An Introduction to Conformal Invariance in String Theory
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Spectra of Conformal Sigma Models
Spectra of Conformal Sigma Models Dissertation zur Erlangung des Doktorgrades an der Fakultät für Mathematik, Informatik und Naturwissenschaften Fachbereich Physik der Universität Hamburg vorgelegt von Václav Tlapák aus Berlin Hamburg 2014 Tag der Disputation: 30. Januar 2015 Folgende Gutachter empfehlen die Annahme der Dissertation: Prof. Dr. Volker Schomerus Prof. Dr. Gleb Arutyunov Zusammenfassung Die vorliegende Arbeit beschäftigt sich mit den Spektren von konformen Sigma Modellen, die auf (verallgemeinerten) symmetrischen Räumen defi- niert sind. Die Räume, auf denen Sigma Modelle ohne Wess-Zumino-Term konform sind, sind Supermannigfaltigkeiten, also Mannigfaltigkeiten, die fermionische Richtungen aufweisen. Wir stellen die Konstruktion von Ver- tex Operatoren vor, gefolgt von der Hintergrundfeld-Entwicklung. Für semi- symmetrische Räume berechnen wir anschließend die diagonalen Terme der anomalen Dimensionen dieser Operatoren in führender Ordnung. Das Resul- tat stimmt mit dem für symmetrische Räume überein, jedoch treten nicht- diagonale Terme auf, die hier nicht weiter betrachtet werden. Anschließend präsentieren wir eine detaillierte Analyse des Spectrums des Supersphären S3j2 Sigma Modells. Dies ist eins der einfachsten Beispie- le für konforme Sigma Modelle auf symmetrischen Räumen und dient als Illustration für die Mächtigkeit der vorgestellten Methoden. Wir verwenden die erhaltenen Daten, um eine Dualität mit dem OSP(4j2) Gross-Neveu Modell zu untersuchen, die von Candu und Saleur vorgeschlagen wurde. Wir verwenden dazu ein Resultat, welches die anomalen Dimensionen von 1 2 BPS Operatoren zu allen Ordnungen berechnet. Wir finden das gesamte Grundzustandsspektrum des Sigma Modells. Darüber hinaus legen wir dar, dass sowohl die Zwangsbedingungen als auch die Bewegungsgleichungen des Sigma Modells korrekt vom Gross-Neveu Modell implementiert werden. Die Dualität wird weiterhin durch ein neues exaktes Resultat für die anomalen Dimensionen der Grundzustände unterstützt. -
Durham Research Online
Durham Research Online Deposited in DRO: 30 January 2017 Version of attached le: Published Version Peer-review status of attached le: Peer-reviewed Citation for published item: Bhattacharya, Jyotirmoy and Lipstein, Arthur E. (2016) '6d dual conformal symmetry and minimal volumes in AdS.', Journal of high energy physics., 2016 (12). p. 105. Further information on publisher's website: https://doi.org/10.1007/JHEP12(2016)105 Publisher's copyright statement: Open Access, c The Authors. Article funded by SCOAP3. This article is distributed under the terms of the Creative Commons Attribution License (CC-BY 4.0), which permits any use, distribution and reproduction in any medium, provided the original author(s) and source are credited. Additional information: Use policy The full-text may be used and/or reproduced, and given to third parties in any format or medium, without prior permission or charge, for personal research or study, educational, or not-for-prot purposes provided that: • a full bibliographic reference is made to the original source • a link is made to the metadata record in DRO • the full-text is not changed in any way The full-text must not be sold in any format or medium without the formal permission of the copyright holders. Please consult the full DRO policy for further details. Durham University Library, Stockton Road, Durham DH1 3LY, United Kingdom Tel : +44 (0)191 334 3042 | Fax : +44 (0)191 334 2971 https://dro.dur.ac.uk Published for SISSA by Springer Received: November 16, 2016 Revised: December 8, 2016 Accepted: December 12, 2016 Published: December 20, 2016 6d dual conformal symmetry and minimal volumes JHEP12(2016)105 in AdS Jyotirmoy Bhattacharya and Arthur E. -
Conformal Symmetry in Field Theory and in Quantum Gravity
universe Review Conformal Symmetry in Field Theory and in Quantum Gravity Lesław Rachwał Instituto de Física, Universidade de Brasília, Brasília DF 70910-900, Brazil; [email protected] Received: 29 August 2018; Accepted: 9 November 2018; Published: 15 November 2018 Abstract: Conformal symmetry always played an important role in field theory (both quantum and classical) and in gravity. We present construction of quantum conformal gravity and discuss its features regarding scattering amplitudes and quantum effective action. First, the long and complicated story of UV-divergences is recalled. With the development of UV-finite higher derivative (or non-local) gravitational theory, all problems with infinities and spacetime singularities might be completely solved. Moreover, the non-local quantum conformal theory reveals itself to be ghost-free, so the unitarity of the theory should be safe. After the construction of UV-finite theory, we focused on making it manifestly conformally invariant using the dilaton trick. We also argue that in this class of theories conformal anomaly can be taken to vanish by fine-tuning the couplings. As applications of this theory, the constraints of the conformal symmetry on the form of the effective action and on the scattering amplitudes are shown. We also remark about the preservation of the unitarity bound for scattering. Finally, the old model of conformal supergravity by Fradkin and Tseytlin is briefly presented. Keywords: quantum gravity; conformal gravity; quantum field theory; non-local gravity; super- renormalizable gravity; UV-finite gravity; conformal anomaly; scattering amplitudes; conformal symmetry; conformal supergravity 1. Introduction From the beginning of research on theories enjoying invariance under local spacetime-dependent transformations, conformal symmetry played a pivotal role—first introduced by Weyl related changes of meters to measure distances (and also due to relativity changes of periods of clocks to measure time intervals). -
Conformal Theory of Everything (CTOE)
Conformal theory of everything F. F. Faria ∗ Centro de Ciˆencias da Natureza, Universidade Estadual do Piau´ı, 64002-150 Teresina, PI, Brazil Abstract By using conformal symmetry we unify the standard model of par- ticle physics with gravity in a consistent quantum field theory which describes all the fundamental particles and forces of nature. arXiv:1903.04893v3 [hep-ph] 26 Feb 2020 PACS numbers: 104.60.-m, 98.80.-k, 04.50.+h * [email protected] 1 Introduction It is well know that the standard model (SM) of particle physics is consistent with the experiments performed so far on particle accelerators such as the large hadron collider (LHC). However, the theory presents some problems such as the hierarchy and the Landau pole problems. Several modifications of the SM at scales between the electroweak and Planck scales, such as GUT [1, 2, 3, 4] or SUSY [5, 6, 7, 8, 9, 10, 11, 12, 13], have been proposed to solve such problems. However, it is likely that there is no new physics beyond the SM all the way up to the Planck scale [14]. This leads us to suppose that the SM is a low energy limit of a fundamental theory defined at the Planck scale. Since gravitational effects are expected to be important around the Planck scale, it is natural to conjecture that this fundamental theory includes quantum gravity. One of the most straightforward ways to extend and unify physical the- ories is to change the symmetry of their actions. A strong candidate to be incorporated in the unification of the SM with gravity is the (local) conformal symmetry, which performs a multiplicative rescaling of all fields according to Φ=Ω(˜ x)−∆Φ Φ, (1) where Ω(x) is an arbitrary function of the spacetime coordinates, and ∆Φ is the scaling dimension of the field Φ, whose values are 2 for the metric field, 0 for gauge bosons, 1 for scalar fields, and 3/2 for fermions.− The consideration of the conformal symmetry as one of the fundamen- tal symmetries of physics is justified for several reasons. -
Conformally Invariant Equations for Graviton 50 5.1 the Conformally Invariant System of Conformal Degree 1
Conformally Invariant Equations for Graviton Mohsen Fathi Department of Physics, Tehran Central Branch Islamic Azad Univeristy arXiv:1210.3436v3 [physics.gen-ph] 12 Nov 2012 A thesis submitted for the Master degree Master of Science in Physics Tehran, Winter 2010 I am grateful to my supervisor Dr. Mohammad Reza Tanhayi for the helps, supports and scientific training, during this work and thereafter. Abstract Recent astrophysical data indicate that our universe might currently be in a de Sitter (dS) phase. The importance of dS space has been primarily ignited by the study of the inflationary model of the universe and the quantum gravity. As we know Einstein’s theory of gravitation (with a nonzero cosmological constant) can be interpreted as a theory of a metric field; that is, a symmetric tensor field of rank-2 on a fixed de Sitter back- ground. It has been shown the massless spin-2 Fierz-Pauli wave equation (or the linearized Einstein equation) is not conformally invariant. This result is in contrary with what we used to expect for massless theories. In this thesis we obtain conformally invariant wave equation for the massless spin-2 in the dS space. This study is motivated by the belief that confor- mal invariance may be the key to a future theory of quantum gravity. Contents Introduction 1 1 The Lorentz and the conformal groups, and the concept of invari- ance 3 1.1 Grouptheory ............................... 3 1.1.1 Orthogonalgroups ........................ 4 1.1.2 Rotationgroups.......................... 5 1.2 Invarianceunderagroupaction . 7 1.2.1 Invarianceofthelawsofphysics. 7 1.3 TheLorentzgroup ............................ 8 1.4 Theconformalgroup .......................... -
Twenty Years of the Weyl Anomaly
CTP-TAMU-06/93 Twenty Years of the Weyl Anomaly † M. J. Duff ‡ Center for Theoretical Physics Physics Department Texas A & M University College Station, Texas 77843 ABSTRACT In 1973 two Salam prot´eg´es (Derek Capper and the author) discovered that the conformal invariance under Weyl rescalings of the metric tensor 2 gµν(x) Ω (x)gµν (x) displayed by classical massless field systems in interac- tion with→ gravity no longer survives in the quantum theory. Since then these Weyl anomalies have found a variety of applications in black hole physics, cosmology, string theory and statistical mechanics. We give a nostalgic re- view. arXiv:hep-th/9308075v1 16 Aug 1993 CTP/TAMU-06/93 July 1993 †Talk given at the Salamfest, ICTP, Trieste, March 1993. ‡ Research supported in part by NSF Grant PHY-9106593. When all else fails, you can always tell the truth. Abdus Salam 1 Trieste and Oxford Twenty years ago, Derek Capper and I had embarked on our very first post- docs here in Trieste. We were two Salam students fresh from Imperial College filled with ideas about quantizing the gravitational field: a subject which at the time was pursued only by mad dogs and Englishmen. (My thesis title: Problems in the Classical and Quantum Theories of Gravitation was greeted with hoots of derision when I announced it at the Cargese Summer School en route to Trieste. The work originated with a bet between Abdus Salam and Hermann Bondi about whether you could generate the Schwarzschild solution using Feynman diagrams. You can (and I did) but I never found out if Bondi ever paid up.) Inspired by Salam, Capper and I decided to use the recently discovered dimensional regularization1 to calculate corrections to the graviton propaga- tor from closed loops of massless particles: vectors [1] and spinors [2], the former in collaboration with Leopold Halpern. -
8.821 String Theory Fall 2008
MIT OpenCourseWare http://ocw.mit.edu 8.821 String Theory Fall 2008 For information about citing these materials or our Terms of Use, visit: http://ocw.mit.edu/terms. 8.821 F2008 Lecture 11: CFT continued; geometry of AdS Lecturer: McGreevy October 17, 2008 In this session, we are going to talk about the following topics. 1. We are making a few comments about CFT. 2. We are discussing spheres and hyperboloids. 3. Finally we are focusing on Lorentzian AdS and its boundary. 1 Conformal Symmetry 1.1 Weyl anomaly Quantumly, conformal symmetry in a curved space (with even number of dimensions) could be anomalous, that is ds2 → Ω(x)ds2 could be no longer a symmetry of the full quantum theory. This µ anomaly can be evaluated from the following diagram with operator Tµ inserted at the left vertex. Figure 1: A contribution to the Weyl anomaly. The conformal anomaly signals a nonzero value for the trace of the energy-momentum tensor. In a curved spacetime, it is related to the curvature: µ D/2 Tµ ∼ R 1 where R denotes some scalar contractions of curvature tensors and D is the number of spacetime dimensions; the power is determined by dimensional analysis. For the special case of D = 2, this is c T µ = − R(2) (1) µ 12 where R(2) is the Ricci scalar in two dimensions and c is the central charge of the Virasoro algebra µ of the 2d CFT. Also in D = 4, the anomaly is given by Tµ = aW + cGB where W and B are defined as 1 W = (Weyl tensor)2 = R....R − 2R..R + R2 (2) ... -
Msy QCD-Instantons and Conformal Inversion Symmetry
DE06FA410 DEUTSCHES ELEKTRONEN-SYNCHROTRON ( msy in der HELMHOLTZ-GEMEINSCHAFT \X^fc, DESY-THESIS-2006-018 July 2006 QCD-Instantons and Conformal Inversion Symmetry by D. Klammer ISSN 1435-8085 NOTKESTRASSE 85 - 22607 HAMBURG DESY behält sich alle Rechte für den Fall der Schutzrechtserteilung und für die wirtschaftliche Verwertung der in diesem Bericht enthaltenen Informationen vor. DESY reserves all rights for commercial use of information included in this report, especially in case of filing application for or grant of patents. To be sure that your reports and preprints are promptly included in the HEP literature database send them to (if possible by air mail): DESY DESY Zentralbibliothek Bibliothek Notkestraße 85 Platanenaliee 6 22607 Hamburg 15738Zeuthen Germany Germany QCD-INSTANTONS AND CONFORMAL INVERSION SYMMETRY Diplomarbeit zur Erlangung des akademischen Grades Magistra der Naturwissenschaften durchgefuhrt¨ unter der Betreuung von Dr. Fridger Schrempp am Deutschen Elektronen Synchrotron, Hamburg eingereicht von Daniela Klammer an der Fakult¨at fur¨ Physik der Universit¨at Wien April 2006 2 2 1 Abstract Instantons are an essential and non-perturbative part of Quantum Chromodynamics, the theory of strong interactions. One of the most relevant quantities in the instanton calculus is the instanton-size distribution, which can be described on the one hand within the framework of instanton perturbation theory and on the other hand investigated numerically by means of lattice computations. A rapid onset of a drastic discrepancy between these respective results indicates that the under- lying physics is not yet well understood. In this work we investigate the appealing possibility of a symmetry under conformal inversion of space-time leading to this deviation. -
Effective Conformal Descriptions of Black Hole Entropy
Entropy 2011, 13, 1355-1379; doi:10.3390/e13071355 OPEN ACCESS entropy ISSN 1099-4300 www.mdpi.com/journal/entropy Article Effective Conformal Descriptions of Black Hole Entropy Steven Carlip Department of Physics, University of California at Davis, Davis, CA 95616, USA; E-Mail: [email protected]. Received: 1 July 2011; in revised form: 12 July 2011 / Accepted: 19 July 2011 / Published: 20 July 2011 Abstract: It is no longer considered surprising that black holes have temperatures and entropies. What remains surprising, though, is the universality of these thermodynamic properties: their exceptionally simple and general form, and the fact that they can be derived from many very different descriptions of the underlying microscopic degrees of freedom. I review the proposal that this universality arises from an approximate conformal symmetry, which permits an effective “conformal dual” description that is largely independent of the microscopic details. Keywords: black holes; Bekenstein–Hawking entropy; conformal dual 1. Introduction Since the seminal work of Bekenstein [1] and Hawking [2], we have understood that black holes behave as thermodynamic systems, with characteristic temperatures and entropies. A central task for quantum gravity is finding a statistical mechanical description of this behavior in terms of microscopic states. One important clue may come from the surprising “universality” of these thermodynamic properties, which manifests itself in two ways: – The Bekenstein–Hawking entropy A S = (1) 4G takes the same simple form for all black holes, independent of the charges, spin, and even the number of spacetime dimensions. If the action differs from that of general relativity, the entropy is modified, but again in a simple and universal way [3]. -
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..................... -
Qcd-Instantons and Conformal Inversion Symmetry
QCD-INSTANTONS AND CONFORMAL INVERSION SYMMETRY Diplomarbeit zur Erlangung des akademischen Grades Magistra der Naturwissenschaften durchgefuhrt¨ unter der Betreuung von Dr. Fridger Schrempp am Deutschen Elektronen Synchrotron, Hamburg eingereicht von Daniela Klammer an der Fakult¨at fur¨ Physik der Universit¨at Wien April 2006 2 2 1 Abstract Instantons are an essential and non-perturbative part of Quantum Chromodynamics, the theory of strong interactions. One of the most relevant quantities in the instanton calculus is the instanton-size distribution, which can be described on the one hand within the framework of instanton perturbation theory and on the other hand investigated numerically by means of lattice computations. A rapid onset of a drastic discrepancy between these respective results indicates that the under- lying physics is not yet well understood. In this work we investigate the appealing possibility of a symmetry under conformal inversion of space-time leading to this deviation. The motivation being that the lattice data seem to be invariant under an inversion of the instanton size. Since the instanton solution of a given size turns into an anti-instanton solution having an inverted size under conformal inversion of space-time, we ask in a first investigation, whether this property is transfered to the quantum level. In order to introduce a new scale, which is indicated by the lattice data and corresponds to the average instanton size as inversion radius, we project the instanton calculus onto the four- dimensional surface of a five-dimensional sphere via stereographic projection. The radius of this sphere is associated with the average instanton size. -
Superconformal Theories in Three Dimensions
Thesis for the degree of Master of Science Superconformal Theories in Three Dimensions Xiaoyong Chu Department of Fundamental Physics Chalmers University of Technology SE-412 96 G¨oteborg, Sweden 2009 ⃝c Xiaoyong Chu, 2009 Department of Fundamental Physics Chalmers University of Technology SE-412 96 G¨oteborg, Sweden Telephone +46 (0)31 772 1000 Typeset using LATEX Cover: Text. Printed by Chalmers Reproservice G¨oteborg, Sweden 2009 Superconformal Theories in 3 Dimensions Xiaoyong Chu Department of Fundamental Physics Chalmers University of Technology Abstract This thesis consists of six chapters, more than half of which are introductory texts. The main content of the master thesis project is presented in section 3.3, chapter 5 and chapter 6. The problem investiged in this thesis is related to three-dimensional superconformal gauge field theories. After introducing the superconformal Lie algebras, we turn to D=3 topological supergravity with Chern-Simons terms and then develop an extended pure supergravity which possesses many interesting properties. After that, three-dimensional superconformal theories of the kind originally suggested by J.Schwarz are discussed. The explicit expressions of BLG/ABJM actions are given, as well as the novel three-algebras. Finally, we couple N = 6 topological supergravity to the ABJM matter action, follow- ing standard techniques. Even though we haven't yet finished the verification of SUSY invariance, some arguments are given to explain why this action should be the complete Lagrangian. The thesis also contains some discussions on Chern-Simons terms and the U(1) gauge field. Key words: Superconformal symmetry, supergravities in 3 dimensions, string theory, M-theory, Branes, Chern-Simons terms.