Noncritical String Theory
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Noncritical String Theory Sander Walg Master’s thesis Supervisor: Prof. Dr. Jan de Boer University of Amsterdam Institute for Theoretical Physics Valckenierstraat 65 1018 XE Amsterdam The Netherlands August 26, 2008 ii Abstract In strings theory, a critical dimension, Dc is required to yield consistent theories. For bosonic strings Dc = 26 and for superstrings Dc = 10. These numbers arise naturally from the theory itself. Less familiar are noncrit- ical string theories, theories with D 6= Dc. These theories emerge when background fields are included to the theory, in particular linear dilaton backgrounds. We will study quintessence-driven cosmologies and show an analogy between them and string theories in a timelike linear dilaton theory. We will also present a set of exact solutions for the linear dilaton-tachyon profile system that gives rise to a bubble of nothing. Generalizing this set- ting induces a dimension-changing bubble, which can also be solved exactly at one-loop order. Eventually, we will consider transitions from one theory to another. In this way, noncritical string theories can be connected to the familiar web of critical string theories. Surprisingly, transitions from su- perstring theories can yield pure bosonic theories. Our main focus will be bosonic strings. iv Preface Foreword When I started writing my thesis, I was immediately confronted with a tremendous abundancy of background material on string theory. Even though string theory is relatively new, already a lot of books and an enor- mous amount of articles have been written on the subject, and the level of difficulty varies greatly. Some books were very advanced, others were much more comprehensible but somewhat limited in detail. I found it was a challenging task to restrict my focus only on those subjects relevant to the scope of this thesis, because it is very easy to get lost in all the fascinating features and idea’s that are indissoluble connected to string theory. At first I had some doubt whether I should go into a lot of detail with calculations or not. But gradually, I found that I gained most satisfaction out of explaining most of the intermediate steps needed to complete a cal- culation, whenever I thought they contributed to the clarity of the subject. Whenever a calculation would become to detailed or advanced, I decided to give a reference to the book or article the problem can be found in. I wrote this thesis on the level of graduate students, with preliminary knowledge on quantum field theory, general relativity and string theory. Only chapter 3 involves some knowledge on algebra and representations. It will not be used later on. With this in mind, I still tried to make the thesis as self-contained as possible, reviewing some general facts where needed. Just as many people before me, I too found out that writing a thesis is by far the most challenging and difficult task of completing my studies as a physics student. Nevertheless, I’ve experienced this as a very educative and enjoyable time, and during this period I found out that my interest in doing theoretical research has grown considerably. Acknowledgments First of all, I would like to thank my supervisor Jan de Boer, who has always been an inspiration to me and could explain difficult subject in a very clear way. I always enjoyed his lectures a lot and his interpretations truly made vi Preface complicated subjects completely comprehensible. Secondly, I would like to thank my student friends who were always open to questions and discussions and who helped me with some difficulties regarding LATEX. I also like to thank my other friends, who never lost faith in me and always helped me regain new energy. They always showed a lot of interest in my studies and my thesis, and in turn I enjoyed explaining them the exotic features of particle physics, cosmology, black holes and string theory. I would like to thank my girlfriend Sabine Wirz, who often found me completely worn out after a long day at the university and who has always been there for me. She supported me a great deal and absolutely helped me through this period. And finally I would like to thank my family, who I could rely on all my years at University. In particular I would like to thank my father, Hugo Walg, who somehow always managed to get the best out of me and supported me with his technical backup. And last, I would like to thank my mother, Doroth´eevan Wijhe, who was always able to motivate me, and who made it possible for me to graduate this year. I don’t think I could have succeeded successfully without her support. Contents Preface v Notation and conventions xi Introduction xiii I Theoretical frame-work 1 1 Basic principles on string theory 3 1.1 Why string theory? . 3 1.2 Relativistic point particle . 5 1.2.1 Point particle action . 5 1.2.2 Auxiliary field . 5 1.3 Relativistic bosonic strings . 6 1.3.1 Polyakov action . 6 1.3.2 World-sheet symmetries . 8 1.4 Solutions of the bosonic string . 9 1.4.1 Choosing a world-sheet gauge . 9 1.4.2 Constraints for embedding coordinates . 9 1.4.3 Solutions for embedding coordinates . 10 1.5 Quantizing the relativistic string . 12 1.5.1 Commutation relations . 12 1.5.2 Mass levels . 13 2 Scale transformations and interactions 15 2.1 Couplings . 15 2.1.1 Interacting theories . 15 2.1.2 Running couplings and renormalization . 16 2.1.3 Renormalization β functions . 16 2.2 Weyl invariance and Weyl anomaly . 17 2.2.1 Weyl invariance . 17 2.2.2 Path integral approach . 18 2.2.3 Critical dimension . 20 viii CONTENTS 2.3 Fields and target space . 21 3 Conformal field theory 23 3.1 Complex coordinates . 23 3.1.1 Wick rotation . 23 3.1.2 Conformal transformation . 24 3.2 Operator-product expansions . 25 3.2.1 Currents and charges . 25 3.2.2 Generators of conformal transformations . 26 3.2.3 Operator-product expansions . 27 3.2.4 Free bosons and OPE’s . 28 3.3 Virasoro operators . 30 3.3.1 Virasoro algebra . 30 3.3.2 Operator-state correspondence . 31 4 Vertex operators and amplitudes 35 4.1 Operator-state correspondence . 35 4.1.1 Applying CFT to string theory . 35 4.1.2 Introducing the vertex operator . 35 4.2 Tachyon tree-diagrams for open strings . 38 4.2.1 Vertex operators for open strings . 38 4.2.2 Emitting one open tachyon state . 39 4.2.3 2-tachyon open string scattering . 40 4.2.4 Vertex operators for excited states . 42 4.3 Tachyon tree-diagrams for closed strings . 43 4.3.1 Closed string tachyon vertex operators . 43 4.3.2 Closed massless string vertex operator . 44 5 Strings with backgrounds 47 5.1 Strings in curved spacetime . 47 5.1.1 Nonlinear sigma model . 47 5.1.2 Coherent background of gravitons . 48 5.2 Other background fields and β functions . 48 5.2.1 β functions up tp first order in background fields . 48 5.2.2 β functions up to first order in α0 . 50 6 Low energy effective action 53 6.1 The string metric . 53 6.1.1 Equations of motion . 53 6.1.2 Spacetime dependent coupling . 55 6.2 Link between β functions and EOM . 55 6.3 The Einstein metric . 56 6.3.1 Effective action in the Einstein frame . 56 6.3.2 Utility of the Einstein frame . 57 CONTENTS ix II Applications on noncritical string theory 59 7 Away from the critical dimension 61 7.1 Constant dilaton . 61 7.1.1 Constant dilaton action . 61 7.1.2 Euler characteristic . 61 7.1.3 UV finite quantum gravity . 62 7.2 Linear dilaton background . 63 7.3 Tachyon profile . 64 7.3.1 On-shell tachyon condition . 64 7.3.2 Liouville field theory . 66 8 Quintessence-driven cosmologies 69 8.1 Quintessent cosmologies . 69 8.1.1 Quintessence . 69 8.1.2 FRW cosmologies in D dimensions . 70 8.1.3 Determining the critical equation of state . 72 8.2 Global structures in quintessent cosmologies . 73 8.2.1 Global structures . 73 8.2.2 Penrose diagrams . 75 9 String theory with cosmological behaviour 77 9.1 Linear dilaton as quintessent cosmologies . 77 9.1.1 Comparing the two theories . 77 9.1.2 Fixing the scale factor . 78 9.2 Stable modes . 80 9.2.1 Stability . 80 9.2.2 Massless modes . 81 9.2.3 Massive modes . 83 10 Exact tachyon-dilaton dynamics 85 10.1 Exact solutions and Feynmann diagrams . 85 10.1.1 Lightcone gauge . 85 10.1.2 Exact solutions . 87 10.2 Bubble of nothing . 88 10.2.1 Bubble of nothing . 88 10.2.2 Particle trajectories . 90 10.3 Tachyon-dilaton low energy effective action . 92 10.3.1 General two-derivative form . 92 10.3.2 Determining the final form . 94 x CONTENTS 11 Dimension-changing solutions 97 11.1 Dimension-change for the bosonic string . 97 11.1.1 Oscillatory dependence in the X2 direction . 97 11.1.2 Classical world-sheet solutions . 99 11.1.3 An energy consideration . 100 11.1.4 Oscillatory dependence on more coordinates . 102 11.2 Quantum corrections . 104 11.2.1 Exact solutions at one-loop order . 104 11.2.2 Dynamical readjustment . 107 11.3 Dimension-change for superstrings . 108 11.3.1 Superstring theories . 108 11.3.2 Transitions among various string theories . 109 12 Summary 111 A Renormalized operators 115 B Curvature 117 B.1 Path length and proper time .