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Noncommutative Supersymmetric/Integrable Models and String Theory PDF

185 Pages·2005·1.491 MB·English
by  TamassiaL
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Preview Noncommutative Supersymmetric/Integrable Models and String Theory

UNIVERSITY OF PAVIA Department of Nuclear and Theoretical Physics 5 0 Noncommutative 0 2 Supersymmetric/Integrable Models n u J and 7 2 String Theory 3 v 4 6 0 6 0 5 0 / Supervisor: Prof. Annalisa Marzuoli h External Referee: Prof. Ulf Lindstr¨om t - p e h : v i X Doctoral Thesis of r a Laura Tamassia Dottorato di Ricerca in Fisica XVII Ciclo Contents Introduction v 1 An introduction to non(anti)commutative geometry and superstring theory 1 1.1 Abriefintroductiontononcommutativeandnon(anti)commutative field theory . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1 1.1.1 The Moyal product . . . . . . . . . . . . . . . . . . . . . . 1 1.1.2 The natural Moyal deformation of a field theory . . . . . 8 1.1.3 Other possible deformations: The free scalar field theory example . . . . . . . . . . . . . . . . . . . . . . . . . . . . 14 1.1.4 The Kontsevich product . . . . . . . . . . . . . . . . . . . 16 1.1.5 Deforming superspace . . . . . . . . . . . . . . . . . . . . 18 1.1.6 Non(anti)commutative superspace . . . . . . . . . . . . . 21 1.1.7 N = 1 supersymmetry . . . . . . . . . . . . . . . . . . . . 31 2 1.2 Non(anti)commutative field theory from the (super)string . . . . 35 1.2.1 Noncommutative Yang-Mills theory from the open string 35 1.2.2 Generalization to the superstring in RNS and GS formalisms . . . . . . . . . . . . . . . . . . . . . . . . . . 43 1.2.3 Noncommutative selfdual Yang-Mills from the =2 N string . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 46 1.2.4 Non(anti)commutative field theories from the covariant superstring . . . . . . . . . . . . . . . . . . . . . . . . . . 48 1.3 Generalization to non-constant backgrounds . . . . . . . . . . . . 54 2 Noncommutative deformation of integrable field theories 57 2.1 Abriefintroductiontoselectedtopicsconcerningtwo-dimensional classical integrable systems . . . . . . . . . . . . . . . . . . . . . 57 2.1.1 Infinite conserved currents and the bicomplex approach . 57 2.1.2 Reductions from selfdual Yang-Mills . . . . . . . . . . . . 60 2.1.3 Properties of the S-matrix . . . . . . . . . . . . . . . . . . 62 2.1.4 Solitons . . . . . . . . . . . . . . . . . . . . . . . . . . . . 63 2.2 Deforming an integrable field theory: The sine-Gordon model (a first attempt) . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 64 2.2.1 Noncommutative solitons . . . . . . . . . . . . . . . . . . 64 i 2.2.2 Noncommutative deformation of integrable field theories . 67 2.2.3 The natural noncommutative generalization of the sine-Gordon model . . . . . . . . . . . . . . . . . . . . . . 68 2.2.4 A noncommutative version of the sine-Gordon equation with an infinite number of conserved currents . . . . . . . 69 2.2.5 Solitons . . . . . . . . . . . . . . . . . . . . . . . . . . . . 71 2.2.6 Reduction from noncommutative selfdual Yang-Mills . . . 71 2.2.7 The action . . . . . . . . . . . . . . . . . . . . . . . . . . 73 2.2.8 The relation to the noncommutative Thirring model . . . 74 2.2.9 (Bad) properties of the S-matrix . . . . . . . . . . . . . . 75 2.2.10 Conclusions . . . . . . . . . . . . . . . . . . . . . . . . . . 78 2.3 The noncommutative integrable sine-Gordon model . . . . . . . . 80 2.3.1 Introduction . . . . . . . . . . . . . . . . . . . . . . . . . 80 2.3.2 A noncommutative integrable sigma model in 2+1 dimensions . . . . . . . . . . . . . . . . . . . . . . . . . . 81 2.3.3 Reduction to noncommutative sine-Gordon . . . . . . . . 84 2.3.4 Relation with the previous noncommutative generalization of the sine-Gordon model . . . . . . . . . . 88 2.3.5 Solitons . . . . . . . . . . . . . . . . . . . . . . . . . . . . 90 2.3.6 (Nice) properties of the S-matrix . . . . . . . . . . . . . . 96 2.3.7 Conclusions . . . . . . . . . . . . . . . . . . . . . . . . . . 104 3 Covariant superstring vertices and a possible nonconstant superspace deformation 105 3.1 An introduction to the pure spinor superstring . . . . . . . . . . 105 3.1.1 Motivation: Problems with RNS and GS formalisms . . . 105 3.1.2 Pure spinor superstring basics. . . . . . . . . . . . . . . . 107 3.1.3 Type II superstring vertex operators . . . . . . . . . . . . 112 3.1.4 Amplitudes . . . . . . . . . . . . . . . . . . . . . . . . . . 115 3.1.5 What we can (cannot) do with this formalism, up to now 117 3.2 An iterative procedure to compute the vertex operators . . . . . 120 3.2.1 Warm up: The open superstring case. . . . . . . . . . . . 120 3.2.2 Linearized IIA/IIB supergravity equations . . . . . . . . . 122 3.2.3 Gauge transformations and gauge fixing . . . . . . . . . . 125 3.2.4 Recursive equations and explicit solution (up to order θ2θˆ2) . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 128 3.2.5 Gauge fixing for massive states . . . . . . . . . . . . . . . 131 3.3 An example: Linearly x-dependent Ramond-Ramond field strength and possible Lie-algebraic superspace deformations . . . 135 3.3.1 Motivation: Nonconstant superspace deformations . . . . 135 3.3.2 The ansatz for the RR field strength . . . . . . . . . . . . 135 3.3.3 The vertex for linearly x-dependent RR field strength . . 137 3.4 Other applications . . . . . . . . . . . . . . . . . . . . . . . . . . 138 3.4.1 Vertex operators with R-R gauge potentials . . . . . . . . 138 3.4.2 Antifields and the kinetic terms for closed superstring field theory . . . . . . . . . . . . . . . . . . . . . . . . . . 139 ii 4 Conclusions and outlook 141 A Conventions 149 A.1 Superspace conventions in d=4 . . . . . . . . . . . . . . . . . . 149 A.2 Superspace conventions in d=10 . . . . . . . . . . . . . . . . . . 152 Acknowledgements 155 iii Introduction Quantum field theory, i.e. quantum mechanics with the basic observables livingatspacetimepoints,istheprincipleunderlyingourcurrentunderstanding of natural phenomena. The incredibly successful Standard Model explains all the forces of nature, except gravity,in terms of local symmetry principles. Attheenergieswearecurrentlyabletotest,gravityiswelldescribedbygen- eralrelativity. However,itisexpectedthatatenergiesoftheorderofthePlanck mass M 1019 GeV, a quantum description of gravity will be necessary. The P ∼ union of gravity with quantum field theory leads to a nonrenormalizable the- ory. History of physics suggests that this should be interpreted as a sign that new physics willappearat higherenergies,comparingfor instance to the Fermi theory case. Anaturalwaytomodifyquantummechanicstodescribea“quantumspace- time”istogeneralizeHeisenbergcommutationrelationstoletthe spacecoordi- natesbenoncommuting. Inafieldtheorysetting,inprincipleonecouldinclude time in noncommutativity and consider a quantum spacetime where [Xµ,Xν]=iθµν(X) This can be realized in a functional formulation by deforming the algebra of functions on spacetime, replacing the ordinary, commutative product with a noncommutative one that, when applied to coordinates themselves, gives [xµ,xν] = xµ xν xν xµ = iθµν. The simplest case, with a constant θµν, is r∗elated to∗spac−etime∗translation invariance. The corresponding (Moyal) product can be uniquely identified by requiring that the deformed algebra of functions remains associative. When a field theory is deformed by replacingordinaryproducts with Moyal products in the action, vertices in the Feynman rules are multiplied by a phase factor with a dependence on the momenta, that generically acts as a regulator. Forthisreason,spacetimenoncommutativitywasfirstintroducedwiththehope that it might reduce the degree of divergence of a given theory [1]. However, since the contributions from a certain diagram also include the case where the phasefactordoesnotdependonloopmomenta,butonlyonexternalmomenta, this does not work [2]. Atthemoment,weonlyknowonewaytoconsistentlycutoffthedivergences appearinginaquantumfieldtheoryofgravity. Thisisstringtheory[3,4],where pointlike interactions are replaced by splitting and joining of one-dimensional objects, so that the interaction itself does not happen at a certain point in spacetime but is described by a smooth two-dimensional surface. String theory provides a consistentquantum theory of gravity. The number of spacetime dimensions is fixed to ten, the theory is consistent only in the presence of supersymmetry, relating bosonic and fermionic degrees of freedom, andleadstogaugegroupsthatincludetheStandardModelone. Stringtheories are unique in the sense that there are no free parameters and no freedom in choosinggauge groups. There is more than one possible string theory (actually v five), but they happen to be all related to each other by dualities. Therefore, a unique underlying theory is expected to exist, from which the various string theories can be obtained as limits in a certain space of parameters. It is striking that the somehow natural proposal for a quantum spacetime where Heseinberg commutation relations are generalized to include a nontriv- ial coordinate algebra can be obtained from string theory. The first works in this directionshowedthat noncommutative toriare solutions to the problem of compactifying M(atrix) theory [5]. Noncommutative field theories were shown toemergeaslowenergylimitsofopenstringdynamicsinthe presenceofacon- stant Neveu-Schwarz Neveu-Schwarz (NS-NS) background and D-branes (i.e. p-dimensional manifolds where open string ends are attached) [6, 7]. Since the backgroundselectspreferreddirectionsinspacetime,the resultingeffectivethe- orybreaksLorentzinvariance[8]. Therefore,noncommutativefieldtheorymust not be thoughtofas a fundamentaltheory,but as aneffective descriptionto be used when certain backgrounds are present. The discovery that noncommutative geometry is somehow embedded in stringtheoryinducedagrowinginterestinthefield. Variousaspectsofnoncom- mutative field theory, such as renormalization properties [9, 10], solitons (see forinstancethelectures[11,12,13])andinstantons[14]havebeeninvestigated. Furthermore,itwasshownthatwhentime is involvedinnoncommutativitythe resulting field theories display awkward features, such as acausality [15] and nonunitarity [16], that spoil the consistency of the theory. However,it was also shown that these ill-defined noncommutative field theories cannot be obtained as a low energy limit of string theory [16]. String correctionsconspire to cancel out the inconsistencies [15, 17]. Applications that are not directly related to string theory have been con- sidered, for instance a model to describe the quantum Hall effect was proposed in [18], based on noncommutative Chern-Simons theory. Moreover, a mech- anism to drive inflation without an inflaton field was studied in [19], based on noncommutativity of spacetime. Particle physics phenomenology based on a noncommutative version of the Standard Model has been studied [20] and possible experimental tests have been proposed [21]. In these applications also noncommutativedeformationsthathavenotyetbeenshowntoarisefromstring theory havebeen considered[22]. Anaturalquestion wouldbe atwhich energy one expects to observe effects of noncommutativity. If one considers this as an effective description in the presence of a background, the energy is related to the background scale, and therefore cannot be determined a priori. As I said, string theoryis consistentonly in the presence ofsupersymmetry. Supersymmetric theories are better described in superspace formalism [23, 24, 25], where spacetime is enlarged by adding fermionic coordinates. Superspace geometry is not flat, torsion is present. Since noncommutative geometry arises inastringtheorycontextandstringsrequiresupersymmetry,itiscompellingto studythepossibledeformationsofsupersymmetrictheories. Thenaturalwayto dothatistoinvestigatethepossibleconsistentdeformationsofsuperspace. This I did in my first paper [26], in collaborationwith D. Klemm and S. Penati. We foundthatconsistentdeformationsofsuperspacearepossibleinbothMinkowski vi andEuclideansignaturesinfourdimensions. IntheEuclideancasemoregeneral structures are allowed because of the different spinor reality conditions. After the appearanceof my paper [26], deformed superspaces were found to emerge in superstring theory [27, 28, 29]. However, to see this effect, a par- ticular formulation of superstring theory has to be considered, where all the symmetries of the theory are manifest. This superPoincar´e covariant formu- lation, found in 2000 by Berkovits [30], is still “work in progress”. However, it has already proven to be superior in handling certain string backgrounds (Ramond-Ramond), that lead to the superspace deformations I found, and to provegeneraltheorems regardingstring amplitudes, like for instance atheorem stating the “finiteness” of perturbative string theory [31]. I’ve been studying this formalism for the superstring and contributed, in [32], written together with P.A. Grassi, by giving an iterative procedure to simplify the computation of superstring vertex operators,that are the main ingredient for the evaluation of superstring amplitudes. Some applications of our analysis are also discussed inthe paper. Forinstance, the verticesassociatedto a R-R fieldstength witha linear dependence on the bosonic coordinates have been computed. These play aroleinthestudyofsuperspacedeformationwithaLie-algebraicstructuresuch that bosonic coordinates of superspace are obtained as the anticommutator of the fermionic ones. This can be interpreted by saying that spacetime has a fermionic substructure [33]. Going back to noncommutative field theory, a puzzling aspect is that the noncommutative generalization of a given ordinary theory is not unique. A selection principle can be based on trying to preserve the nice properties of a modelinits noncommutativedeformation. Thesymmetrystructureofatheory is its most important characteristic and actually defines the theory when the fieldcontentis given. Therefore,preservingthe symmetry structureofa theory shouldbethefirstcriteriumtoconsiderwhenconstructingitsdeformation. This isalsotheguidingprincipleweusedinstudyingdeformationsofsupersymmetric theories in [26]. A very special case is given by systems endowed with an infinite number of local conserved charges. These systems, known as integrable by analogy to the case with a finite number of degrees of freedom, display very special features. The presence of such a strong symmetry structure underlying the system puts constraints on the dynamics, for instance causing the S-matrix to be factorized and preventing particle production processes to occur. Moreover, integrable systems usually display localized classical solutions, known as solitons, that do not change shape or velocity after collisions. Therefore, when constructing the noncommutative generalization of an integrable system, one would like to pre- serveboththesymmetrystructureunderlyingthesystemandtheconsequences that this has in ordinary geometry. The two-dimensional case is particularly problematic in noncommutative field theory, because time must be necessar- ily involved in noncommutativity and thus it is expected that acausality and nonunitarity will spoil the consistency of the theory. One may hope that inte- grability can cure these inconsistencies. I studied the problem of constructing the generalization of two-dimensional vii integrable systems by focusing on a very special example, the sine-Gordonthe- ory,describingthedynamicsofascalarfieldgovernedbyanoscillatingpotential. Integrability is a property of the equations of motion and in most cases an ac- tion generating them is not known. The sine-Gordon model is one of the cases whereanactionisalsoknown. Thereforeitispossibletomoveontoaquantum description of the model. The project about the noncommutative sine-Gordon was started by M.T. GrisaruandS.Penatiin[34],wheretheyconstructedanoncommutativeversion ofthesine-Gordonsystembymakinguseofabidifferentialcalculusapproach,so thatitwasguaranteedthatthesystempossessedaninfinitenumberofconserved currents. In the resulting noncommutative model the dynamics of a single, scalar field is described by two equations. The second equations has the form of a conservation law and becomes trivial in the noncommutative limit. This pattern is somehow unavoidable, since it is related to the necessary extension of SU(2) to U(2) in noncommutative geometry [35]. Because of the unusual structure of the equations, in [34] an action for the model was not found. This was the first goal of my paper [36], written in collaboration with M.T. Grisaru, L. Mazzanti and S. Penati. There we found an action for the model and studied its tree-level scattering amplitudes. We discovered that they are plagued by acausality and that particle production occurs. Therefore this model had to be discarded and a different one had to be constructed. In [37], in collaboration with O. Lechtenfeld, L. Mazzanti, S. Penati and A.D.Popov,weproposedanothermodelobtainedbyatwo-stepreductionfrom selfdual Yang-Mills theory, that proved to possess a well-defined, causal and factorizedS-matrix. Moreover,solitonsolutionsofthismodelwereconstructed. Thetwodifferentnoncommutativeversionsofthesine-GordonmodelIstud- ieddifferinthegeneralizationoftheoscillatinginteractionterm. Theycanboth beobtainedbydimensionalreductionfromnoncommutativeselfdualYang-Mills equations, with a different parametrization of the gauge group. The second model is obtained by reducing U(2) to its U(1) U(1) subgroup, which seems × the most natural choice and indeed leads to a successful integrable theory. Thisthesiscontainsfourchapters. Inthefirstone,Iwillgiveanintroduction to Moyal deformation of bosonic spacetime. I will review the main results in noncommutative field theory and in particular I will discuss the problems aris- ing when time is involved in noncommutativity. I will summarize Kontsevich results about coordinate-dependent noncommutativity. I will then move on to supersymmetrictheories,discusstheresultsIobtainedin[26]concerningsuper- spacenon(anti)commutative deformationsin fourdimensions andtheir relation with following works. In the rest of the chapter I will review the string the- oryresults concerningthe lowenergydescriptionofD-branedynamics interms of non(anti)commutative field theory. In particular I will consider the bosonic, RNS,GSandN =2stringsinthepresenceofconstantNS-NSbackgrounds,the covariantsuperstringcompactifiedonaCalabi-Yauthree-foldinthepresenceof a R-Rselfdual field strengthand the generalizationto the uncompactifiedcase. viii

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