3model.We do not consider them here for simplicity,and all the considerations that follow are independent of the presence of thesefields.6See also[31]for further considerations on the K¨a hler potential of D=4orientifold models.withλi (T i )=ln(ic i T i +d i ).(2.10)The sigma-model symmetry in question is therefore the combination of an isometry and a K¨a hler transformation,and potential anomalies will therefore involve both connections (2.3)and (2.4).In order to be able to derivean explicit formula at least for mixed sigma-gauge/gravitational anomalies,we need to make some extra assumptions on the potential K (M )and the transformations (2.8).We take here the one usually consid-ered in the literature,that indeed holds generically for heterotic models [32]:κ2K (M )(M α,¯M α,T i ,¯T i )=α3 i =1(T i +¯T i )n αi ¯M αM α+...,M α→(ic i T i +d i )n αi M α,(2.11)where the dots stand for possible higher order terms in M α,¯M α.The numbers n αi are the so-called “modular weights”[33]of the fields M α.It is straightforward to see that for the reparametrizations (2.6),(2.7)and (2.8),and the K¨a hler transformation (2.9)and (2.10)(F =λi ),the total connection Z M µ≡A (K )µ+A (I )M µM transforms as a U (1)connection 7:Z M µ→Z M µ+(1+2n M i )∂µIm λi ,(2.12)where n αiare the coefficients defined in (2.11),n a i =−δa i ,and n j i =−2δj i .The sigma-model symmetry can therefore be viewed as a U (1)i symmetry with “modularcharge”Q M i =(1+2n M i ).The explicit form of ZM and its field-strength G M =dZ M can be easily evaluated.It is actually convenient to disentangle the modular charges Q M i from the connection and define the three connections Z µ,i and their field-strength G µ,i so that Z M µ= i Q M i Z i,µand G M µν= i Q M i G i,µν.One finds:Z i,µ=it i +¯t i ,(2.13)G i,µν=2i ∂[µt i ∂ν]¯t i 7In deriving (2.12)we assumed that the orbifold limit corresponds to C a = M α =0.The orbifold limit,however,is generically assumed to be given by m α =0,where the scalars m αbelong to the linear multiplets L α,dual of the chiral multiplets M α[21].So we are assuming that at leading order m α =0corresponds to M α =0.3.Anomalies in orientifold modelsIn this section,we will set up the general strategy for studying all types of anoma-lies in chiral orientifold models,and investigate their cancellation.We will begin byreviewing the main aspects of the approach developed in[26,27]for standard anoma-lies(see also[34]for a similar analysis in non-geometric models),and generalize itto sigma-gauge-gravitational anomalies.To begin,we shall briefly recall some basic but important facts about anomaliesfor the convenience of the reader.Anomalies in a quantumfield theory effective actionhave to satisfy the Wess-Zumino(WZ)consistency condition.These in turn implythat any anomaly in D dimensions is uniquely characterized by a gauge-invariant andclosed(D+2)-form ing the standard WZ-descent notation8:A=2πi I(1). The anomaly polynomial I is a characteristic class of the gauge and tangent bundles,of degree(D+2)/2in the curvature two-forms.3.1The strategyThe cancellation of anomalies in string theory is achieved in a very natural andelegant way,and is intimately related to more general consistency requirements,likemodular invariance and tadpole cancellation.Possible anomalies arise exclusivelyfrom boundaries of the moduli space of one-loop string world-sheets.Moreover,direct computations have shown[35]that the whole tower of massive string statescontribute in general to anomalies in such a way that these vanish for consistentmodels,even if the massless spectrum is generically anomalous on its own.From alow-energy effectivefield theory point of view,where massive states are integrated outand only the resulting effective dynamics of the light modes is considered,the totalone-loop anomaly is canceled by an exactly opposite anomaly arising in tree-levelprocesses involving the magnetic exchange of tensorfields[36].This is the celebratedGreen-Schwarz(GS)mechanism[36],and is an absolutely crucial ingredient for theexistence of consistent supersymmetric chiral gauge theories in higher dimensions.In the following,we will focus on the CP-odd part of the one-loop effectiveaction,where anomalies arise.For consistent models,the exact string theory compu-tation is expected to yield a vanishing anomaly.However,as discussed above,this isinterpreted as a non-trivial GS mechanism of anomaly cancellation in a low-energy√effective theory valid at energies E≪1/8The invariant closed(D+2)-form I defines locally a non-invariant Chern-Simons(D+1)-formI(0)such that I=dI(0),whose gauge variation then defines a(D)-form I(1)throughδI(0)=dI(1).over the world-sheet moduli.The motivation to pursue this strategy,instead of the more direct full string theory computation,is threefold.First,the required computa-tions simplify dramatically.Furthermore,one gets an improved understanding of the low-energy mechanism of anomaly cancellation.Finally,one can extract important WZ couplings appearing in the effective action by factorization[26,27].Consider now orientifold models.The relevant anomalous string diagrams are the annulus(A),the M¨o bius strip(M)and the Klein bottle(K).These world-sheet surfaces lead to potential divergences due to possible tadpoles for massless particles propagating in the transverse channel.Consequently,they also lead to potential anomalies.In addition,also the torus(T)surface can be anomalous,in the limit under consideration.We will see that there are contributions to the anomaly from this diagram,but they turn out to always cancel among themselves.The most general situation which is allowed by the property that anomalous amplitudes are boundary terms in moduli space is the following.The A,M and K surfaces are parametrized by a real modulus t∈[0,∞].The contribution from the boundary at t→∞is interpreted as the standard quantum anomaly,whereas the contributions from the other boundary at t→0is interpreted as classical inflow of anomaly.The T amplitude is instead parametrized by a complex modulusτ∈F, where F is the fundamental domain.Again,the contribution from the component ∂F∞=[−1/2+i∞,1/2+i∞]of the boundary∂F at infinity is interpreted as the standard quantum anomaly,whereas the contribution from the remaining component ∂F0should be associated to the classical inflow of anomaly.Summing up,one would therefore get a quantum anomaly A=(A+M+K+T)|∞and a classical inflow I=(A+M+K+T)|0.It should be however mentioned that the above interpretation for the T surface involves some conceptual subtleties related to modular invariance,that might mix different contributions.Luckily,we will see that the T amplitude gives a vanishing contribution anyhow:the pieces in the∂F0component cancel pairwise thanks to modular invariance[37],that still holds in theα′→0limit,whereas the ∂F∞component vanishes by itself.Moreover,the A,M and K contributions are topological and independent of the modulus.Correspondingly,A and I are identical to each other and cancel.As last important remark,notice that in four dimensions even in non-planar diagrams the closed string state exchanged in the transverse channel is always on-shell,due to the conservation of momentum.Strictly speacking,this means that the usual argument for the cancellation of anomalies at the string level[35]does not apply in this case,giving further motivation for a detailed analysis.3.2Set-up of the computationThe computation of the A,M,K and T amplitudes proceeds along the lines of[26, 27],that we shall briefly review and extend.For the time being,we shall assume that the composite connections(2.13)are described by suitable effective vertex operators, postponing a detailed discussion of this issue to next subsection.An anomaly of the type discussed above,in the CP-odd part of the effective action,is encoded in a one-loop correlation function in the odd spin-structure on the A,M and K surfaces,and in the odd-even and even-odd spin-structures on the T surface,involving gluons,gravitons and composite connections.Denoting byρthe modulus of the surface and by F its integration domain,one has on a given surface and spin-structureA1...n= F dρ V1′V2...V n J .(3.1) The insertion of the supercurrent J is due to the existence of a world-sheet gravitino zero-mode;more precisely,J=T F+˜T F in the odd spin-structure on the A,M and K surfaces,and J=T F,˜T F in the odd-even and even-odd spin-structures respectively on T.The vertex V′is taken in the−1-picture in the odd sector and represents an unphysical particle.Taking the latter to be a longitudinally polarized gluon, graviton or composite connection,one computes the variation of the one-loop effective action under gauge,diffeomorphisms or sigma-model transformations.The remaining vertices V are taken in the0-picture and represent physical background gluons, gravitons or composite connections.Thanks to world-sheet supersymmetry and the limitα′→0,one can use effective vertex operators which are simpler to handle.After some formal manipulations,the correlation function above can be rewritten as boundary terms in moduli space[38,37]A1...n= ∂F dρ W1V2...V n ,(3.2) where W is an auxiliary vertex defined out of V′for the unphysical particle.Impor-tantly,the vertices V’s contain two tangent fermionic zero-modes,whereas W does not contain any of them.The insertion of W,rather than V,for the unphysical par-ticle representing the gauge variation of the one-loop effective action corresponds to the fact that the anomaly A is given by the WZ descent of the anomaly polynomial I:A=2πi I(1).More precisely,one can show[26,27]that the latter is obtained simply by substituting back V instead of W,that isI1...n= ∂F dρ V1V2...V n ,(3.3) with the convention of working in two more dimensions and omitting the integration over bosonic zero-modes.Finally,it is possible to define the generating functional ofall the possible anomalies by exponentiating one representative vertex for each type of particle and compute the resulting deformed partition function Z′.Finally,the total anomaly polynomial is given just byI= ∂F dρZ′.(3.4) 3.3Effective verticesThe fact that one can use effective vertices in the computation of the partition func-tion yielding the anomaly polynomial is due to theα′→0limit and to certain special properties of correlation functions in supersymmetric spin-structures like those of rel-evance here.One way to understand this is to notice that the partition functions to be computed are related to topological indices which are almost insensitive to any continuous parameter deformation.From a more technical point of view,there is always a fermionic zero-mode for each spacetime direction.The corresponding Berezin integral in the partition function yields a vanishing result unless the inter-action vertices provide one of each fermionic zero-mode.Infact,products of these fermionic zero modes provide a basis of forms of all degrees in the target spacetime, the Berezin integral selecting the appropriate total degree.On general grounds,it is expected that the effective vertices depend only on the corresponding curvature.Since these behave as two-forms,they must be contracted with two tangent fermionic zero-modes.Moreover,the vertices must be world-sheet supersymmetric.Finally,thanks to theα′→0limit,they cannot contain additional momenta,beside from those defining the curvature.These three basic requirements, together with the index structure of the curvatures and conformal invariance,turn out to severely constrain the effective vertices in each case.For gluons and gravi-tons,they can be derived in a straightforward way as in[26],but for the composite connections(2.13),the analysis is much more involved since the latter are not funda-mentalfields but composite of the scalarfields of the theory,and there are therefore no vertex operators directly associated to them.Our main observation is that the field-strengths(2.14)have a quadratic dependence on the untwisted t i and¯t i moduli fluctuations.Correspondingly,suitable amplitudes with the insertion of the vertex operators associated to these scalars should reproduce the insertion of the composite connections(2.13).The untwisted t i moduli are defined as[10]t i=e−φ10g i¯i+iθi,(3.5)whereφ10is the ten-dimensional dilaton,g i¯i is the metric component along the T2i torus andθi is a RR axion.The real part of these moduli is therefore represented bya NSNS vertex operator,whereas the imaginary part is described by a RR vertex, involving spin-fields and particularly unpleasant to deal with.Notice for the moment that these vertex operators can provide at most one spacetime fermionic zero-mode. Since physical gluons and gravitons bring each two fermionic zero-modes,correlations with an odd number of moduli vanish,as expected from the fact these should come in pairs reconstructing composite connections.Moreover,in the limit of interest, the correlation functions under analysis factorize into an internal correlation among modulifields and a spacetime correlation among gluons and gravitons.We now propose an approach to the derivation of the effective vertex for the composite connection,which is not exhaustive but will allow us to emphasize a few important points.Focus for simplicity on a single internal torus only,for which the composite curvature(2.14)becomes(no sum over the indices)G i,µν=2i K i¯i∂[µt i∂ν]¯t i, with K i¯i=(t i+¯t i)−2.On general grounds,one expects the moduli to pair and reconstruct only composite curvatures of this form.At leading order in the momenta, the structure of the internal correlation between two moduli must therefore be as follows:V t i(p1)V¯t i(p2) =αi K i¯i p1µt i p2ν¯t iψµ0ψν0,(3.6)V t i V t i = V¯t i V¯t i =0,(3.7) whereαi are some coefficients and V t i and V¯t i are the vertex operators for the scalars t i and¯t i.As already mentioned,correlations such as(3.6)are potentially difficult to compute in orientifold models,because the moduli vertices have a simple NSNS real part,but a complicated RR imaginary part.More precisely,the sigma-model curvature can be rewritten as G iµν=i K i¯i∂[µ(t i−¯t i)∂ν](t i+¯t i),and one has in principle to use one RR vertex V t i−V¯t i and one NSNS vertex V t i+V¯t i.One could then proceed by contracting the NSNS and RR vertex,take theα′→0limit and try tofigure out which is the effective vertex that,inserted in the correlation function, gives the same result.This procedure is however complicated,so we prefer to use a trick that will allow us to deduce the effective vertex in a quicker(although not rigorous)way.The point is that correlations involving only pairs of V t i+V¯t i vertices are formally proportional to the corresponding correlations involving pairs of V t i+V¯t i and V t i−V¯t i vertices.Indeed,using(3.6)and(3.7),one gets:(V t i±V¯t i)(p1)(V t i+V¯t i)(p2) =αi K i¯i p1µt i p2ν¯t i±(1↔2) ψµ0ψν0.(3.8) Due to the symmetrization in1↔2,one gets a vanishing result for two NSNS vertices (upper sign),but a non vanishing one for one RR and one NSNS vertices(lower sign).。

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