String Field Theory, Nuclear Physics B271 (1986) 540
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Duality and Strings Dieter Lüst, LMU and MPI München
Duality and Strings Dieter Lüst, LMU and MPI München Freitag, 15. März 13 Luis made several very profound and important contributions to theoretical physics ! Freitag, 15. März 13 Luis made several very profound and important contributions to theoretical physics ! Often we were working on related subjects and I enjoyed various very nice collaborations and friendship with Luis. Freitag, 15. März 13 Luis made several very profound and important contributions to theoretical physics ! Often we were working on related subjects and I enjoyed various very nice collaborations and friendship with Luis. Duality of 4 - dimensional string constructions: • Covariant lattices ⇔ (a)symmetric orbifolds (1986/87: W. Lerche, D.L., A. Schellekens ⇔ L. Ibanez, H.P. Nilles, F. Quevedo) • Intersecting D-brane models ☞ SM (?) (2000/01: R. Blumenhagen, B. Körs, L. Görlich, D.L., T. Ott ⇔ G. Aldazabal, S. Franco, L. Ibanez, F. Marchesano, R. Rabadan, A. Uranga) Freitag, 15. März 13 Luis made several very profound and important contributions to theoretical physics ! Often we were working on related subjects and I enjoyed various very nice collaborations and friendship with Luis. Duality of 4 - dimensional string constructions: • Covariant lattices ⇔ (a)symmetric orbifolds (1986/87: W. Lerche, D.L., A. Schellekens ⇔ L. Ibanez, H.P. Nilles, F. Quevedo) • Intersecting D-brane models ☞ SM (?) (2000/01: R. Blumenhagen, B. Körs, L. Görlich, D.L., T. Ott ⇔ G. Aldazabal, S. Franco, L. Ibanez, F. Marchesano, R. Rabadan, A. Uranga) ➢ Madrid (Spanish) Quiver ! Freitag, 15. März 13 Luis made several very profound and important contributions to theoretical physics ! Often we were working on related subjects and I enjoyed various very nice collaborations and friendship with Luis. -
From Vibrating Strings to a Unified Theory of All Interactions
Barton Zwiebach From Vibrating Strings to a Unified Theory of All Interactions or the last twenty years, physicists have investigated F String Theory rather vigorously. The theory has revealed an unusual depth. As a result, despite much progress in our under- standing of its remarkable properties, basic features of the theory remain a mystery. This extended period of activity is, in fact, the second period of activity in string theory. When it was first discov- ered in the late 1960s, string theory attempted to describe strongly interacting particles. Along came Quantum Chromodynamics— a theoryof quarks and gluons—and despite their early promise, strings faded away. This time string theory is a credible candidate for a theoryof all interactions—a unified theoryof all forces and matter. The greatest complication that frustrated the search for such a unified theorywas the incompatibility between two pillars of twen- tieth century physics: Einstein’s General Theoryof Relativity and the principles of Quantum Mechanics. String theory appears to be 30 ) zwiebach mit physics annual 2004 the long-sought quantum mechani- cal theory of gravity and other interactions. It is almost certain that string theory is a consistent theory. It is less certain that it describes our real world. Nevertheless, intense work has demonstrated that string theory incorporates many features of the physical universe. It is reasonable to be very optimistic about the prospects of string theory. Perhaps one of the most impressive features of string theory is the appearance of gravity as one of the fluctuation modes of a closed string. Although it was not discov- ered exactly in this way, we can describe a logical path that leads to the discovery of gravity in string theory. -
Introduction to Conformal Field Theory and String
SLAC-PUB-5149 December 1989 m INTRODUCTION TO CONFORMAL FIELD THEORY AND STRING THEORY* Lance J. Dixon Stanford Linear Accelerator Center Stanford University Stanford, CA 94309 ABSTRACT I give an elementary introduction to conformal field theory and its applications to string theory. I. INTRODUCTION: These lectures are meant to provide a brief introduction to conformal field -theory (CFT) and string theory for those with no prior exposure to the subjects. There are many excellent reviews already available (or almost available), and most of these go in to much more detail than I will be able to here. Those reviews con- centrating on the CFT side of the subject include refs. 1,2,3,4; those emphasizing string theory include refs. 5,6,7,8,9,10,11,12,13 I will start with a little pre-history of string theory to help motivate the sub- ject. In the 1960’s it was noticed that certain properties of the hadronic spectrum - squared masses for resonances that rose linearly with the angular momentum - resembled the excitations of a massless, relativistic string.14 Such a string is char- *Work supported in by the Department of Energy, contract DE-AC03-76SF00515. Lectures presented at the Theoretical Advanced Study Institute In Elementary Particle Physics, Boulder, Colorado, June 4-30,1989 acterized by just one energy (or length) scale,* namely the square root of the string tension T, which is the energy per unit length of a static, stretched string. For strings to describe the strong interactions fi should be of order 1 GeV. Although strings provided a qualitative understanding of much hadronic physics (and are still useful today for describing hadronic spectra 15 and fragmentation16), some features were hard to reconcile. -
Introduction to String Theory A.N
Introduction to String Theory A.N. Schellekens Based on lectures given at the Radboud Universiteit, Nijmegen Last update 6 July 2016 [Word cloud by www.worldle.net] Contents 1 Current Problems in Particle Physics7 1.1 Problems of Quantum Gravity.........................9 1.2 String Diagrams................................. 11 2 Bosonic String Action 15 2.1 The Relativistic Point Particle......................... 15 2.2 The Nambu-Goto action............................ 16 2.3 The Free Boson Action............................. 16 2.4 World sheet versus Space-time......................... 18 2.5 Symmetries................................... 19 2.6 Conformal Gauge................................ 20 2.7 The Equations of Motion............................ 21 2.8 Conformal Invariance.............................. 22 3 String Spectra 24 3.1 Mode Expansion................................ 24 3.1.1 Closed Strings.............................. 24 3.1.2 Open String Boundary Conditions................... 25 3.1.3 Open String Mode Expansion..................... 26 3.1.4 Open versus Closed........................... 26 3.2 Quantization.................................. 26 3.3 Negative Norm States............................. 27 3.4 Constraints................................... 28 3.5 Mode Expansion of the Constraints...................... 28 3.6 The Virasoro Constraints............................ 29 3.7 Operator Ordering............................... 30 3.8 Commutators of Constraints.......................... 31 3.9 Computation of the Central Charge..................... -
Achievements, Progress and Open Questions in String Field Theory Strings 2021 ICTP-SAIFR, S˜Ao Paulo June 22, 2021
Achievements, Progress and Open Questions in String Field Theory Strings 2021 ICTP-SAIFR, S˜ao Paulo June 22, 2021 Yuji Okawa and Barton Zwiebach 1 Achievements We consider here instances where string field theory provided the answer to physical open questions. • Tachyon condensation, tachyon vacuum, tachyon conjectures The tachyon conjectures (Sen, 1999) posited that: (a) The tachyon potential has a locally stable minimum, whose energy density measured with respect to that of the unstable critical point, equals minus the tension of the D25-brane (b) Lower-dimensional D-branes are solitonic solutions of the string theory on the back- ground of a D25-brane. (c) The locally stable vacuum of the system is the closed string vac- uum; it has no open string excitations exist. Work in SFT established these conjectures by finding the tachyon vac- uum, first numerically, and then analytically (Schnabl, 2005). These are non-perturbative results. 2 • String field theory is the first complete definition of string pertur- bation theory. The first-quantized world-sheet formulation of string theory does not define string perturbation theory completely: – No systematic way of dealing with IR divergences. – No systematic way of dealing with S-matrix elements for states that undergo mass renormalization. Work of A. Sen and collaborators demonstrating this: (a) One loop-mass renormalization of unstable particles in critical string theories. (b) Fixing ambiguities in two-dimensional string theory: For the one- instanton contribution to N-point scattering amplitudes there are four undetermined constants (Balthazar, Rodriguez, Yin, 2019). Two of them have been fixed with SFT (Sen 2020) (c) Fixing the normalization of Type IIB D-instanton amplitudes (Sen, 2021). -
Chapter 9: the 'Emergence' of Spacetime in String Theory
Chapter 9: The `emergence' of spacetime in string theory Nick Huggett and Christian W¨uthrich∗ May 21, 2020 Contents 1 Deriving general relativity 2 2 Whence spacetime? 9 3 Whence where? 12 3.1 The worldsheet interpretation . 13 3.2 T-duality and scattering . 14 3.3 Scattering and local topology . 18 4 Whence the metric? 20 4.1 `Background independence' . 21 4.2 Is there a Minkowski background? . 24 4.3 Why split the full metric? . 27 4.4 T-duality . 29 5 Quantum field theoretic considerations 29 5.1 The graviton concept . 30 5.2 Graviton coherent states . 32 5.3 GR from QFT . 34 ∗This is a chapter of the planned monograph Out of Nowhere: The Emergence of Spacetime in Quantum Theories of Gravity, co-authored by Nick Huggett and Christian W¨uthrich and under contract with Oxford University Press. More information at www.beyondspacetime.net. The primary author of this chapter is Nick Huggett ([email protected]). This work was sup- ported financially by the ACLS and the John Templeton Foundation (the views expressed are those of the authors not necessarily those of the sponsors). We want to thank Tushar Menon and James Read for exceptionally careful comments on a draft this chapter. We are also grateful to Niels Linnemann for some helpful feedback. 1 6 Conclusions 35 This chapter builds on the results of the previous two to investigate the extent to which spacetime might be said to `emerge' in perturbative string the- ory. Our starting point is the string theoretic derivation of general relativity explained in depth in the previous chapter, and reviewed in x1 below (so that the philosophical conclusions of this chapter can be understood by those who are less concerned with formal detail, and so skip the previous one). -
String Field Theory, Nucl
1 String field theory W. TAYLOR MIT, Stanford University SU-ITP-06/14 MIT-CTP-3747 hep-th/0605202 Abstract This elementary introduction to string field theory highlights the fea- tures and the limitations of this approach to quantum gravity as it is currently understood. String field theory is a formulation of string the- ory as a field theory in space-time with an infinite number of massive fields. Although existing constructions of string field theory require ex- panding around a fixed choice of space-time background, the theory is in principle background-independent, in the sense that different back- grounds can be realized as different field configurations in the theory. String field theory is the only string formalism developed so far which, in principle, has the potential to systematically address questions involv- ing multiple asymptotically distinct string backgrounds. Thus, although it is not yet well defined as a quantum theory, string field theory may eventually be helpful for understanding questions related to cosmology arXiv:hep-th/0605202v2 28 Jun 2006 in string theory. 1.1 Introduction In the early days of the subject, string theory was understood only as a perturbative theory. The theory arose from the study of S-matrices and was conceived of as a new class of theory describing perturbative interactions of massless particles including the gravitational quanta, as well as an infinite family of massive particles associated with excited string states. In string theory, instead of the one-dimensional world line 1 2 W. Taylor of a pointlike particle tracing out a path through space-time, a two- dimensional surface describes the trajectory of an oscillating loop of string, which appears pointlike only to an observer much larger than the string. -
Exceptional Field Theory and Supergravity Arnaud Baguet
Exceptional Field Theory and Supergravity Arnaud Baguet To cite this version: Arnaud Baguet. Exceptional Field Theory and Supergravity. High Energy Physics - Experiment [hep-ex]. Université de Lyon, 2017. English. NNT : 2017LYSEN022. tel-01563063 HAL Id: tel-01563063 https://tel.archives-ouvertes.fr/tel-01563063 Submitted on 17 Jul 2017 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Numéro National de Thèse : 2017LYSEN022 Thèse de Doctorat de l’Université de Lyon opérée par l’École Normale Supérieure de Lyon École Doctorale 52 École Doctorale de Physique et d’Astrophysique de Lyon Soutenue publiquement le 30/06/2017, par : Arnaud Baguet Exceptional Field Theory and Supergravity - Théorie des Champs Exceptionnels et Supergravité Devant le jury composé de : Martin Cederwall Chalmers University of Technology Rapporteur François Delduc École Normale Supérieure de Lyon Examinateur Axel Kleinschmidt Max Planck Institute Postdam Rapporteur Michela Petrini Université Pierre et Marie Curie Examinatrice Henning Samtleben École Normale Supérieure de Lyon Directeur Contents 1 Introduction 9 1.1 String theory, dualities and supergravity . 11 1.2 The bosonic string . 13 1.3 Compactification and T-duality . 18 1.4 Double Field Theory . 21 1.5 Exceptional Field Theory . -
Kaluza-Klein Theories
Kaluza-Klein for Kids William O. Straub Pasadena, California 91104 June 27, 2014 Abstract A very elementary overview of the original Kaluza-Klein theory is presented, suitable for undergraduates who want to learn the basic mathematical formalism behind a revolutionary idea that was proposed one hun- dred years ago, yet today serves as the template for modern higher-dimensional particle and gravity theories. 1. Introduction In the years immediately following Einstein’s November 1915 announcement of the general theory of relativity (GTR), numerous attempts were made by Einstein and others to unify gravitation and electromagnetism, the only forces of Nature then known. These efforts generally involved theories that went outside the formalism of Riemannian geometry; both Einstein and Elie Cartan investigated the nonsymmetry of the GTR metric and connection term, while Hermann Weyl developed a non-Riemannian geometry that initially appeared to include all of electrodynamics as a purely geometrical construct. These efforts failed, as did all similar theories that were proposed over the following decades. In 1919, the German mathematician Theodor Kaluza developed a theory that maintained all the formalism of Riemannian geometry but extended the geometry’s reach by proposing the possibility that Nature in fact utilized a five-dimensional spacetime, with electromagnetism appearing as a natural consequence of the unseen fifth dimension (the same idea was actually proposed by the Finnish physicist Gunnar Nordström in 1914, but was ignored). Kaluza communicated his idea to Einstein in the form of a draft paper, who was initially very enthusiastic about the concept of electromagnetism springing from the fifth dimension. -
Quantum Gravity, Effective Fields and String Theory
Quantum gravity, effective fields and string theory Niels Emil Jannik Bjerrum-Bohr The Niels Bohr Institute University of Copenhagen arXiv:hep-th/0410097v1 10 Oct 2004 Thesis submitted for the degree of Doctor of Philosophy in Physics at the Niels Bohr Institute, University of Copenhagen. 28th July 2 Abstract In this thesis we will look into some of the various aspects of treating general relativity as a quantum theory. The thesis falls in three parts. First we briefly study how gen- eral relativity can be consistently quantized as an effective field theory, and we focus on the concrete results of such a treatment. As a key achievement of the investigations we present our calculations of the long-range low-energy leading quantum corrections to both the Schwarzschild and Kerr metrics. The leading quantum corrections to the pure gravitational potential between two sources are also calculated, both in the mixed theory of scalar QED and quantum gravity and in the pure gravitational theory. Another part of the thesis deals with the (Kawai-Lewellen-Tye) string theory gauge/gravity relations. Both theories are treated as effective field theories, and we investigate if the KLT oper- ator mapping is extendable to the case of higher derivative operators. The constraints, imposed by the KLT-mapping on the effective coupling constants, are also investigated. The KLT relations are generalized, taking the effective field theory viewpoint, and it is noticed that some remarkable tree-level amplitude relations exist between the field the- ory operators. Finally we look at effective quantum gravity treated from the perspective of taking the limit of infinitely many spatial dimensions. -
Black Holes in String Theory and Gravitational Wave Observations
Black holes in string theory and gravitational wave observations Bert Vercnocke KU Leuven Amsterdam, 12 November 2019 Why quantum modifications of GR horizon? Outline 1. Why study black holes in string theory? 2. What is a black hole in string theory? 3. What are the observable consequences? Outline 1. Why study black holes in string theory? 2. What is a black hole in string theory? 3. What are the observable consequences? Resolution is QUANTUM gravitational in nature Why study black holes in string theory? 3 kBc surface gravity SBH = AH ; TH = ~GN 2π [Bekenstein; Hawking; BH thermodynamics Bardeen, Hawking, Carter . ] QFT in a fixed GR background: 1. Evaporation ! information paradox? 2. Entropy ! microstates? 3. Singularity ! Experience of infalling observer? Why study black holes in string theory? 3 kBc surface gravity SBH = AH ; TH = ~GN 2π [Bekenstein; Hawking; BH thermodynamics Bardeen, Hawking, Carter . ] QFT in a fixed GR background: 1. Evaporation ! information paradox? 2. Entropy ! microstates? 3. Singularity ! Experience of infalling observer? Resolution is QUANTUM gravitational in nature Resolving the information paradox Need to give up at least one of: 1. Unitarity 2. No high-entropy remnants 3. Effective Field Theory outside horizon (GR + QFT) 4. Quantum gravity corrections heavily suppressed near horizon 5. Or other hidden assumptions Some proposed resolutions from the string community non-local interactions [Giddings], wormholes from entanglement[ER=EPR, Maldacena-Susskind] firewalls [AMPS ’13 ], fuzzballs [Mathur ’01 + many more] observables in quantum mechanics depend on black hole microstate [Papadodimas-Raju ’15] Resolve information paradox? Need to give up at least one of: 1. Effective Field Theory (GR + QFT) breaks down 2. -
Black Holes and String Theory
Black Holes and String Theory Hussain Ali Termezy Submitted in partial fulfilment of the requirements for the degree of Master of Science of Imperial College London September 2012 Contents 1 Black Holes in General Relativity 2 1.1 Black Hole Solutions . 2 1.2 Black Hole Thermodynamics . 5 2 String Theory Background 19 2.1 Strings . 19 2.2 Supergravity . 23 3 Type IIB and Dp-brane solutions 25 4 Black Holes in String Theory 33 4.1 Entropy Counting . 33 Introduction The study of black holes has been an intense area of research for many decades now, as they are a very useful theoretical construct where theories of quantum gravity become relevant. There are many curiosities associated with black holes, and the resolution of some of the more pertinent problems seem to require a quantum theory of gravity to resolve. With the advent of string theory, which purports to be a unified quantum theory of gravity, attention has naturally turned to these questions, and have remarkably shown signs of progress. In this project we will first review black hole solutions in GR, and then look at how a thermodynamic description of black holes is made possible. We then turn to introduce string theory and in particular review the black Dp-brane solutions of type IIB supergravity. Lastly we see how to compute a microscopic account of the Bekenstein entropy is given in string theory. 1 Chapter 1 Black Holes in General Relativity 1.1 Black Hole Solutions We begin by reviewing some the basics of black holes as they arise in the study of general relativity.