Comment on Gauge Invariance and $k_T$-Factorization of Exclusive Processes

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Quantum Hall effect - Wikipedia, the free encyclopedia

Quantum Hall effect - Wikipedia, the free encyclopedia

Quantum Hall effectFrom Wikipedia, the free encyclopediaThe quantum Hall effect (or integer quantum Hall effect) is a quantum-mechanical version of the Hall effect, observed in two-dimensional electron systems subjected to low temperatures and strong magnetic fields, in which the Hall conductance G undergoes certain quantum Hall transitions to take on the quantized valueswhere is the channel current, is the Hall voltage, e is the elementary charge and h is Planck's constant. The prefactor ν is known as the "filling factor", and can take on either integer (ν = 1, 2, 3, .. ) or fractional (ν = 1/3, 2/5, 3/7, 2/3, 3/5, 1/5, 2/9, 3/13, 5/2, 12/5 ...) values. The quantum Hall effect is referred to as the integer or fractional quantum Hall effect depending on whether ν is an integer or fraction respectively. The integer quantum Hall effect is very well understood, and can be simply explained in terms of single-particle orbitals of an electron in a magnetic field (see Landau quantization). The fractional quantum Hall effect is more complicated, as its existence relies fundamentally on electron–electron interactions. It is also very well understood as an integer quantum Hall effect, not of electrons but of charge-flux composites known as composite fermions. In 1988, it was proposed that there was quantum Hall effect without Landau levels. This quantum Hall effect is referred to as the quantum anomalous Hall (QAH) effect. There is also a new concept of the quantum spin Hall effect which is an analogue of the quantum Hall effect, where spin currents flow instead of charge currents.[1]Contents◾1 Applications◾2 History◾3 Integer quantum Hall effect – Landau levels◾4 Mathematics◾5 See also◾6 References◾7 Further readingApplicationsThe quantization of the Hall conductance has the important property of being incredibly precise. Actual measurements of the Hall conductance have been found to be integer or fractional multiples of e2/h to nearly one part in a billion. This phenomenon, referred to as "exact quantization", has been shown to be a subtle manifestation of the principle of gauge invariance.[2] It has allowed for the definition of a new practical standard for electrical resistance, based on the resistance quantum givenby the von Klitzing constant R K = h/e2 = 25812.807557(18) Ω.[3] This is named after Klaus von Klitzing, the discoverer of exact quantization. Since 1990, a fixed conventional value R K-90 is used in resistance calibrations worldwide.[4] The quantum Hall effect also provides an extremely precise independent determination of the fine structure constant, a quantity of fundamental importance in quantum electrodynamics.HistoryThe integer quantization of the Hall conductance was originally predicted by Ando, Matsumoto, and Uemura in 1975, on the basis of an approximate calculation which they themselves did not believe to be true. Several workers subsequently observed the effect in experiments carried out on the inversion layer of MOSFETs. It was only in 1980 that Klaus von Klitzing, working at the high magnetic field laboratory in Grenoble with silicon-based samples developed by Michael Pepper and Gerhard Dorda, made the unexpected discovery that the Hall conductivity was exactly quantized. For this finding, von Klitzing was awarded the 1985 Nobel Prize in Physics. The link between exact quantization and gauge invariance was subsequently found by Robert Laughlin. Most integer quantum Hall experiments are now performed on gallium arsenide heterostructures, although many other semiconductor materials can be used. In 2007, the integer quantum Hall effect was reported in graphene at temperatures as high as room temperature,[5] and in the oxide ZnO-Mg x Zn1-x O.[6] Integer quantum Hall effect – Landau levelsIn two dimensions, when classical electrons are subjected to a magnetic field they follow circular cyclotron orbits. When the system is treated quantum mechanically, these orbits are quantized. The energy levels of these quantized orbitals take on discrete values: , where ωc = eB/m is the cyclotron frequency. These orbitals are known as Landau levels, and at weak magnetic fields, their existence gives rise to many interesting "quantum oscillations" such as the Shubnikov–de Haas oscillations and the de Haas–van Alphen effect (which is often used to map the Fermi surface of metals). For strong magnetic fields, each Landau level is highly degenerate (i.e. there are many single particle states which have the same energy E n). Specifically, for a sample of area A, inmagnetic field B, the degeneracy of each Landau level is (where g s represents a factor of 2 for spin degeneracy, and is the magnetic flux quantum). ForHofstadter's butterfly sufficiently strong B-fields, each Landau level may have so many states that all of the free electrons in the system sit in only a few Landau levels; it is in this regime where one observes the quantum Hall effect.MathematicsThe integers that appear in the Hall effect are examples oftopological quantum numbers. They are known inmathematics as the first Chern numbers and are closelyrelated to Berry's phase. A striking model of much interest inthis context is the Azbel-Harper-Hofstadter model whosequantum phase diagram is the Hofstadter butterfly shown inthe figure. The vertical axis is the strength of the magneticfield and the horizontal axis is the chemical potential, whichfixes the electron density. The colors represent the integer Hall conductances. Warm colors represent positive integersand cold colors negative integers. The phase diagram isfractal and has structure on all scales. In the figure there is an obvious self-similarity.Concerning physical mechanisms, impurities and/or particular states (e.g., edge currents) are important for both the 'integer' and 'fractional' effects. In addition, Coulomb interaction is also essential in the fractional quantum Hall effect. The observed strong similarity between integer and fractional quantum Hall effects is explained by the tendency of electrons to form bound states with an even number of magnetic flux quanta, called composite fermions .See also◾quantum Hall transitions◾Fractional quantum Hall effect◾Composite fermions◾Hall effect◾Hall probe◾Graphene◾Quantum spin Hall effect◾Coulomb potential between two current loops embedded in a magnetic fieldReferences1.^ Ezawa, Zyun F. (2013). Quantum Hall Effects: Recent Theoretical and Experimental Developments (3rd ed.). World Scientific. ISBN 978-981-4360-75-3.2.^ Laughlin, R. (1981). "Quantized Hall conductivity in twodimensions" (/abstract/PRB/v23/i10/p5632_1). Physical Review B 23 (10): 5632–5633. Bibcode:1981PhRvB..23.5632L (/abs/1981PhRvB..23.5632L).doi:10.1103/PhysRevB.23.5632 (/10.1103%2FPhysRevB.23.5632). Retrieved 8 May 2012.3.^ Tzalenchuk, Alexander; Lara-Avila, Samuel; Kalaboukhov, Alexei; Paolillo, Sara; Syväjärvi, Mikael;Yakimova, Rositza; Kazakova, Olga; Janssen, T. J. B. M.; Fal'ko, Vladimir; Kubatkin, Sergey (2010)."Towards a quantum resistance standard based on epitaxialgraphene" (/nnano/journal/v5/n3/abs/nnano.2009.474.html). NatureNanotechnology5 (3): 186–189. arXiv:0909.1220 (https:///abs/0909.1220).Bibcode:2010NatNa...5..186T (/abs/2010NatNa...5..186T).doi:10.1038/nnano.2009.474 (/10.1038%2Fnnano.2009.474). PMID 20081845(https:///pubmed/20081845).4.^ "conventional value of von Klitzing constant" (/cgi-bin/cuu/Value?rk90). NIST.5.^ Novoselov, K. S.; Jiang, Z.; Zhang, Y.; Morozov, S. V.; Stormer, H. L.; Zeitler, U.; Maan, J. C.;Boebinger, G. S.; Kim, P.; Geim, A. K. (2007). "Room-Temperature Quantum Hall Effect in Graphene".Science315 (5817): 1379. arXiv:cond-mat/0702408 (https:///abs/cond-mat/0702408).Bibcode:2007Sci...315.1379N (/abs/2007Sci...315.1379N).doi:10.1126/science.1137201 (/10.1126%2Fscience.1137201). PMID 17303717(https:///pubmed/17303717).6.^ Tsukazaki, A.; Ohtomo, A.; Kita, T.; Ohno, Y.; Ohno, H.; Kawasaki, M. (2007). "Quantum Hall Effectin Polar Oxide Heterostructures". Science315 (5817): 1388–91. Bibcode:2007Sci...315.1388T(/abs/2007Sci...315.1388T). doi:10.1126/science.1137430(/10.1126%2Fscience.1137430). PMID 17255474(https:///pubmed/17255474).Further reading◾Ando, Tsuneya; Matsumoto, Yukio; Uemura, Yasutada (1975). "Theory of Hall Effect in a Two-Dimensional Electron System". J. Phys. Soc. Jpn.39 (2): 279–288.Bibcode:1975JPSJ...39..279A (/abs/1975JPSJ...39..279A).doi:10.1143/JPSJ.39.279 (/10.1143%2FJPSJ.39.279).◾Klitzing, K.; Dorda, G.; Pepper, M. (1980). "New Method for High-Accuracy Determination of the Fine-Structure Constant Based on Quantized Hall Resistance". Phys. Rev. Lett.45 (6): 494–497. Bibcode:1980PhRvL..45..494K(/abs/1980PhRvL..45..494K). doi:10.1103/PhysRevLett.45.494(/10.1103%2FPhysRevLett.45.494).◾Laughlin, R. B. (1981). "Quantized Hall conductivity in two dimensions". Phys. Rev. B.23(10): 5632–5633. Bibcode:1981PhRvB..23.5632L(/abs/1981PhRvB..23.5632L). doi:10.1103/PhysRevB.23.5632(/10.1103%2FPhysRevB.23.5632).◾Yennie, D. R. (1987). "Integral quantum Hall effect for nonspecialists". Rev. Mod. Phys.59(3): 781–824. Bibcode:1987RvMP...59..781Y(/abs/1987RvMP...59..781Y). doi:10.1103/RevModPhys.59.781(/10.1103%2FRevModPhys.59.781).◾Hsieh, D.; Qian, D.; Wray, L.; Xia, Y.; Hor, Y. S.; Cava, R. J.; Hasan, M. Z. (2008). "A topological Dirac insulator in a quantum spin Hall phase". Nature452 (7190): 970–974.arXiv:0902.1356 (https:///abs/0902.1356). Bibcode:2008Natur.452..970H(/abs/2008Natur.452..970H). doi:10.1038/nature06843(/10.1038%2Fnature06843). PMID 18432240(https:///pubmed/18432240).◾25 years of Quantum Hall Effect, K. von Klitzing, Poincaré Seminar (Paris-2004). Postscript (http://parthe.lpthe.jussieu.fr/poincare/textes/novembre2004.html). Pdf(/PhysicsHorizon/25yearsQHE-lecture.pdf).◾Magnet Lab Press Release Quantum Hall Effect Observed at Room Temperature (/mediacenter/news/pressreleases/2007february15.html)◾Avron, Joseph E.; Osadchy, Daniel, Seiler, Ruedi (2003). "A Topological Look at the Quantum Hall Effect" (/resource/1/phtoad/v56/i8/p38_s1).Physics Today56 (8): 38. Bibcode:2003PhT....56h..38A(/abs/2003PhT....56h..38A). doi:10.1063/1.1611351(/10.1063%2F1.1611351). Retrieved 8 May 2012.◾Zyun F. Ezawa: Quantum Hall Effects - Field Theoretical Approach and Related Topics.World Scientific, Singapore 2008, ISBN 978-981-270-032-2◾Sankar D. Sarma, Aron Pinczuk: Perspectives in Quantum Hall Effects. Wiley-VCH, Weinheim 2004, ISBN 978-0-471-11216-7◾Baumgartner, A.; Ihn, T.; Ensslin, K.; Maranowski, K.; Gossard, A. (2007). "Quantum Hall effect transition in scanning gate experiments". Physical Review B76 (8).Bibcode:2007PhRvB..76h5316B (/abs/2007PhRvB..76h5316B).doi:10.1103/PhysRevB.76.085316 (/10.1103%2FPhysRevB.76.085316).◾E. I. Rashba and V. B. Timofeev, Quantum Hall Effect, Sov. Phys. - Semiconductors v. 20, pp.617-647 (1986).Retrieved from "/w/index.php?title=Quantum_Hall_effect&oldid=605304404"Categories: Hall effect Condensed matter physics Quantum electronics SpintronicsQuantum phases Mesoscopic physics◾This page was last modified on 22 April 2014 at 14:51.◾Text is available under the Creative Commons Attribution-ShareAlike License; additional terms may apply. By using this site, you agree to the Terms of Use and Privacy Policy.Wikipedia® is a registered trademark of the Wikimedia Foundation, Inc., a non-profitorganization.。

Gauge Freedom in Chiral Gauge Theory with Vacuum Overlap

Gauge Freedom in Chiral Gauge Theory with Vacuum Overlap

a r X i v :h e p -l a t /9709149v 1 29 S e p 19971RU-97-78KUNS-1465HE(TH)97/14Gauge Freedom in Chiral Gauge Theory with Vacuum Overlap ∗Yoshio Kikukawa a †aDepartment of Physics and Astronomy,Rutgers University,Piscataway,NJ 08855-0849,USADynamical nature of the gauge degrees of freedom and its effect to fermion spectrum are studied at β=∞for two-and four-dimensional nonabelian chiral gauge theories in the vacuum overlap formalism.It is argued that the disordered gauge degrees of freedom does not contradict to the chiral spectrum of lattice fermion.1.Introduction —Pure gauge limit In the vacuum overlap formalism[1]of a generic chiral gauge theory,gauge symmetry is explic-itly broken by the complex phase of fermion de-terminant.In order to restore the gauge invari-ance,gauge average —the integration along gauge orbit—is invoked.Then,what is required for the dynamical nature of the gauge freedom at β=∞(pure gauge limit)is that the global gauge symmetry is not broken spontaneously and the bosonic fields of the gauge freedom have large mass compared to a typical mass scale of the the-ory so as to decouple from physical spectrum[2,1].However,through the analysis of the waveg-uide model[3,4],it has been claimed that this required disordered nature of the gauge freedom causes the vector-like spectrum of fermion[5].In this argument,the fermion correlation functions at the waveguide boundaries were examined.One may think of the counter parts of these correla-tion functions in the overlap formalism by putting creation and annihilation operators in the overlap of vacua with the same signature of mass.Let us refer this kind of correlation function as bound-ary correlation function and the correlation func-tion in the original definition as overlap correla-tion function .We should note that the boundary correlation functions are no more the observables in the sense defined in the overlap formalism;they cannot be expressed by the overlap of two vacua with their phases fixed by the Wigner-Brillouin| +|v + |v +|v −v −|−2Then the model describes the gauge degrees of freedom coupled to fermion through the gauge non-invariant piece of the complex phase of chiral determinants.Z= [dg] rep. +|ˆG|+ | −|ˆG†|− | ≡ dµ[g].(3)ˆG is the operator of the gauge transformation given by:ˆG=exp ˆa†i n{log g}i jˆa nj .(4) In this limit,one of the possible definitions of the boundary correlation functions is given as fol-lows for the case of the negative mass and in the representation r:φniφ†m j −r≡12δnmδj i |− rλ2 .(8)In four-dimensions,we consider the covariantgaugefixing term and the Faddeev-Popov deter-minant[7],following Hata[9](cf.[10–12]):−12i U nµ−U†nµ −12i U nµ−U†nµ ,with the pure gauge link variable Eq.(2).ˆM ab nm isthe lattice Faddeev-Popov operator.We can show by the perturbation theory inλ(backgroundfield method)that both puregauge models share the novel features of the two-dimensional nonlinear sigma model even in thepresense of the imaginary action.The model isrenormalizable(at one-loop in four-dimensions)andλis asymptotically free.Severe infrared di-vergence occurs and it prevents local order pa-rameters from emerging.Based on these dynamical features,we assumethat the global gauge symmetry does not breakspontaneously for the entire region ofλand thegauge freedom acquires mass M g dynamicallythrough the dimensional transmutation.Withthis assumption,the decoupling of the gauge free-dom could occur as M gր133.Boundary correlation functionThe asymptotic freedom allows us to tamethe gaugefluctuation by approaching the criticalpoint of the gauge freedom.There we can invokethe spin wave approximation for the calculationof the invariant boundary correlation functionφniφ†m i −r,(10)which is free from the IR divergence.At one-looporder,we obtain1(2π)D e ip(n−m)1µsin2pµ+(B(p)−m0)2,(14) andπnπm ′= d D p µ4sin2pµ2(1−m0),(m0=0.5).(16)We also see that the quantum correction due to the gaugefluctuation at one-loop does not affect the leading short-distance nature.There is no symmetry against the spectrum mass gap.There-fore it seems quite reasonable to assume that it holds true asλbecomes large.Since the overlap correlation function does not depend on the gauge freedom and does show the chiral spectrum[1],the above fact means that the entire fermion spec-trum is chiral.The author would like to thank H.Neuberger and R.Narayanan for enlightening discussions. He also would like to thank H.Hata,S.Aoki, H.So and A.Yamada for discussions. REFERENCES1.R.Narayanan and H.Neuberger,Nucl.Phys.B412(1994)574;Phys.Rev.Lett.71(1993) 3251;Nucl.Phys.B(Proc.Suppl.)34(1994) 95,587;Nucl.Phys.B443(1995)305.2. D.Foerster,H.B.Nielsen and M.Ninomiya,Phys.Lett.B94(1980)135;S.Aoki,Phys.Rev.Lett.60(1988)2109;Phys.Rev.D38 (1988)618;K.Funakubo and T.Kashiwa, 60(1988)2113;J.Smit,Nucl.Phys.B(Proc.Suppl.)4(1988)451.3. D.B.Kaplan,Nucl.Phys.B30(Proc.Suppl.)(1993)597.4.M.Golterman,K.Jansen,D.Petcher and J.Vink,Phys.Rev.D49(1994)1606;M.F.L.Golterman and Y.Shamir,Phys.Rev.D51 (1995)3026.5.M.F.L.Golterman and Y.Shamir,Phys.Lett.B353(1995)84;Erratum-ibid.B359(1995) 422.R.Narayanan and H.Neuberger,Phys.Lett.B358(1995)303.6.Y.Kikukawa,KUNS-1445HE(TH)97/08,May1997,hep-lat/9705024.7.Y.Kikukawa,KUNS-1446HE(TH)97/09,July1997,hep-lat/9707010.8.Y.Kikukawa and S.Miyazaki,Prog.Theor.Phys.96(1996)1189.9.H.Hata,Phys.Lett.143B(1984)171.10.A.Borrelli,L.Maiani,G.C.Rossi,R.Sistoand M.Testa,Nucl.Phys.B333(1990)335.11.Y.Shamir,TAUP-2306-95,Dec1995;Y.Shamir,Nucl.Phys.B(Proc.Suppl.)53 (1997)664.12.M.F.L.Golterman and Y.Shamir,Phys.Lett.B399(1997)148.13.E.Witten,Commun.Math.Phys.92(1984)455.。

物理学博士研究生培养方案

物理学博士研究生培养方案

物理学博士研究生培养方案(专业代码:0702)一、学科概况西北师范大学的物理学专业为教育部特色建设专业,甘肃省重点学科;具有物理学博士后科研流动站、物理学一级博士点。

建立了原子分子物理与功能材料省级重点实验室,与中科院近物所联合建立了极端环境原子分子物理实验室。

学科点凝聚了一批高学历、高水平、结构合理的学科带头人和学术梯队。

具有享受国务院特殊津贴专家1人,省优秀专家1人,省领军人才5人,省科技创新人才4人,留学回国人员20 余人。

在原子分子物理、理论物理、凝聚态物理、等离子体物理等方向形成了明显特色与优势,在国内外产生了一定影响。

近五年承担国家自然科学基金30余项、省部级项目20余项、国际合作项目2项,年科研经费近一千万元;每年在SCI收录期刊发表论文60多篇,在Phys. Rev.系列等标志性刊物上的论文数逐年增加。

研究成果获甘肃省自然科学奖2项、甘肃省高校科技进步奖7项。

研究生招生规模、培养质量、对外影响稳步提升,与多所国内外著名大学和研究机构建立了稳定的交流合作及研究生联合培养机制;在近几年的《中国研究生教育分专业排行榜》上,原子与分子物理专业被评为A级,物理学一级学科被评价为B+级。

本学科涵盖理论物理、原子与分子物理、等离子体物理、凝聚态物理、光学5个二级学科。

二、培养目标本专业培养的博士研究生应是热爱祖国、学风良好、治学严谨、身心健康,掌握本专业坚实宽广的理论基础和系统深入的专门知识及技能,有较强的创新能力,熟练掌握一门外语,并具有独立从事与物理学专业相关的教学、科研工作的高级专门人才。

三、研究方向1.非线性物理2. 玻色-爱因斯坦凝聚3. 原子结构与原子碰撞4. 强激光场中的原子分子物理5. 基于加速器的原子物理6. 大气环境中的原子分子过程7. 团簇的结构与性质8. 功能薄膜材料结构与物性9. 纳米结构的光电性质四、学习年限及应修学分全日制博士研究生的学习年限一般为3年,在职攻读博士学位研究生的学习年限原则上为4年。

Gauge Invariance and the Pauli-Villars Regulator in Lorentz- and CPT-Violating Electrodynam

Gauge Invariance and the Pauli-Villars Regulator in Lorentz- and CPT-Violating Electrodynam

a rXiv:h ep-th/047172v12J ul24IUHET-473Gauge Invariance and the Pauli-Villars Regulator in Lorentz-and CPT-Violating Electrodynamics B.Altschul 1Department of Physics Indiana University Bloomington,IN 47405USA Abstract We examine the nonperturbative structure of the radiatively induced Chern-Simons term in a Lorentz-and CPT-violating modification of QED.Although the coefficient of the induced Chern-Simons term is in general undetermined,the nonperturbative theory appears to generate a definite value.However,the CPT-even radiative corrections in this same formulation of the theory generally break gauge invariance.We show that gauge invariance may yet be preserved through the use of a Pauli-Villars regulator,and,contrary to earlier expectations,this regulator does not necessarily give rise to a vanishing Chern-Simons term.Instead,two possible values of the Chern-Simons coefficient are allowed,one zero and one nonzero.This formulation of the theory therefore allows the coefficientto vanish naturally,in agreement with experimental observations.One of the most interesting terms that arises in the study of Lorentz-and CPT-violating corrections to the standard model action[1,2,3]is the electromagnetic Chern-=1Simons term,with Lagrange density LFµνFµν+¯ψ(i∂−m−e A− bγ5)ψ.(1)4This theory has the potential to induce afinite radiatively-generated Chern-Simons term, with∆k CS proportional to b.However,the coefficient of proportionality depends upon the regularization[10,11,12].If the regulator used enforces the gauge invariance of the induced Lagrange density,then∆k CS must necessarily vanish[13];however,this is not particularly interesting,because it excludes the existence of a Chern-Simons term a priori.Other regulators lead to different values of∆k CS,and through a suitable choice, any coefficient of proportionality between the two may be found.This ambiguity has been extensively studied,and several potentially interesting values of∆k CS have been identified[11,14,15,16,17,18].Most notably,if the theory is defined nonperturbatively in b,then the ambiguity is lessened,and a single value appears to be preferred[10,11,14]. However,since this value is nonzero,there is a potential for conflict with the observed vanishing of k CS.We shall continue the analysis of the nonperturbatively-defined theory.While the in-duced Chern-Simons term itself has been extensively studied,the higher-order,CPT-even corrections to this theory have largely been neglected.In a nonperturbatively defined the-ory,the terms of all orders in b are tied together,and so information about the CPT-even terms may help clarify the structure of the CPT-odd Chern-Simons term.We have pre-viously demonstrated[19]that the O(b2)terms in the photon self-energy may violate the Ward identity that enforces the transversality of the vacuum polarization—pµΠµν(p)=0; however,our calculation was limited to the case of m=0.We shall demonstrate here that the same result holds in the opposite limit,when|b2|≪m2(which represents the physi-cal regime for all electrically charged elementary particles).This failure of transversality could represent a significant problem for the nonperturbative formulation of the theory. However,this difficulty may be overcome through the use of a Pauli-Villars regulator. Introducing such a regulator changes the nature of the ambiguity in the Chern-Simons term.When the Ward-identity-violating terms are eliminated,we are left with a theory1in which the coefficient∆k CS of the induced Chern Simons term is not in any way forced to vanish,yet it still may vanish quite naturally.This may represent a resolution of the physical paradox described above.We shall calculate the O(b2)contribution to the zero-momentum photon self-energy,Πµν(p=0),under the assumption thatΠµν(p)may be expanded as a power series in b. However,we do not expect this assumption to be generically valid.The exact fermion propagator,iS(l)=.(3)(l2−m2−b2)2+4[l2b2−(l·b)2]At l=0,the denominator of the rationalized propagator becomes(m2+b2)2.The square root|m2+b2|of this expression arises in the calculation ofΠµν(p=0),and the absolute value leads to behavior that is nonanalytic in b.The b-odd portion of the self-energy(which is just the Chern-Simons term)has different forms for−b2≤m2=0,−b2<m2=0,and m=0.For the b-even terms,we also expect the power-series representation of the self-energy to break down at b2=−m2;moreover,there may exist other thresholds for nonanalytic behavior as well.We shall therefore restrict our attention to the regime in which|b2|≪m2.Since large values of b2are excluded for most physical particles,this is a reasonable restriction.To control the high-energy behavior of our theory,we shall use a Pauli-Villars regula-tor.By utilizing this method of regulation,we may deal with the usual divergences that arise in the photon self-energy[at O(b0)],as well as the Ward-identity-violating terms that appear at O(b2).The use of a single regulator at all orders in b is necessary,because in the nonperturbative formalism,there is actually only a single Feynman diagram that contributes to the photon self-energy at O(e2).This diagram is the usual QED vacuum polarization,but with the usual fermion propagator replaced by the b-exact S(l).We shall use a symmetric integration prescription in our calculation,because this is appropriate at O(b0),and it preserves the expected transformation properties of the loop integral. (Moreover,without symmetric integration,additional ambiguities in∆k CS would exist.) The Pauli-Villars regularization of the photon self-energy involves the introduction of afictitious species of heavy fermions,whose contribution to the self-energy is subtractive. This subtraction renders the Lorentz-invariant part of the self-energyfinite and preserves its gauge invariance.Previously,it has been believed that the same subtraction will cause the O(b)Chern-Simons term to vanish.However,we shall show that this is not necessarily the case.Thefictitious Pauli-Villars particles have the exact propagatoriS M(l)=where M is the particles’large mass,and b M is the Lorentz-violating coefficient appropri-ate to thesefictitious particles.Previous analyses have assumed that b M=b,and indeed this must be the case in a perturbatively defined theory,in which the b interaction is treated as a vertex.However,in the nonperturbative formulation,this restriction is ab-sent,and b and b M exist as distinct objects.Depending upon what properties we demand for the self-energy,b M may take on different values.Even if we place quite strong(yet quite natural)conditions on the form ofΠµν(p),we are still left with a discrete freedom in our choice of b M;either b M=b or b M=−b will suffice.In fact,the weakest condition that we may place upon b M is no condition at all.If we choose not to worry about the failure of the Ward identity at O(b2),then the only restriction on the Pauli-Villars propagator is that it must cancel the divergences at O(b0). In that case,any value of b M is acceptable.We might be tempted to choose a vanishing b M,which would produce a formulation of the theory equivalent to that used in[10]. However,since Lorentz violation is already present in the theory,there is no reason to prefer this value.Similarly,the choice b M=b,while aesthetically pleasing,has nothing special to recommend it.We are left with an arbitrary b M,which will generate an arbitrary Chern-Simons term.Moreover,since b and b M need not point in the same direction,the coefficient∆k CS of the induced Chern-Simons term need not even be parallel to b;this is an even greater degree or arbitrariness in∆k CS than has been found previously.The above scenario illustrates an interesting point.In the theory as we have described it,there can exist a radiatively-induced Chern-Simons term even if b vanishes,because the regulator involves the Lorentz-violating parameter b M.In a general Lorentz-violating quantumfield theory,the Lagrange density need not be the only source of the viola-tion.The regularization prescription can also break Lorentz invariance,and the Lorentz violation of the regulator need not be determined by the behavior of any terms in the unrenormalized action.It may seem somewhat unnatural for the regulator to become an additional source of Lorentz violation.However,it is well established thatfictitious Pauli-Villars fermions may generate radiative corrections that are qualitatively different from those generated by a theory’s real fermions.For example,in massless QED,with a Pauli-Villars regulator,it is thefictitious heavy particles which are solely responsible for the anomalous nonconservation of the axial vector and dilation currents.However,the specific scenario presented in the previous paragraph is probably unrealistic,because we had to abandon the Ward identity in order to avoid placing any restrictions on b M.The key to developing a more sophisticated theory—one in which gauge invariance holds at all orders—is the determination of the O(b2)part of the self-energy.Since we are only interested in the situation in which we may expandΠµν(p)as a power series in b, we may use the approximation scheme developed in[10]to expand the exact propagator to second order in b.WefindS(l)≈il−m(−i bγ5)il−m(−i bγ5)il−m.(5)Naively,this might appear equivalent to treating the b term as an interaction vertex.3However,there are subtle differences that characterize our nonperturbative approach; since there is only a single diagram,there is a complex interplay between terms at different orders in b.The one-loop photon self-energy isΠµν(p)=−ie2 d4k(2π)4tr γµi k−mγνi k−mγµi k−m(−i bγ5)i k−m+(µ↔ν) .(7)=ie2 d4k(k2−m2)4tr{γµ(k+m)b(k−m)γν(k−m)b(k+m) +[γµ(k+m)γν(k+m)b(k−m)b(k+m)+(µ↔ν)]}(8)The only Lorentz structures that may be present inΠµνb2(0)are bµbνand gµνb2,so itis simplest to evaluate the self-energy by calculating gµνΠµνb2(0)and bµbν(2π)4tr{[2(k b k−m2b)+4(k−2m)(k+m)b](k−m)b(k+m)}(2π)416m2[2(b·k)2−b2k2]−10m4b24π2.(11)4Similarly,we also havebµbνb2 d4k(k2−m2)4(12)=−4ie2 d4k(k2−m2)4(13)e2b2=−24π2 2bµbν+gµνb2 .(15) This is the same result that we found previously in the m=0case[19].Since pµ(2bµbν+ gµνb2)=0,there is the potential for a violation of gauge invariance.However,since we are using a Pauli-Villars regularization,there is also a contribution fromΠµνM(p)that is second order in b M.This contribution is precisely e2bµ;(16)8π2this is twice the value found in[10,11,14],since there are equal contributions from b and b M.This is a novel situation.Unambiguouslyfinite yet undetermined radiative corrections generally involve continuously variable parameters that describe the arbitrariness of the results[20],and indeed,in more general formulations of the theory we are discussing,there is a continuous ambiguity in the induced Chern-Simons term.However,in this instance, only a discrete set of values for∆k CS is allowed.Since zero is one of these allowed values, this formulation allows for the existence of a gauge-invariant Lagrange density,but it does not force the density to be so invariant.The Pauli-Villars formulation therefore allows the theory to possess a naturally vanishing induced Chern-Simons term without externally enforcing the gauge invariance of the Lagrange density.Moreover,since the Pauli-Villars regulator is covariant,it should be possible to generalize our calculations to occur in a weakly curved spacetime[21].As we remarked in[19],the O(b)and O(b2)terms in the photon self-energy both violate gauge invariance in the strongest fashions that are allowed by their tensor structures.5The Chern-Simons term violates the gauge invariance of the Lagrange density;however, because the induced density necessarily involves the antisymmetricǫ-tensor,the Wardidentity is preserved and the integrated action remains gauge invariant.Πµνb2(p)possessesno such special structure,and so it violates the Ward identity explicitly.In order to ensure gauge invariance,we have therefore been forced to place a very strong condition on the tensor structure of the second-order correction to the self-energy;we have insisted that it must vanish at p=0.Since there is more than one way to enforce this condition, we have found more than one possible value for∆k CS.This is the origin of the discrete ambiguity in this formulation of the theory.We may now ask what may happen if the mass scale m2is not large compared with the Lorentz-violation scale|b2|.When the real fermions are massless,their O(b2)contributiontoΠµν(p)is exactly theΠµνb2(0)of equation(15).In this instance,as in the|b2|≪m2case,the use of a power series expansion to determine the second-order portion of the photon self-energy is justified,so the similarity of the results is somewhat unsurprising. If a Pauli-Villars regulator is used in this case,the Ward identity may be preserved,but the Chern-Simons term cannot be made to vanish.The choice is between∆kµCS=e24π2bµ.So this formulation of the theory does not allow for∆k CS to vanishnaturally if there are massless fermions coupled to the gaugefield.When a power series expansion in b is not justified,the gauge noninvariant portions of the self-energy must be calculated directly from the nonperturbative propagator(3). Only if the result is of the form A(b2)bµbν+B(b2)gµνb2,with A(b2)=2B(b2)≤0,will the Pauli-Villars regulator be capable of restoring the Ward identity.If we do choose to use a Pauli-Villars regulator and also insist upon gauge invariance as a requirement of our theory,then any breakdowns of the Ward identity when|b2|≪m2can be interpreted as giving restrictions on the allowed values of b.Applied to the standard model,this could imply that the scale of b-generated Lorentz violation should be smaller than the smallest nonzero fermionic mass scale present.However,this is all merely conjectural,since we do not know the general form taken by the self-energy when|b2|≪m2,and because of the substantial additional complexity of the standard model.This work has demonstrated that there exist new,unexpected subtleties in the struc-ture of the radiatively-induced Chern-Simons term.We have identified new types of ambiguities in the value of the Chern-Simons coefficient;these ambiguities are derived from the use of a Pauli-Villars regulator and a nonperturbative formulation of the theory. If we do not insist that the Ward identity hold at second order,then the coefficient is completely arbitrary and is not even constrained to be parallel to b.However,if,more reasonably,we do insist on transversality of the vacuum polarization at higher orders, then there is a binary ambiguity in the value of the induced coefficient.If m=0,either of two nonzero values for∆k CS is allowed.However,if|b2|≪m2,then∆k CS=0is allowed, in addition to a particular nonzero value.This may provide a satisfactory explanation for why the electromagnetic Chern-Simons coefficient vanishes in nature.6AcknowledgmentsThe author is grateful to V.A.Kosteleck´y,M.P´e rez-Victoria,and R.Jackiw for many helpful discussions.This work is supported in part by funds provided by the U.S.Depart-ment of Energy(D.O.E.)under cooperative research agreement DE-FG02-91ER40661. References[1]D.Colladay,V.A.Kosteleck´y,Phys.Rev.D55,6760(1997).[2]D.Colladay,V.A.Kosteleck´y,Phys.Rev.D58,116002(1998).[3]V.A.Kosteleck´y,R.Lehnert,Phys.Rev.D63,065008(2001).[4]R.Jackiw,S.Templeton,Phys.Rev.D23,2291(1981).[5]J.Schonfeld,Nucl.Phys.B185,157(1981).[6]S.M.Carroll,G.B.Field,R.Jackiw,Phys.Rev.D41,1231(1990).[7]S.M.Carroll,G.B.Field,Phys.Rev.Lett.79,2394(1997).[8]M.Goldhaber,V.Trimble,J.Astrophys.Astron.17,17(1996).[9]V.A.Kosteleck´y,ne,A.G.M.Pickering,Phys.Rev.D65,056006(2002).[10]R.Jackiw,V.A.Kosteleck´y,Phys.Rev.Lett.82,3572(1999).[11]M.P´e rez-Victoria,Phys.Rev.Lett.83,2518(1999).[12]M.P´e rez-Victoria,JHEP04,032(2001).[13]S.Coleman,S.L.Glashow,Phys.Rev.D59,116008(1999).[14]J.M.Chung,Phys.Lett.B461,138(1999).[15]J.M.Chung,P.Oh,Phys.Rev.D60,067702(1999).[16]W.F.Chen,Phys.Rev.D60,085007(1999).[17]J.M.Chung,Phys.Rev.D60,127901(1999).[18]A.A.Andrianov,P.Giacconi,R.Soldati,JHEP02,030(2002).[19]B.Altschul,Phys.Rev.D69,125009(2004).[20]R.Jackiw,Int.J.Mod.Phys.B14,2011(2000).[21]V.A.Kosteleck´y,Phys.Rev.D6*******(2004).7。

A Systematic Approach to Confinement in N=1 Supersymmetric Gauge Theories

A Systematic Approach to Confinement in N=1 Supersymmetric Gauge Theories

a r X i v :h e p -t h /9610139v 1 17 O c t 1996hep-th/9610139MIT-CTP-2581BUHEP-96-41A Systematic Approach to Confinement in N =1Supersymmetric Gauge TheoriesCsaba Cs´a ki a ,Martin Schmaltz b and Witold Skiba aaCenter for Theoretical Physics Laboratory for Nuclear Science and Department of Physics Massachusetts Institute of Technology Cambridge,MA 02139,USA csaki@,skiba@ b Department of Physics Boston University Boston,MA 02215,USA schmaltz@ Abstract We give necessary criteria for N =1supersymmetric theories to be in a smoothly confining phase without chiral symmetry breaking and with a dynamically generated ing our general arguments we find all such confining SU and Sptheories with a single gauge group and no tree level superpotential.Following the initial breakthrough in the works of Seiberg on exact results in N=1supersymmetric QCD(SQCD)[1],much progress has been made in extending these results to other theories with different gauge and matterfields[2-11].We now have a whole zoo of examples of supersymmetric theories for which we know results about the vacuum structure and the infrared spectrum.A number of theories are known to have dual descriptions,others are known to confine with or without chiral symmetry breaking,and some theories do not possess a stable ground state.Unfortunately,we are still lacking a systematic and general approach that allows one to determine the infrared properties of a given theory.The results in the literature have mostly been obtained by an ingenious guess of the infrared spectrum.This guess is then justified by performing a number of non-trivial consistency checks which include matching of the global anomalies,detailed study of the moduli space of vacua, and the behavior of the theory under perturbations.In this letter,we will depart from the customary trial and error procedure and give some general arguments which allow us to classify a subset of supersymmetric theories. To be specific,we intend to answer the general question of which supersymmetricfield theories may be confining without chiral symmetry breaking and with a confining superpotential.We present a few simple arguments which allow us to rule out most theories as possible candidates for confinement without chiral symmetry breaking.For the most part,these arguments already exist in the literature but our systematic way of putting them to use is new.As a demonstration of the power of our arguments we give a complete list of all SU(N)and Sp(N)gauge theories with no tree level superpotential which confine without chiral symmetry breaking,and we determine the confined degrees of freedom and the superpotential describing their interactions (“confining superpotential”).To begin,let usfirst explain what we mean by“smooth confinement without chiral symmetry breaking and with a non-vanishing confining superpotential”,which,from now on,we will abbreviate by s-confinement.We will call a theory confining when its infrared physics can be described exactly in terms of gauge invariant composites and their interactions.This description has to be valid everywhere on the moduli space of vacua.Our definition of s-confinement also requires that the theory dynamically generates a confining superpotential,which excludes models of the type presented in Ref.[11].Furthermore,the phrase“without chiral symmetry breaking”implies that the origin of the classical moduli space is also a vacuum in the quantum theory.In this vacuum,all the global symmetries of the ultraviolet remain unbroken.Finally,the confining superpotential is a holomorphic function of the confined degrees of freedom and couplings,which describes all the interactions in the extreme infrared.Note that this definition excludes theories which are in a Coulomb phase on a submanifold of the moduli space[2],or theories which have distinct Higgs and confining phases with associated phase boundaries on the moduli space.Our prototype example for an s-confining theory is Seiberg’s SQCD[1]with the number offlavors F chosen to equal N+1,where N is the number of colors,and a“flavor”is a pair of matterfields in the fundamental and antifundamental represen-tations of SU(N).Seiberg argued that the matterfields Q and¯Q are confined into “mesons”M=Q¯Q and“baryons”B=Q N,¯B=¯Q N.At the origin of moduli space all components of the mesons and baryons are massless and interact via the confining superpotential1W=1We normalize the index of the fundamental representation to1.integers.Therefore2, jµj−µ(G)=1or2,and for SU and Sp theories anomaly cancellation further constrainsjµj−µ(G)=2.(3)This formula constitutes a necessary condition for s-confinement,it enables us to rule out most theories immediately.For example,for SQCD wefind that the only candidate theory is the theory with F=N+1.Unfortunately,Eq.3is not a sufficient condition.An example for a theory which satisfies Eq.3but does not s-confine is SU(N)with an adjoint superfield and oneflavor.This theory is easily seen to be in an Abelian Coulomb phase for generic VEVs of the adjoint scalars and vanishing VEVs for the fundamentals.We could now simply examine all theories that satisfy Eq.3byfinding all in-dependent gauge invariants and checking if this ansatz for the confining spectrum matches the anomalies.Apart from being very cumbersome,this method is also not very useful to demonstrate that a given theory satisfying Eq.3is not s-confining.A better strategy relies on our second observation.An s-confining theory with a smooth description in terms of gauge invariants at the origin must also be s-confining everywhere on its moduli space.This is because the confining superpotential at the origin which is a simple polynomial in thefields is analytical everywhere,and no additional massless states are present anywhere on the moduli space.Therefore,the theory restricted to a particularflat direction must have a smooth description as well. This observation has two very useful applications.First,if we have a theory that s-confines and we know its confined spectrum and superpotential,we can easilyfind new s-confining theories by going to different points on moduli space.In the ultraviolet description,the gauge group is broken to a sub-group of the original group,some matterfields are eaten by the Higgs mechanism, and the remaining ones decompose under the unbroken subgroup.The corresponding confined description is obtained by simplyfinding the corresponding point on the moduli space of the confined theory.The global symmetries will be broken in the same way,and somefields may be massive and can be integrated out.This newly found confined theory is guaranteed to pass all the standard consistency checks be-cause they are a subset of the consistency checks for the original theory.For example, the anomalies of the new s-confining theory are guaranteed to match:the unbroken global symmetries are a subgroup of original global symmetries,and the anomalies under the subgroup are left unchanged–both in the infrared and ultraviolet descrip-tions–because the fermions which obtain masses give cancelling contributions to the anomalies.Second,the above observation can be turned around to provide another necessary condition for s-confinement.If anywhere on the moduli space of a given theory we find a theory which is not s-confining or completely higgsed,we know that the original theory cannot be s-confining either.Let us study some examples.Suppose we knew that SU(N)with N+1flavors for some large N is s-confining,then we could immediately conclude that the theories with n<N also s-confine.We simply need to give a VEV to some of the quark-antiquark pairs to break SU(N)to any SU(n)subgroup.The quarks with vevs are eaten,leaving n+1flavors and some singlets.We remove these singlets by adding “mirror”superfields with opposite global charges and giving them a mass.We now identify the corresponding point on the moduli space of the confined SU(N)theory. Somefields obtain masses from the superpotential of Eq.1when we expand around the new point in moduli space.After integrating the massivefields and removing the fields corresponding to the singlets in the ultraviolet theory via masses with mirror partners,we obtain the correct confined description of SU(n).A non-trivial example of a theory which can be shown to not s-confine is SU(4) with three antisymmetric tensors and twoflavors.This theory satisfies Eq.3and is therefore a candidate for s-confinement.By giving a VEV to an antisymmetric tensor we canflow from this theory to Sp(4)with two antisymmetric tensors and four fundamentals.VEVs for the other antisymmetric tensors let usflow further to SU(2) with eight fundamentals which is known to be at an interactingfixed point in the infrared.We conclude that the SU(4)and Sp(4)theories and all theories thatflow to them cannot be s-confining either.This allows us to rule out the following chain of theories,all of which are gauge anomaly free and satisfy Eq.3SU(7)→SU(6)→SU(5)→SU(4)→Sp(4)(4)432232Note that a VEV for one of the quarkflavors of the SU(4)theory lets usflow to an SU(3)theory with fourflavors which is s-confining.We must therefore be careful, when wefind aflow to an s-confining theory,it does not follow that the original theory is s-confining as well.Theflow is only a necessary condition.However,we suspect that a theory with a single gauge group and no tree-level superpotential is s-confining if it is found toflow to s-confining theories in all directions of its moduli space.We do not know of any counter examples.Armed with formula in Eq.3and our observation onflows of s-confining theories, we were able tofind all s-confining SU and Sp gauge theories with a single gauge group and no tree-level superpotential for arbitrary tensor representations.To achieve this, wefirst found all possible matter contents satisfying Eq.3.We list all these theories in Table1.We then studied the possibleflows of these theories and discarded all those withflows to theories which do not s-confine.This process eliminated all except about a dozen theories for which we then explicitly determined the independent gaugeinvariants and matched anomalies tofind the confining spectra.These results are summarized in Table1.Six of the ten theories which s-confine are new3:SU(N)with++3, SU(7)with2+6,SU(6)with2++4+4,and SU(5)with3+3.For the theories which do not s-confine we indicated the method by which we obtained this result:either by noting that the theory has a branch with only unbroken U(1)gauge groups,or else byflowing along aflat direction to a theory with smaller non-Abelian gauge group which does not s-confine.Detailed results on the new theories including the confining spectra,superpoten-tials,variousflows,and consistency checks will be reported elsewhere[14].Here,we just point out a few salient features.Most of the new s-confining theories contain vector-like matter.Perturbing these theories by adding mass terms for some of the vector-like matter,we easily obtain exact results on the theories with the matter integrated out.Among the theories that wefind in this way are new theories which confine with chiral symmetry breaking, theories with runaway vacua,and theories which confine without chiral symmetry breaking and vanishing superpotentials.Since many of the new theories presented here are chiral,they can be used tofind models of dynamical supersymmetry breaking along the lines of Refs.[15].Examples for such supersymmetry breaking theories will also be included in the detailed paper[14].Our s-confining theories might be used for building extensions of the standard model with composite quarks and leptons[16].Finally,we comment on possible exceptions and generalizations of our arguments.A possible exception to our condition in Eq.3arises,when allµi andµ(G)have a common divisor.Then the superpotential Eq.2can be holomorphic even when jµj−µ(G)= 2.However,whereas Eq.3is preserved under mostflows,the property that allµ’s have a common divisor is not.Therefore,such theoriesflow to theories which are not s-confining,and by our second necessary condition the original theory is not s-confining either.Another possibility is that the confining superpotential vanishes,and the confined degrees of freedom are free in the infrared.This can only happen if there are no clas-sical constraints among the basic gauge invariant operators which satisfy the’t Hooft anomaly matching conditions,otherwise the quantum solution would not have the correct classical limit.Examples of theories which are believed to confine in this way can be found in the literature[7,11,14].Generalizations to SO(N)groups are not completely straightforward because in the case of SO(N)theories“exotic composites”containing the chiral superfield Wαmight appear in the infrared spectrum and superpotential,thus modifying our argu-ment and result of Eq.3.SU(N)(N+1)(s-confiningSU(N)+N+4s-confiningSU(N)++)+SU(4)Adj++)SU(4)4+SU(2):+4Coulomb branchSU(5)3(+)+4)SU(5)2++) SU(6)2+5+s-confiningSU(6)2+SU(4):3+2(+4(s-confiningSU(6)+2+ ++Sp(6):SU(6)2+)SU(7)2(+3)+4+2SU(6):SU(7)+Sp(6):Sp(2N)(2N+4)s-confiningSp(2N)+6s-confiningSp(2N)+2Coulomb branchSp(4)3+2SU(2):+4SU(2):2Sp(6)2+2Sp(4):2+4+5Sp(4):2+4++SU(2):+4Sp(8)2Generalizations to theories with more than one gauge group or tree level super-potentials are more difficult.The additional interactions break some of the global symmetries which are now not sufficient to completely determine the functional form of the confining superpotential.Another complication is that in these theories theflat directions of the quantum theory are sometimes difficult to identify.Since our second argument only applies toflows in directions which are on the quantum moduli space, incorrect conclusions would be obtained fromflows along classicalflat directions which are notflat in the quantum theory.In summary,we have discussed general criteria for s-confinement and used them tofind all s-confining theories with SU(N)or Sp(2N)gauge groups.It is a pleasure to thank P.Cho,A.Cohen,N.Evans,L.Randall,and R.Sundrum for useful discussions.We also thank B.Dobrescu,A.Nelson,and J.Terning for comments on the manuscript. C.C.and W.S.are supported in part by the U.S. Department of Energy under cooperative agreement#DE-FC02-94ER40818.M.S.is supported by the U.S.Department of Energy under grant#DE-FG02-91ER40676. References[1]N.Seiberg,Phys.Rev.D49,6857(1994),hep-th/9402044;Nucl.Phys.B435,129(1995),hep-th/9411149.[2]K.Intriligator and N.Seiberg,Nucl.Phys.B431,551(1994),hep-th/9408155.[3]E.Poppitz and S.Trivedi,Phys.Lett.365B,125(1996),hep-th/9507169;P.Pouliot,Phys.Lett.367B,151(1996),hep-th/9510148.[4]K.Intriligator and P.Pouliot,Phys.Lett.353B,471(1995),hep-th/9505006.[5]P.Cho and P.Kraus,hep-th/9607200.[6]C.Cs´a ki,W.Skiba and M.Schmaltz,hep-th/9607210.[7]K.Intriligator and N.Seiberg,Nucl.Phys.B444,125(1995),hep-th/9503179.[8]P.Pouliot,Phys.Lett.359B,108(1995),hep-th/9507018;P.Pouliot and M.Strassler,Phys.Lett.370B,76(1996),hep-th/9510228;Phys.Lett.375B,175 (1996),hep-th/9602031.[9]I.Pesando,Mod.Phys.Lett.A10,1871(1995),hep-th/9506139;S.Giddingsand J.Pierre Phys.Rev.D52,6065(1995),hep-th/9506196.[10]K.Intriligator,R.G.Leigh,and M.J.Strassler,Nucl.Phys.B456,567(1995),hep-th/9506148;K.Intriligator,R.Leigh,and N.Seiberg,Phys.Rev.D50,1092 (1994),hep-th/9403198;D.Kutasov,Phys.Lett.351B,230(1995);D.Kutasovand A.Schwimmer,Phys.Lett.354B,315(1995);D.Kutasov,A.Schwimmer, and N.Seiberg,Nucl.Phys.B459,455(1996),hep-th/9510222;M.Luty,M.Schmaltz and J.Terning,hep-th/9603034;N.Evans and M.Schmaltz,hep-th/9609183.[11]K.Intriligator,N.Seiberg and S.Shenker,Phys.Lett.342B,152(1995),hep-th/9410203.[12]I.Affleck,M.Dine,and N.Seiberg,Nucl.Phys.B256,557(1985).[13]A.Nelson,private communication.[14]C.Cs´a ki,M.Schmaltz,and W.Skiba,to appear.[15]M.Dine,A.Nelson,Y.Nir and Y.Shirman,Phys.Rev.D53,2658(1996),hep-ph/9507378;K.Intriligator and S.Thomas,Nucl.Phys.B473,121(1996), hep-th/9603158;E.Poppitz,Y.Shadmi and S.Trivedi,hep-th/9605113,hep-th/9606184;C.Cs´a ki,L.Randall and W.Skiba,hep-th/9605108;C.Cs´a ki,L.Randall,W.Skiba and R.Leigh,hep-th/9607021.[16]A.Nelson and M.Strassler,hep-ph/9607362;A.Cohen,D.Kaplan and A.Nel-son,hep-ph/9607394.。

GW Invariants and Invariant Quotients

GW Invariants and Invariant Quotients
1991 Mathematics Subject Classification. 14H10, 14L30.
1
2
GW INVARIANTS AND INVARIANT QUOTIENTS
precise meaning of the notations will be given later on): ˆ := exp.dim M g,k (X/ ˆ) = (3 − dim X/ ˆ + k, D /G, A /G)(g − 1) + c1 (X/ /G) · A /G D − dim G := exp . dim .M g,k (X, A)/ = (3 − dim X )(g − 1) + c1 (X ) · A + k − dim G, and therefore ˆ − (D − dim G) = g · dim G. (⋆) D ˆ) is larger From this computation we deduce that in general the space M g,k (X/ /G, A than M g,k (X, A)/ /G, the only exception happening in genus zero. Very shortly, the explanation for this phenomenon is that the projective line is the only one smooth curve which has the property that a topologically trivial, holomorphic principal G-bundle over it is also holomorphically trivial. In higher genera, holomorphic principal G-bundles with fixed topological type depend on ‘moduli’, whose number agrees with the difference (⋆) above. This is the reason why for computing higher ˆ we will need to consider maps into a larger variety X ¯ whose genus invariants of X construction, in the case when G is a torus, is given in lemma 6.1. The article is organized as follows: the first section recalls some basic facts about stable maps and their moduli spaces, the reference being [9]. In section 2 we describe the G-semi-stable points of the moduli space of stable maps M g,k (X, A). The results obtained in this section hold in full generality, no matter what the G-action on X looks like. We obtain the sufficient result (theorem 2.5) which says that a map with image contained in the semi-stable locus of X is G-semi-stable as a point of M g,k (X, A) and a necessary result (corollary 2.4) which says that a stable map representing a G-semi-stable point of M g,k (X, A) does not have its image contained in the unstable locus of X . Section 3 characterizes the semi-stable points of M g,k (X, A) from a symplectic point of view, which will be useful later on in section 6 where we will give an algebro-geometric construction of the space of maps needed for defining certain ‘Hamiltonian invariants’. We compute an explicit formula for the moment map on the space of stable maps which corresponds to a C∗ -action (proposition 3.4), and using it we give (theorem 3.7) a second proof for theorem 2.5. Finally, section 4 closes the first part of the article giving a partial answer to the initial problem, that of comparing the genus zero GW-invariants of X and X/ /G. Theorem 4.1 states, under certain transversality assumptions which are technical in nature, that if G acts freely on the semi-stable locus of X , A is a spherical class for which a representative may be found to lie entirely in the stable locus X ss and ˆ denotes the push-forward class in X/ A /G, then

Improved Nonrelativistic QCD for Heavy Quark Physics

Improved Nonrelativistic QCD for Heavy Quark Physics

• Finite Lattice Spacing. As in all lattice simulations, there are errors resulting from the discretization of space and time. For our systems, such errors are O(a2 p2 ) and O(aK ), where a is the lattice spacing and p and K are the typical three-momentum and kinetic energy of a quark in the hadron. Since typically a ∼ 1/M , where M is the quark mass, these errors are roughly the same order as those due to relativity. These may also be systematically removed by correcting the heavy-quark action. • Radiative Corrections. As in the Dirac action, the basic action in NRQCD contains only two parameters: the QCD coupling constant g , and the quark mass M .3 However, each of the new interactions added to NRQCD to correct for relativity or finite lattice spacing introduces a new coupling constant. These new couplings can be treated as free parameters, to be adjusted by fitting to experimental data, but this significantly reduces the predictive power of a simulation. Alternatively one can try to compute these couplings in terms of g and M using perturbation theory, thereby reducing the number of parameters back to two. The radiative corrections to these coupling constants are determined by physics at distances of order the lattice spacing a, and therefore perturbation theory should be applicable provided a is small enough. However, a must not be too small. NRQCD is nonrenormalizable, and as a result the radiative corrections contain power-law ultraviolet divergences, like g 2 /aM , which make perturbation theory useless unless a ∼ 1/M or larger. Lattice spacings currently in use, where g 2 ≈ 1, are probably suitable for both c and b quarks, and also seem small enough for perturbation theory to work. Radiative corrections of order 20–40% could easily result, making these among the largest contributions at the order we are considering. We will see that they are well estimated using mean-field theory techniques. Uncalculable corrections due to nonperturbative physics at short distances could be of order a few percent. • Finite Lattice Volume. Quarkonium hadrons are much smaller than

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C e n t r u m v o o r W i s k u n d e e n I n f o r m a t i c aPNAProbability, Networks and AlgorithmsProbability, Networks and AlgorithmsAn image retrieval system based on adaptive waveletliftingP.J. Oonincx, P.M. de ZeeuwR EPORT PNA-R0208 M ARCH 31, 2002CWI is the National Research Institute for Mathematics and Computer Science. It is sponsored by the Netherlands Organization for Scientific Research (NWO).CWI is a founding member of ERCIM, the European Research Consortium for Informatics and Mathematics. CWI's research has a theme-oriented structure and is grouped into four clusters. Listed below are the names of the clusters and in parentheses their acronyms.Probability, Networks and Algorithms (PNA)Software Engineering (SEN)Modelling, Analysis and Simulation (MAS)Information Systems (INS)Copyright © 2001, Stichting Centrum voor Wiskunde en InformaticaP.O. Box 94079, 1090 GB Amsterdam (NL)Kruislaan 413, 1098 SJ Amsterdam (NL)Telephone +31 20 592 9333Telefax +31 20 592 4199ISSN 1386-3711CWIP.O.Box94079,1090GB Amsterdam,The NetherlandsPatrick.Oonincx,Paul.de.Zeeuw@cwi.nl1.I NTRODUCTIONContent-based image retrieval(CBIR)is a widely used term to indicate the process of retrieving desired images from a large collection on the basis of features.The extraction process should be automatic(i.e. no human interference)and the features used for retrieval can be either primitive(color,shape,texture) or semantic(involving identity and meaning).In this paper we confine ourselves to grayscale images of objects against a background of texture.This class of images occurs for example in various databases created for the combat of crime:stolen objects[21],tyre tracks and shoe sole impressions[1].In this report we restrict ourselves to the following problem.Given an image of an object(a so-called query)we want to identify all images in a database which contain the same object irrespective of translation,rotation or re-sizing of the object,lighting conditions and the background texture.One of the most classical approaches to the problem of recognition of similar images is by the use of moment invariants[11].This method is based on calculating moments in both the-and-direction of the image density function up to a certain order.Hu[11]has shown that certain homogeneous polynomials of these moments can be used as statistical quantities that attain the same values for images that are of the same class,i.e.,that can be obtained by transforming one single original image(affine transforms and scaling).However,this method uses the fact that such images consists of a crisp object against a neutral background.If the background contains‘information’(noise,environment in a picture)the background should be the same for all images in one class and should also be obtained from one background using the same transformations.In general this will not be the case.The kind of databases we consider in this paper consists of classes of different objects pasted on different background textures.To deal with the problem of different backgrounds one may use somefiltering process as a preprocessing step.In Do et al.[7]the wavelet transform modulus maxima is used as such preprocessing step.To measure the(dis)similarity between images,moments of the set of maxima points are determined(per scale)and subsequently Hu’s invariants are computed.Thus,each image is indexed by a vector in the wavelet maxima moment space.By its construction,this vector predominantly represents shapes.In this report we propose to bring in adaptivity by using different waveletfilters for smooth and unsmooth parts of the image.Thefilters are used in the context of the(redundant)lifting scheme[18].The degree2of”smoothness”is determined by measuring the relative local variance(RLV),which indicates whether locally an image behaves smoothly or not.Near edges low order predictionfilters are activated which lead to large lifting detail coefficients along thin curves.At backgrounds of texture high order predictionfilters are activated which lead to negligible detail coefficients.Moments and subsequently moment invariants are computed with respect to these wavelet detail coefficients.With the computation of the detail coefficients a certain preprocessing is required to make the method robust for shifts over a non-integer number of gridpoints.Further we introduce the homogeneity condition which means that we demand a homogeneous change in the elements of a feature vector if the image seen as a density distribution is multiplied by a scalar.The report is organized as follows.In Sections2and3we discuss the lifting scheme and its adaptive version.Section4is devoted to the topic of affine invariances of the coefficients obtained from the lifting scheme.In Section5the method of moment invariants is recapitulated.The homogeneity condition is in-troduced which leads to a normalization.Furthermore,the mathematical consequences for the computation of moments of functions represented byfields of wavelet(detail)coefficients are investigated.Section6 discusses various aspects of thefinal retrieval algorithm,including possible metrics.Numerical results of the algorithm for a synthetic database are presented in Section7.Finally,some conclusions are drawn in Section8.2.T HE L IFTING S CHEMEThe lifting scheme as introduced by Sweldens in1997,see[18],is a method for constructing wavelet transforms that are not necessarily based on dilates and translates of one function.In fact the construction does not rely on the Fourier transform which makes it also suitable for functions on irregular grids.The transform also allows a fully in-place calculation,which means that no auxiliary memory is needed for the computations.The idea of lifting is based on splitting a given set of data into two subsets.In the one-dimensional case this can mean that starting with a signal the even and odd samples are collected into two new signals,i.e.,,where and,for all.The next step of the lifting scheme is to predict the value of given the sequence.This prediction uses a prediction operator acting on.The predicted value is subtracted from yielding a ‘detail’signal.An update of the odd samples is needed to avoid aliassing problems.This update is performed by adding to the sequence,with the update operator.The lifting procedure can also be seen as a2-bandfilter bank.This idea has been depicted in Figure1.The inverse lifting scheme can/.-,()*+/.-,()*+/.-,()*+/.-,()*+/.-,()*+Figure1:The lifting scheme:splitting,predicting,updating.immediately be found by undoing the prediction and update operators.In practice,this comes down in Figure1to simply changing each into a and vice versa.Compared to the traditional wavelet transform the sequence can be regarded as detail coefficients of the signal.The updated sequence can be regarded as the approximation of at a coarse ing again as input for the lifting scheme yields detail and approximation signals at lower resolution levels.We observe that every discrete wavelet transform can also be decomposed into a finite sequence of lifting steps[6].To understand the notion of vanishing moments in terms of the prediction and update operators,we com-pare the lifting scheme with a two-channelfilter bank with analysisfilters(lowpass)and(highpass) and synthesisfilters and.Such afilter bank has been depicted in Figure2.Traditionally we say that a389:;?>=<89:;?>=</.-,()*+89:;?>=<89:;?>=<Figure2:Classical2-band analysis/synthesisfilter bank.filter bank has primal and vanishing moments ifandwhere denotes the space of all polynomial sequences of order.Given thefilter operators and, the correspondingfilters and can be computed by(2.1)(2.2)where and denote thefilter sequences of the operators and respectively.In[12]Kovacevic and Sweldens showed that we can always use lifting schemes with primal vanishing moments and dual vanishing moments by taking for a Nevillefilter of order with a shift and for half the adjoint of a Nevillefilter of order and shift,see[17].Example2.1We take and.With these operators we getThefilter bank has only one vanishing moment.The lifting transform corresponds in this example to the Haar wavelet transform.Example2.2For more vanishing moments,i.e.,smoother approximation signals,we takeThese Nevillefilters give rise to a2-channelfilter bank with2primal and4dual vanishing moments. The lifting scheme can also be used for higher dimensional signals.For these signals the lifting scheme consists of channels,where denotes the absolute value of the determinant of the dilation matrix,that is used in the corresponding discrete wavelet transform.In each channel the signal is translated along one of the coset representatives from the unit cell of the corresponding lattice,see[12]. The signal in thefirst channel is then used for predicting the data in all other channels by using possible different prediction operators.Thereafter thefirst channel is updated using update operators on the other channels.Let us consider an image as a two-dimensional signal.An important example of the lifting scheme applied to such a signal is one that involves channels().We subdivide the lattice on which the signal has been defined into two sets on quincunx grids,see Figure3.This division is also called ”checkerboard”or”red-black”division.The pixels on the red spots()are used to predict the samples on the black spots(),while updating of the red spots is performed by using the detailed data on the black spots.An example of a lifting transform with second order prediction and updatefilters is given by4Figure3:A rectangular grid composed of two quincunx grids.order200000040000060008Table1:Quincunx Nevillefilter coefficientsThe algorithm using the quincunx lattice is also known as the red-black wavelet transform by Uytterhoeven and Bultheel,see[20].In general can be written as(2.3) with a subset of mod and,a set of coefficients in. In this case a general formula for reads(2.4)with depending on the number of required primal vanishing moments.For several elements in the coefficients attain the same values.Therefore we take these elements together in subsets of, i.e.,(2.5)Table1indicates the values of all,for different values of(2through8)when using quincunx Nevillefilters,see[12],which are thefilters we use in our approach.We observe that and so a44tapsfilter is used as prediction/update if the requiredfilter order is8.For an illustration of the Nevillefilter of order see Figure4.Here the numbers,correspond to the values of thefilter coefficients as given in and respectively at that position.The left-handfilter can be used to transform a signal defined on a quincunx grid into a signal defined on a rectangular grid,the right-hand filter is the degrees rotated version of the left-handfilter and can be used to transform a signal from a rectangular grid towards a quincunx grid.We observe that the quincunx lattice yields a non separable2D-wavelet transform,which is also sym-metric in both horizontal and vertical direction.Furthermore,we only need one prediction and one update operator for this2D-lifting scheme,which reduces the number of computations.The prediction and update operators for the quincunx lattice do also appear in schemes for other lattices, like the standard2D-separable lattice and the hexagonal lattice[12].The algorithm for the quincunx lattice can be extended in a rather straightforward way for these two other well-known lattices.5111122222222111122222222Figure 4:Neville filter of order :rectangular (left)and quincunx (right)Figure 5illustrates the possibility of the use of more than channels in the lifting scheme.Herechannels are employed,using a four-colour division of the 2D-lattice.It involves (interchange-able)prediction steps.Each of the subsets with colours ,and respectively,is predicted by application of a prediction filter on the subset with colour .Figure 5:Separable grid (four-colour division).3.A DAPTIVE L IFTINGWhen using the lifting scheme or a classical wavelet approach,the prediction/update filters or wavelet/scaling functions are chosen in a fixed fashion.Generally they can be chosen in such way that a signal is approximated with very high accuracy using only a limited number of coefficients.Discontinuities mostly give rise to large detail coefficients which is undesirable for applications like compression.For our purpose large detail coefficients near edges in an images are desirable,since they can be identified with the shape of objects we want to detect.However,they are undesirable if such large coefficients are related to the background of the image.This situation occurs if a small filter is used on a background of texture that contains irregularities locally.In this case a large smoothing filter gives rise to small coefficients for the background.These considerations lead to the idea of using different prediction filters for different parts of the signal.The signal itself should indicate (for example by means of local behavior information)whether a high or low order prediction filter should be used.Such an approach is commonly referred to as an adaptive approach.Many of these adaptive approaches have been described already thoroughly in the literature,e.g.[3,4,8,13,19].In this paper we follow the approach proposed by Baraniuk et al.in [2],called the space-adaptive approach.This approach follows the scheme as shown in Figure 6.After splitting all pixels of a given image into two complementary groups and (red/black),thepixels inare used to predict the values in .This is done by means of a prediction filter acting on ,i.e.,.In the adaptive lifting case this prediction filter depends on local information of the image pixels .Choices for may vary from high to low order filters,depending on the regularity of the image locally.For the update operator,we choose the update filter that corresponds to the prediction filter with lowest order from all possible to be chosen .The order of the update filter should be lower or equal to the order of the prediction filter as a condition to provide a perfect reconstruction filter bank.As with the classical wavelet filter bank approach,the order of the prediction filter equals the number of dual vanishing6/.-,()*+/.-,()*+Figure6:Generating coefficients via adaptive liftingmoments while the order of the updatefilter equals the number of primal vanishing moments,see[12].The above leads us to use a second order Nevillefilter for the update step and an th order Nevillefilter for the prediction step,where.In our application the reconstruction part of the lifting scheme is not needed.In[2],Baraniuk et al.choose to start the lifting scheme with an update operator followed by an adaptively chosen prediction operator.The reason for interchanging the prediction and update operator is that this solves stability and synchronization problems in lossy coding applications.We will not discuss this topic in further detail,but only mention that they took for thefilters of and the branch of the Cohen-Daubechies-Feauveau(CDF)filter family[5].The order of the predictionfilter was chosen to be,,or,depending on the local behavior of the signal.Thefilter orders of the CDFfilters in their paper correspond to thefilter orders of the Nevillefilters we are using in our approach.Relative local variance We propose a measure on which the decision operator in the2D adaptive lifting scheme can be based on,namely the relative local variance of an image.This relative local variance(RLV) of an image is given byrlv var(3.1) with(3.2) For the window size we take,since with this choice all that are used for the prediction of contribute to the RLV for,even for the8th order Nevillefilter.When the RLV is used at higher resolution levels wefirst have to down sample the image appropriately.Thefirst time the predictionfilter is applied(to the upper left pixel)we use the8th order Nevillefil-ter on the quincunx lattice as given in Table1.For all other subsequent pixels to be predicted,we first compute rlv.Then quantizing the values of the RLV yields a decisionmap indicating which predictionfilter should be used at which positions.Values above the highest quantizing level induce a 2nd order Nevillefilter,while values below the lowest quantizing levels induce an8th order Nevillefil-ter.For the quantizing levels we take multiples of the mean of the RLV.Test results have shown that rlv rlv rlv are quantizing levels that yield a good performance in our application.In Figure7we have depicted an image(left)and its decision map based on the RLV(right).4.A FFINE I NVARIANT L IFTINGAlthough both traditional wavelet analysis and the lifting scheme yield detail and approximation coeffi-cients that are localised in scale and space,they are both not translation invariant.This means that if a signal or image is translated along the grid,its lifting coefficients may not be just be given by a translation of the original coefficients.Moreover,in general the coefficients will attain values in the same range of the original values(after translation),but they will be totally different.7a) original image b) decision map (RLV)Figure7:An object on a wooden background and its rel.local variance(decision map):white=8th order, black=2nd order.For studying lifting coefficients of images a desirable property would also be invariance under reflections and rotations.However,for these two transformations we have to assumefirst that the values of the image on the grid points is not affected a rotation or reflection.In practice,this means that we only consider reflections in the horizontal,the vertical and the diagonal axis and rotations over multiples of.4.1Redundant LiftingFor the classical wavelet transform a solution for translation invariance is given by the redundant wavelet transform[15],which is a non-decimated wavelet(at all scales)transform.This means that one gets rid of the decimation step.As a consequence the data in all subbands have the same size as the size as the input data of the transform.Furthermore,at each scaling level,we have to use zero padding to thefilters in order to keep the multiresolution analysis consistent.Not only more memory is used by the redundant transform,also the computing complexity of the fast transform increases.For the non-decimated transform computing complexity is instead of for the fast wavelet transform.Whether the described redundant transform is also invariant under reflections and rotations depends strongly on thefilters(wavelets)themselves.Symmetry of thefilters is necessary to guarantee certain rotation and reflection invariances.This is a condition that is not satisfied by many well-known wavelet filters.The redundant wavelet transform can also be translated into a redundant lifting scheme.In one dimension this works out as follows.Instead of partitioning a signal into and we copy to both and.The next step of the lifting scheme is to predict by(4.1) The predictionfilter is the samefilter as used for the non-redundant case,however now it depends on the resolution level,since at each level zero padding is applied to.This holds also for the updatefilters .So,the update step reads(4.2)For higher dimensional signals we copy the data in all channels of the usedfilter bank. Next the-channel lifting scheme is applied on the data,using zero padding for thefilters at each resolu-8................ ........Figure8:Tree structure of the-channel lifting scheme.tion level.Remark,that for each lifting step in the redundant-channel lifting scheme we have to store at each scaling level times as much data as in the non-redundant scheme,see Figure8.We observe that in our approach Nevillefilters on a quincunx lattice are used.Due to their symmetry properties,see Table1,the redundant scheme does not only guarantee translation invariance,but also invariance under rotations over multiples of and reflections in the horizontal,vertical and diagonal axis is assured.Invariance under other rotations and reflections can not be guaranteed by any prediction and updatefilter pair,since the quincunx lattice is not invariant under these transformations.4.2An Attempt to Avoid Redundancy:Fixed Point LiftingAs we have seen the redundant scheme provides a way offinding detail and approximation coefficients that are invariant under translations,reflections and rotations,under which the lattice is also invariant.Due to its redundancy this scheme is stable in the sense that it treats all samples of a given signal in the same way.However redundancy also means additional computational costs and perhaps even worse additional memory to store the coefficients.Therefore we started searching for alternative schemes that are also invariant under the described class of affine transformation.Although we did not yet manage to come up with an efficient stable scheme,we would like to stretch the principal idea behind the building blocks of such approach.In the sequel we will only use the redundant lifting scheme as described in the preceding section.Before we start looking for possible alternative schemes we examine why the lifting scheme is not translation invariant.Assume we have a signal that is analysed with an-band lifting scheme. Then after one lifting step we have approximation data and detail data.Whether one sample,is determined to become either a sample of or a sample ofdepends only on its position on the lattice and the way we partition the lattice into groups.Of course, this partitioning is rather arbitrary.The more channels we use the higher the probability is that for afixed partitioning one sample that was determined to be used for predicting other samples,will become a sample of after translating.Following Figure8it is clear that any sample,can end up after lifting steps in ways,either in approximation data at level or in detail data at some level.The idea of the alternative scheme we propose here is to partition a signal not upon its position on the lattice but upon its structure.This means that for each individual signal we indicate afixed point for which we demand that it will end up in the approximation data after lifting steps.If this point can be chosen independent of its coordinates on the lattice,the lifting scheme based on this partitioning will then translation invariant.For higher dimensional signals we can also achieve invariance under the other discussed affine transformations,however then we have tofix more points,depending on the number ofchannels.In our approach the quincunx lattice is used and thereforefixing one approximation sample on scales will immediatelyfix the partitioning of all other samples on the quincunx lattice at scale. As a result thefixed point lifting scheme is invariant under translations,rotations and reflections that leave the quincunx lattice invariant.In the sequel of this chapter we will only discuss the lifting scheme for for the quincunx lattice.Although the proposedfixed point lifting scheme may seem to be a powerful tool for affine invariant lifting,it will be hard to deal with in practice.The problem we will have to face is how to choose afixed point in every image.In other words we have tofind a suitable decision operator that adds to every a unique,itsfixed point,i.e.,If we demand to depend only on and not on the lattice(coordinate free)it will be hard tofind such that is well defined.This independence of the coordinates is necessary for rotation invariances.However, this is not the only difficulty we have to face.Stability of the scheme is an other problem.If for some reason afixed point has been wrongly indicated,for example due to truncation errors,the whole scheme might collapse down.Although we cannot easily solve the problem of determining incorrectfixed points we can increase the stability of the scheme by not imposing that at each scale should be an index number of the coarse scale data after zero padding.Instead of this procedure we rather determine afixed point for both the original signal()and for the coarse scale data(at each scale.Then we impose that should be used for prediction in the th lifting step,for and with.Furthermore,stability may be increased by using decision operators that generate a set offixed points.However,since no stable method (uniform decision operator)is available yet,we will use the redundant lifting scheme in our approach and do not work out the idea offixed point lifting here at this moment.5.M OMENT I NVARIANTSAt the outset of this section we give a brief introduction into the theory of statistical invariants for imag-ing purposes,based on centralized moments.Traditionally,these features have been widely used in pat-tern recognition applications to recognize the geometrical shapes of different objects[11].Here,we will compute invariants with respect to the detail coefficients as produced by the wavelet lifting schemes of Sections2–4.We use invariants based on moments of the coefficients up to third order.We show how to construct a feature vector from the obtained wavelet coefficients at several scales It is followed by proposals for normalization of the moments to keep them in comparable range.5.1Introduction and recapitulationWe regard an image as a density distribution function,the Schwartz class.In order to obtain translation invariant statistics of such we use central moments of for our features.The order central moment of is given by(5.1) with the center of massand(5.2)Computing the centers of mass and of yieldsand bining this with(5.1)showsi.e.,the central moments are translation invariant.We also require that the features should be invariant under orthogonal transformations(rotations).For deriving these features we follow[11]using a method with homogeneous polynomials of order.These are given by(5.3) Now assume that the variables are obtained from other variables under some linear transformation,i.e.,then is an algebraic invariant of weight if(5.4) with the new coefficients obtained after transforming by.For orthogonal transformations we have and therefore is invariant under rotations ifParticularly we have from[11],that if is an algebraic invariant,then also the moments of order have the same invariant,i.e.,(5.5) From this equation2functions of second order can be derived that are invariant under rotations,see[11]. For we have the invariantsandIt was also shown that these two functions are also invariant under reflections,which can be a useful property for identifying reflected images.Since the way of deriving these invariants may seem a bit technical and artificial,we illustrate with straightforward calculus that and are indeed invariant under rotations.The invariance under reflections is left to the reader,since showing this follows the same calculations.We consider the rotated distribution functionand the corresponding invariants and,which are and but now based on moments calculated from.So what we have to show is that and.It follows from(5.1)and(5.2)that if and only ifwith and.Obviously this holds true,considering the trigonometric rule .To do the same for we also have to introduce and.Because we have to take products of integrals that define,we cannot use and in both integrals.As for we can now derive from(5.1)and(5.2)that if and only ifWe simplify the right-hand side term by term.Thefirst term,that is related to becomes The second term(related to)becomesAdding these two terms gives uswhich demonstrates that indeed also is invariant under rotations.Similar calculus shows that invariance under reflections also holds.From Equation(5.5)four functions of third order and one function of both second and third order can be derived that are invariant under both rotations and reflecting,namelyandwithThe last polynomial that is invariant under both rotations and reflections consists of both second and third order moments and is given bywith and as above.To these six invariants we can add a seventh one,which is only invariant under rotations and changes sign under reflections.It is given bySince we want to include reflections as well in our set of invariant transformations we will use instead of in our approach.From now on,we will identify with.We observe that all possible linear combinations of these invariants are invariant under proper orthogonal transformations and translations.Therefore we can call these seven invariants also invariant generators.。

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a r X i v :0808.1526v 1 [h e p -p h ] 11 A u g 2008Comment on ”Gauge Invariance and k T -Factorization of Exclusive Processes”Hsiang-nan Li ∗Institute of Physics,Academia Sinica,Taipei,Taiwan 115,Republic of China,Department of Physics,National Cheng-Kung University,Tainan,Taiwan 701,Republic of China andDepartment of Physics,National Tsing-Hua University,Hsinchu,Taiwan 300,Republic of ChinaWe point out mistakes made in the one-loop calculation of some diagrams for the process πγ∗→γin the preprint arXiv:0807.0296,and present correct results.It is explained that the gauge-dependentlight-cone singularity found in arXiv:0807.0296does not exist.It is then shown that a hard kernelin k T factorization of exclusive processes is gauge invariant and free of the light-cone singularity.PACS numbers:In a recent preprint arXiv:0807.0296[1],the authors studied the pion transition form factor in the k T factorization theorem at one-loop level,calculating the full QCD diagrams for the form factor (see their Fig.4)and the diagrams for the k T -dependent pion wave function (see their Figs.2and 3)in the covariant gauge.They focused on a special piece of contribution,which depends on the gauge parameter,and contains a light-cone singularity.It was found that the full QCD diagrams do not generate this contribution,but those for the pion wave function do,if the involved partons are taken to be off-shell.Therefore,the hard kernel,defined as the difference of the above two sets of diagrams,is gauge dependent,and contains the light-cone singularity.They were then led to the conclusion that the k T factorization theorem for exclusive processes violates gauge invariance,and that the perturbative QCD (PQCD)approach [2,3,4,5]to exclusive B meson decays,based on the k T factorization theorem,is also gauge dependent.This conclusion contradicts to that drawn in our previous work [6].In this comment we shall point out mistakes made in their calculation,and demonstrate that the gauge-dependent light-cone singularity does not exist.The all-order proof for the gauge invariance and infrared finiteness of a hard kernel in k T factorization [6]is indeed correct.Consider the process π(P )γ∗→γ(p )with P (p )being the pion (outgoing photon)momentum along the plus (minus)direction.Define the momenta of the valence quark and anti-quark in the pion as (see Fig.1in [1])k µ1=(k +1,0, k 1⊥),k µ2=(k +2,0,− k ⊥),(1)respectively,with k +1=x 0P +and k +2=(1−x 0)P +,x 0being the momentum fraction.The leading-order (LO)hard kernel is given,in terms of the above momenta,by H (0)=1x 0Q 2+k 21⊥,(2)with the momentum transfer Q 2=2P +p −.At next-to-leading order (NLO),a loop momentum q carried by the additional gluon may flow through the hard kernel,for example,in Fig.2of [1].In this case the factorized k T -dependent wave function is convoluted with H (0)=1(2π)41q 2+iεN µν(q )=−iq 2+iε .(5)This integral,not involving a scale,is equal to zero.An alternative understanding of this result is that the ultraviolet (UV)and infrared(IR)divergences cancel exactly.To isolate the IR pole,the usual method is to introduce a gluon massλ2L:I=iα16g2s d4q(q2−λ2L+iε)2,(6) and then apply the Feynman parametrization.It is easy to obtainI=α4αsµ2+UV pole,(7)where lnλ2L denotes the light-cone singularity[1],andµis the renormalization scale.However,if employing the contour integration,Eq.(6)vanishes:I=iα16g2s d4q(2q+q−−q2⊥−λ2L+iε)2=0.(8)The poles in the above integrand always locate in the same half plane,either upper or lower,no matter one integrates over q−or q+first.Therefore,one can enclose the contour in the other half plane without containing the poles. Obviously,Eq.(8)contradicts to Eq.(7).How to understand this puzzle is the key to clarify the conflict between [1]and[6].The answer is that adding the gluon massλ2L works to separate the UV and IR poles in the Feynman parametrization,but does not in the contour integration.A possible way to separate the UV and IR poles in the latter is to further introduce a small scale a:I=lima→0iα16g2s d4q(2q+q−−q2⊥−λ2L+iε)[2(q+−a)q−−q2⊥−λ2L+iε],(9)if one integrates over q−first.If integrating over q+first,the small scale a should be added to form q−−a.Then there exists a pinched pole in the q−complex plane for0<q+<a.A trivial evaluation of Eq.(9)gives an expression identical to Eq.(7).The above example illustrates that a naive application of the contour integration to an integral containing the denominator(q2)2may lead to a false result:an IR pole would be hidden in Eq.(8),if employing the contour integration naively.This is exactly the reason the authors of[1]drew a wrong conclusion from Fig.2.The correct application of the contour integration demands the further introduction of the small scale a indicated in Eq.(9). Below we shall recalculate Fig.2in[1]following this prescription,and demonstrate that Figs.2a,2b,and2c are in fact free of the gauge-dependent light-cone singularityαlnλ2L.Since the authors of[1]have evaluated Fig.3(diagrams for the pion wave function without the loop momentumflowing through the hard kernel)and Fig.4(diagrams for the form factor)using the Feynman parametrization,these results are valid.We have confirmed them by the above prescription for the contour integration.We start from Fig.2b,whose gauge-dependent part is written as[1]φα|2b=i16αg2s d4q[(k1−q)2+iε](q2+iε)2δ(k+−(k1−q)+)δ2( k⊥−( k1− q)⊥).(10) The wave functionφα|2b is convoluted with the LO hard kernel:φα|2b⊗H(0)= 10dx d2k⊥1q2−λ2L+iε gµν−αqµqνP+πlnλ2LNow we further introduce the small scale a into the gluon propagator,so that Eq.(10)contains1P+π2 a0dq+q2⊥−2(q+/k+1) k1⊥· q⊥+(q+/k+1)k21⊥+[1−(q+/k+1)]λ2L ×1q2⊥+[1−(q+/a)α]λ2L.(15)The ratio in the last line can be approximated by unity,since the difference is proportional to the small massλ2L.A straightforward calculation givesφ′α|2b⊗H(0)=−4ααsx0Q2+k21⊥+finite terms,(16)which cancels the IR pole in Eq.(13),implying that Fig.2b is free of the gauge-dependent light-cone singularity.The same conclusion applies to Fig.2c of[1].It is easy to understand why the authors in[1]got a fake light-cone singularity from Fig.2b.When using the contour integration naively,an IR pole has been hidden,just like that an IR pole is hidden in Eq.(8).One has to apply the prescription in Eq.(9)in order to isolate this hidden IR pole,which will cancel the fake singularity.Our observation is natural from the viewpoint of the Ward identity.Contracting the loop momentum q to the vertex on the internal quark line[see the numerator of the gauge-dependent term in Eq.(12)],p−k1(p−k1+q)2=p−k1(p−k1+q)2,(17)thefirst(second)term leads to the LO hard kernel associated with Fig.3c(Fig.2b).The full QCD diagram Fig.4c is then factorized into convolutions of the LO hard kernel with Figs.2b and3c.If Figs.4c and3c do not contain the light-cone singularity as found in[1],Fig.2b should not either.Another support to our result comes from the following simple observation.In the light-cone region the q+and q⊥dependence in the LO hard kernel is negligible. Then Figs.2b and3c involve exactly the same loop integral,namely,the same behavior in the light-cone region.If Fig.3c does not produce the light-cone singularity as found in[1],Fig.2b should not either.We then turn to Fig.2a,which appears as a consequence of factorizing the box diagram Fig.4a for the form factor. Again,Fig.2a should not produce the gauge-dependent light-cone singularity,because Fig.4a does not.The explicit expression for the leading contribution from Fig.2a in the light-cone region is given byφα|2a=−i64αg2s d4q((k1−q)2+iε)((k2+q)2+iε)(q2−λ2L+iε)(q2−(1−α)λ2L+iε)×δ(k+−(k1−q)+)δ2( k⊥−( k1− q)⊥),(18) where the numerator(q−)2arises from qµqνin the gluon propagator forµ=ν=−.Integrating over q−first,we get two poles,q−=| k1⊥− q⊥|2/[2(q+−k+1)]+iεfor0<q+<k+1and q−=| k1⊥− q⊥|2/[2(q++k+2)]−iεfor −k+2<q+<0.Adopting the approximation in the light-cone region,it is easy to confirm that the above two poles give the result in[1],φα|2a⊗H(0)=−4ααsx0Q2+k21⊥+finite terms,(19)which is also a fake singularity.Introducing the small scale a,we have an additional pole q−=[q2⊥+(1−α)λ2L]/[2(q+−a)]+iε,which leads toφ′α|2a⊗H(0)=−lima→04ααsa d2q⊥1(k+1−q+)Q2/P++| k1⊥− q⊥|2×q2⊥+(1−α)λ2Lq2⊥+[1−(q+/a)α]λ2L.(20)The ratios in the last line can be approximated by unity subject to corrections suppressed by a orλ2L.It is trivial to work out the integration over q⊥and q+,givingφ′α|2a⊗H(0)=4ααsx0Q2+k21⊥+finite terms.(21)The sum of Eqs.(19)and(21),i.e.,Fig.2a is free of the gauge-dependent light-cone singularity,contrary to the observation in[1].In summary,all the diagrams in Figs.2-4,except those with the gluons attaching only to the Wilson lines(Figs.2d,3b,and3e),do not generate the gauge-dependent light-cone singularity.We then comment on the diagrams Figs.2d,3b,and3e.These diagrams do not appear in the factorization of collinear gluons[7,8,9]from the pion transition form factor.It has been shown that their sum is IRfinite[1].This must be the case,since all the IR divergences in Fig.4,which arise from the collinear region with the scaling law (q+,q−,q⊥)∼(1,δ2,δ),have been absorbed into the other diagrams in Figs.2and3[6].However,in view of a gauge invariant definition for the pion wave function,Figs.2d,3b,and3e should be included.A resolution is to invoke a soft subtraction factor in the denominator[1,7]:φ(x0;x,k⊥)= dy−(2π)2e−ixP+1y−+i k⊥· y⊥ 0|¯q(y)W y(n)†I n;y,0W0(n)γ+γ5q(0)|q(k1)¯q(k2)4πu·n(u·n)2−u2n2ln ǫ+ln4πµ24π 1λ2L eγE.(25)It is easy tofind that the above two expressions cancel exactly for u2n2<0and u·n/above conditions for u and n are satisfied.Eventually,we just need to calculate the seven effective diagrams in Fig.2 of[6]for the pion wave function in the Feynman gauge at one-loop level.After clarifying the conflict,the all-order proof of the leading-power k T factorization theorem for the pion transition form factor in Sec.III of[6]follows straightforwardly.Below we mention the points of the proof briefly.Because the light-cone singularity[1]does not exist,the substitution for the metric tensor of the gluon propagator in the covariant gauge,Eq.(47)of[6],works for extracting all IR(collinear)divergences.We then employ the derivative in Eq.(50) of[6]to collect the gauge-dependent terms arising from the off-shell partons.The derivative of the soft subtraction factor vanishes,since it is gauge invariant.The derivative of the pion wave function is then related to the derivative of the numerator in Eq.(22),which,after applying the Ward identity,gives Eq.(53)in[6].Combining Eqs.(52)and (53)in[6],the k T factorization theorem for the pion transition form factor is proved by induction.In conclusion,the only necessary revision for[6]is to replace the definition for the k T-dependent pion wave function by Eq.(22)with an appropriate vector u.Except this modification,all the results in[6]are valid.The gauge-dependent light-cone singularity found in[1]does not exist actually,which is attributed to a careless application of the contour integration to the extraction of IR poles.The appropriate prescription for extracting IR poles is to further introduce the small scale a as indicated in Eq.(9).We have confirmed that the all-order proof of the k T factorization theorem for the pion transition form factor holds:the gauge dependence,arising from the off-shell external partons, cancels between the full QCD diagrams for the form factor and the effective diagrams for the pion wave function. Therefore,k T factorization gives a gauge invariant and IRfinite hard kernel,and provides a solid basis for the PQCD approach to exclusive B meson decays.We thank J.P.Ma and Q.Wang for useful discussions.The work was supported in part by the National Science Council of R.O.C.under Grant No.NSC-95-2112-M-050-MY3,by the National Center for Theoretical Sciences of R.O.C.,and by Kavli Institute for Theoretical Physics,China.[1]F.Feng,J.P.Ma,and Q.Wang,arXiv:0807.0296[hep-ph].[2]H-n.Li and G.Sterman,Nucl.Phys.B381,129(1992).[3]H-n.Li and H.L.Yu,Phys.Rev.Lett.74,4388(1995);Phys.Lett.B353,301(1995);Phys.Rev.D53,2480(1996).[4]Y.Y.Keum,H-n.Li,and A.I.Sanda,Phys.Lett.B504,6(2001);Phys.Rev.D63,054008(2001);Y.Y.Keum and H-n.Li,Phys.Rev.D63,074006(2001).[5]C.D.L¨u,ai,and M.Z.Yang,Phys.Rev.D63,074009(2001).[6]S.Nandi and H-n.Li,Phys.Rev.D76,034008(2007).[7]J.C.Collins,Adv.Ser.Direct.High Energy Phys.5,573(1989).[8]H-n.Li,Phys.Rev.D64,014019(2001);M.Nagashima and H-n.Li,Eur.Phys.J.C40,395(2005).[9]M.Nagashima and H-n.Li,Phys.Rev.D67,034001(2003).[10]X.Ji,and F.Yuan,Phys.Lett.B543,66(2002);A.V.Belitsky,X.Ji,and F.Yuan,Nucl.Phys.B656,165(2003).[11]H-n.Li and H.S.Liao,Phys.Rev.D70,074030(2004).。

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