Supersymmetry, Duality and Bound States
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String Theory. Volume 1, Introduction to the Bosonic String
This page intentionally left blank String Theory, An Introduction to the Bosonic String The two volumes that comprise String Theory provide an up-to-date, comprehensive, and pedagogic introduction to string theory. Volume I, An Introduction to the Bosonic String, provides a thorough introduction to the bosonic string, based on the Polyakov path integral and conformal field theory. The first four chapters introduce the central ideas of string theory, the tools of conformal field theory and of the Polyakov path integral, and the covariant quantization of the string. The next three chapters treat string interactions: the general formalism, and detailed treatments of the tree-level and one loop amplitudes. Chapter eight covers toroidal compactification and many important aspects of string physics, such as T-duality and D-branes. Chapter nine treats higher-order amplitudes, including an analysis of the finiteness and unitarity, and various nonperturbative ideas. An appendix giving a short course on path integral methods is also included. Volume II, Superstring Theory and Beyond, begins with an introduction to supersym- metric string theories and goes on to a broad presentation of the important advances of recent years. The first three chapters introduce the type I, type II, and heterotic superstring theories and their interactions. The next two chapters present important recent discoveries about strongly coupled strings, beginning with a detailed treatment of D-branes and their dynamics, and covering string duality, M-theory, and black hole entropy. A following chapter collects many classic results in conformal field theory. The final four chapters are concerned with four-dimensional string theories, and have two goals: to show how some of the simplest string models connect with previous ideas for unifying the Standard Model; and to collect many important and beautiful general results on world-sheet and spacetime symmetries. -
Lectures on D-Branes
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by CERN Document Server CPHT/CL-615-0698 hep-th/9806199 Lectures on D-branes Constantin P. Bachas1 Centre de Physique Th´eorique, Ecole Polytechnique 91128 Palaiseau, FRANCE [email protected] ABSTRACT This is an introduction to the physics of D-branes. Topics cov- ered include Polchinski’s original calculation, a critical assessment of some duality checks, D-brane scattering, and effective worldvol- ume actions. Based on lectures given in 1997 at the Isaac Newton Institute, Cambridge, at the Trieste Spring School on String The- ory, and at the 31rst International Symposium Ahrenshoop in Buckow. June 1998 1Address after Sept. 1: Laboratoire de Physique Th´eorique, Ecole Normale Sup´erieure, 24 rue Lhomond, 75231 Paris, FRANCE, email : [email protected] Lectures on D-branes Constantin Bachas 1 Foreword Referring in his ‘Republic’ to stereography – the study of solid forms – Plato was saying : ... for even now, neglected and curtailed as it is, not only by the many but even by professed students, who can suggest no use for it, never- theless in the face of all these obstacles it makes progress on account of its elegance, and it would not be astonishing if it were unravelled. 2 Two and a half millenia later, much of this could have been said for string theory. The subject has progressed over the years by leaps and bounds, despite periods of neglect and (understandable) criticism for lack of direct experimental in- put. To be sure, the construction and key ingredients of the theory – gravity, gauge invariance, chirality – have a firm empirical basis, yet what has often catalyzed progress is the power and elegance of the underlying ideas, which look (at least a posteriori) inevitable. -
Towards a String Dual of SYK Arxiv:2103.03187V1 [Hep-Th] 4 Mar
Towards A String Dual of SYK Akash Goel and Herman Verlinde Department of Physics, Princeton University, Princeton, NJ 08544, USA Abstract: We propose a paradigm for realizing the SYK model within string theory. Using the large N matrix description of c < 1 string theory, we show that the effective theory on a large number Q of FZZT D-branes in (p; 1) minimal string theory takes the form of the disorder averaged SYK model with J p interaction. The SYK fermions represent open strings between the FZZT branes and the ZZ branes that underly the matrix model. The continuum SYK dynamics arises upon taking the large Q limit. We observe several qualitative and quantitative links between the SYK model and (p; q) minimal string theory and propose that the two describe different phases of a single system. We comment on the dual string interpretation of double scaled SYK and on the relevance of our results to the recent discussion of the role of ensemble averaging in holography. arXiv:2103.03187v2 [hep-th] 24 Aug 2021 Contents 1 Introduction2 2 SYK from the Two Matrix Model4 2.1 FZZT-branes in the two matrix model4 2.2 Kontsevich matrix model from FZZT branes6 2.3 SYK matrix model from FZZT branes7 3 Towards the Continuum SYK model8 3.1 Non-commutative SYK8 4 From Minimal Strings to SYK 10 4.1 SYK and the (p; q) spectral curve 11 4.2 FZZT brane correlation function 12 4.3 Minimal String-SYK phase diagram 13 5 SYK as a Non-Critical String 14 6 Conclusion 16 A D-branes in Minimal String Theory 18 A.1 Matrices and the non-commutative torus 23 A.2 Non-commutative SYK 24 A.3 Matrix SYK 26 A.4 Mapping between Matrix SYK and Non-Commutative SYK 27 { 1 { 1 Introduction The SYK model is the prototype of a maximally chaotic quantum system with low energy dynamics given by near-AdS2 gravity. -
Pitp Lectures
MIFPA-10-34 PiTP Lectures Katrin Becker1 Department of Physics, Texas A&M University, College Station, TX 77843, USA [email protected] Contents 1 Introduction 2 2 String duality 3 2.1 T-duality and closed bosonic strings .................... 3 2.2 T-duality and open strings ......................... 4 2.3 Buscher rules ................................ 5 3 Low-energy effective actions 5 3.1 Type II theories ............................... 5 3.1.1 Massless bosons ........................... 6 3.1.2 Charges of D-branes ........................ 7 3.1.3 T-duality for type II theories .................... 7 3.1.4 Low-energy effective actions .................... 8 3.2 M-theory ................................... 8 3.2.1 2-derivative action ......................... 8 3.2.2 8-derivative action ......................... 9 3.3 Type IIB and F-theory ........................... 9 3.4 Type I .................................... 13 3.5 SO(32) heterotic string ........................... 13 4 Compactification and moduli 14 4.1 The torus .................................. 14 4.2 Calabi-Yau 3-folds ............................. 16 5 M-theory compactified on Calabi-Yau 4-folds 17 5.1 The supersymmetric flux background ................... 18 5.2 The warp factor ............................... 18 5.3 SUSY breaking solutions .......................... 19 1 These are two lectures dealing with supersymmetry (SUSY) for branes and strings. These lectures are mainly based on ref. [1] which the reader should consult for original references and additional discussions. 1 Introduction To make contact between superstring theory and the real world we have to understand the vacua of the theory. Of particular interest for vacuum construction are, on the one hand, D-branes. These are hyper-planes on which open strings can end. On the world-volume of coincident D-branes, non-abelian gauge fields can exist. -
Duality and the Nature of Quantum Space-Time
Duality and the nature of quantum space-time Sanjaye Ramgoolam Queen Mary, University of London Oxford, January 24, 2009 INTRODUCTION Strings provide a working theory of quantum gravity existing in harmony with particle physics Successes include computations of quantum graviton scattering, new models of beyond-standard-model particle physics based on branes, computation of black hole entropy A powerful new discovery : Duality I An unexpected equivalence between two systems, which a priori look completely unrelated, if not manifest opposites. I Large and Small (T-duality) I Gravitational and non-Gravitational. (Gauge-String duality) Unification and Duality I They are both powerful results of string theory. They allow us to calculate things we could not calculate before. I Unification : We asked for it and found it. We kind of know why it had to be there. I Duality : We didn’t ask for it. We use it. We don’t know what it really means. Unification v/s Duality I Unification has an illustrious history dating back to the days of Maxwell. I Before Maxwell, we thought magnets attracting iron on the one hand and lightning on the other had nothing to do with each other I After Maxwell : Magnets produce B-field. Electric discharge in lightning is caused by E-fields. The coupled equations of both allow fluctuating E, B-fields which transport energy travelling at the speed of light. In fact light is electromagnetic waves. Unification v/s Duality I Einstein tried to unify gravity with quantum phsyics. I String Theory goes a long way. I Computes graviton interaction probablities. -
8. Compactification and T-Duality
8. Compactification and T-Duality In this section, we will consider the simplest compactification of the bosonic string: a background spacetime of the form R1,24 S1 (8.1) ⇥ The circle is taken to have radius R, so that the coordinate on S1 has periodicity X25 X25 +2⇡R ⌘ We will initially be interested in the physics at length scales R where motion on the S1 can be ignored. Our goal is to understand what physics looks like to an observer living in the non-compact R1,24 Minkowski space. This general idea goes by the name of Kaluza-Klein compactification. We will view this compactification in two ways: firstly from the perspective of the spacetime low-energy e↵ective action and secondly from the perspective of the string worldsheet. 8.1 The View from Spacetime Let’s start with the low-energy e↵ective action. Looking at length scales R means that we will take all fields to be independent of X25: they are instead functions only on the non-compact R1,24. Consider the metric in Einstein frame. This decomposes into three di↵erent fields 1,24 on R :ametricG˜µ⌫,avectorAµ and a scalar σ which we package into the D =26 dimensional metric as 2 µ ⌫ 2σ 25 µ 2 ds = G˜µ⌫ dX dX + e dX + Aµ dX (8.2) Here all the indices run over the non-compact directions µ, ⌫ =0 ,...24 only. The vector field Aµ is an honest gauge field, with the gauge symmetry descend- ing from di↵eomorphisms in D =26dimensions.Toseethisrecallthatunderthe transformation δXµ = V µ(X), the metric transforms as δG = ⇤ + ⇤ µ⌫ rµ ⌫ r⌫ µ This means that di↵eomorphisms of the compact direction, δX25 =⇤(Xµ), turn into gauge transformations of Aµ, δAµ = @µ⇤ –197– We’d like to know how the fields Gµ⌫, Aµ and σ interact. -
LOCALIZATION and STRING DUALITY 1. Introduction According
LOCALIZATION AND STRING DUALITY KEFENG LIU 1. Introduction According to string theorists, String Theory, as the most promising candidate for the grand unification of all fundamental forces in the nature, should be the final theory of the world, and should be unique. But now there are five different looking string theories. As argued by the physicists, these theories should be equivalent, in a way dual to each other. On the other hand all previous theories like the Yang-Mills and the Chern-Simons theory should be parts of string theory. In particular their partition functions should be equal or equivalent to each other in the sense that they are equal after certain transformation. To compute partition functions, physicists use localization technique, a modern version of residue theorem, on infinite dimen- sional spaces. More precisely they apply localization formally to path integrals which is not well-defined yet in mathematics. In many cases such computations reduce the path integrals to certain integrals of various Chern classes on various finite dimensional moduli spaces, such as the moduli spaces of stable maps and the moduli spaces of vector bundles. The identifications of these partition functions among different theories have produced many surprisingly beautiful mathematical formulas like the famous mirror formula [22], as well as the Mari˜no-Vafa formula [25]. The mathematical proofs of these formulas from the string duality also depend on localization techniques on these various finite dimensional moduli spaces. The purpose of this note is to discuss our recent work on the subject. I will briefly discuss the proof of the Marin˜o-Vafa formula, its generalizations and the related topological vertex theory [1]. -
New Worldsheet Formulae for Conformal Supergravity Amplitudes
New Worldsheet Formulae for Conformal Supergravity Amplitudes Joseph A. Farrow and Arthur E. Lipstein Department of Mathematical Sciences Durham University, Durham, DH1 3LE, United Kingdom Abstract We use 4d ambitwistor string theory to derive new worldsheet formulae for tree- level conformal supergravity amplitudes supported on refined scattering equations. Unlike the worldsheet formulae for super-Yang-Mills or supergravity, the scattering equations for conformal supergravity are not in general refined by MHV degree. Nevertheless, we obtain a concise worldsheet formula for any number of scalars and gravitons which we lift to a manifestly supersymmetric formula using four types of vertex operators. The theory also contains states with non-plane wave boundary conditions and we show that the corresponding amplitudes can be obtained from plane-wave amplitudes by applying momentum derivatives. Such derivatives are subtle to define since the formulae are intrinsically four-dimensional and on-shell, so we develop a method for computing momentum derivatives of spinor variables. arXiv:1805.04504v3 [hep-th] 11 Jul 2018 1 Contents 1 Introduction 2 2 Review 4 3 Plane Wave Graviton Multiplet Scattering 6 3.1 Supersymmetric Formula . .8 4 Non-Plane Wave Graviton Multiplet Scattering 9 5 Conclusion 11 A BRST Quantization 13 B Derivation of Berkovits-Witten Formula 16 C Momentum Derivatives 17 D Non-plane Wave Examples 19 D.1 Non-plane Wave Scalar . 19 D.2 Non-plane Wave Graviton . 21 1 Introduction Starting with the discovery of the Parke-Taylor formula for tree-level gluon amplitudes [1], the study of scattering amplitudes has suggested intruiging new ways of formulating quantum field theory. -
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). -
Black Holes and the Multiverse
Home Search Collections Journals About Contact us My IOPscience Black holes and the multiverse This content has been downloaded from IOPscience. Please scroll down to see the full text. JCAP02(2016)064 (http://iopscience.iop.org/1475-7516/2016/02/064) View the table of contents for this issue, or go to the journal homepage for more Download details: IP Address: 165.123.34.86 This content was downloaded on 01/03/2016 at 21:11 Please note that terms and conditions apply. ournal of Cosmology and Astroparticle Physics JAn IOP and SISSA journal Black holes and the multiverse Jaume Garriga,a;b Alexander Vilenkinb and Jun Zhangb JCAP02(2016)064 aDepartament de Fisica Fonamental i Institut de Ciencies del Cosmos, Universitat de Barcelona, Marti i Franques, 1, Barcelona, 08028 Spain bInstitute of Cosmology, Tufts University, 574 Boston Ave, Medford, MA, 02155 U.S.A. E-mail: [email protected], [email protected], [email protected] Received December 28, 2015 Accepted February 3, 2016 Published February 25, 2016 Abstract. Vacuum bubbles may nucleate and expand during the inflationary epoch in the early universe. After inflation ends, the bubbles quickly dissipate their kinetic energy; they come to rest with respect to the Hubble flow and eventually form black holes. The fate of the bubble itself depends on the resulting black hole mass. If the mass is smaller than a certain critical value, the bubble collapses to a singularity. Otherwise, the bubble interior inflates, forming a baby universe, which is connected to the exterior FRW region by a wormhole. -
Introduction to the Ads/CFT Correspondence Outline I CFT
Introduction to the AdS/CFT correspondence Outline I CFT review II AdS/CFT correspondence |||||||||||||||||||||||| III Large N review 5 IV D3 branes and AdS5×S |||||||||||||||||| V Finite T, probe branes, quarks, other extensions 1 0 References Descriptive: • B. Zwiebach, \A first course in string theory," 2nd ed., (Cambridge, 2004). • S. S. Gubser and A. Karch, \From gauge-string duality to strong in- teractions: a pedestrian's guide," [arXiv:0901.0935]. Detailed: • O. Aharony, S. S. Gubser, J. M. Maldacena, H. Ooguri and Y. Oz, \Large N field theories, string theory and gravity," [arXiv:hep-th/9905111]. • I. R. Klebanov and E. Witten, \AdS/CFT correspondence and sym- metry breaking," [arXiv:hep-th/9905104]. • E. D'Hoker and D. Z. Freedman, \Supersymmetric gauge theories and the AdS/CFT correspondence," [arXiv:hep-th/0201253]. • K. Skenderis, \Lecture notes on holographic renormalization," [arXiv:hep- th/0209067]. 2 I CFT review Scale-invariant quantum field theories are important as possible end- points of RG flows. Knowledge of them and their relevant deformations (partially) organizes the space of QFTs. UV CFT CFT IR CFT It is believed that unitary scale-invariant theories are also conformally invariant: the space-time symmetry group Poincar´ed×Dilatations en- larges to the Conformald group. (d = no. of space-time dimensions.) Equivalently, there exists a local, conserved, traceless energy-momentum tensor T µν(x). 3 CFT review: conformal algebra Conformald = group of reparameterizations which preserve the (flat) space-time metric up to -
T ¯ T Deformed CFT As a Non-Critical String Arxiv:1910.13578V1 [Hep-Th]
Prepared for submission to JHEP T T¯ deformed CFT as a non-critical string Nele Callebaut,a;c;d Jorrit Kruthoffb and Herman Verlindea aJoseph Henry Laboratories, Princeton University, Princeton, NJ 08544, USA bStanford Institute for Theoretical Physics, Stanford University, Stanford, CA 94305, USA cDepartment of Physics and Astronomy, Ghent University, Krijgslaan 281-S9, 9000 Gent, Belgium dDepartment of Mathematics and Haifa Research Center for Theoretical Physics and Astrophysics, University of Haifa, Haifa 31905, Israel Abstract: We present a new exact treatment of T T¯ deformed 2D CFT in terms of the world- sheet theory of a non-critical string. The transverse dimensions of the non-critical string are represented by the undeformed CFT, while the two longitudinal light-cone directions are de- scribed by two scalar fields X+ and X− with free field OPE's but with a modified stress tensor, arranged so that the total central charge adds up to 26. The relation between our X± field vari- ables and 2D dilaton gravity is indicated. We compute the physical spectrum and the partition function and find a match with known results. We describe how to compute general correlation functions and present an integral expression for the three point function, which can be viewed as an exact formula for the OPE coefficients of the T T¯ deformed theory. We comment on the relationship with other proposed definitions of local operators. arXiv:1910.13578v1 [hep-th] 29 Oct 2019 Contents 1 Introduction2 2 A non-perturbative definition of T T¯ 3 2.1 T T¯ at c = 24 as a