N= 1 Theories, T-Duality, and Ads/CFT Correspondence
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S-Duality, the 4D Superconformal Index and 2D Topological QFT
Review of superconformal index = 2 : A generalized quivers = 2: A generalized quivers = 4 index = 1 N 1 N 2 N N S-duality, the 4d Superconformal Index and 2d Topological QFT Leonardo Rastelli with A. Gadde, E. Pomoni, S. Razamat and W. Yan arXiv:0910.2225,arXiv:1003.4244, and in progress Yang Institute for Theoretical Physics, Stony Brook Rutgers, November 9 2010 Review of superconformal index = 2 : A generalized quivers = 2: A generalized quivers = 4 index = 1 N 1 N 2 N N A new paradigm for 4d =2 susy gauge theories N (Gaiotto, . ) Compactification of the (2, 0) 6d theory on a 2d surface Σ, with punctures. = =2 superconformal⇒ theories in four dimensions. N Review of superconformal index = 2 : A generalized quivers = 2: A generalized quivers = 4 index = 1 N 1 N 2 N N A new paradigm for 4d =2 susy gauge theories N (Gaiotto, . ) Compactification of the (2, 0) 6d theory on a 2d surface Σ, with punctures. = =2 superconformal⇒ theories in four dimensions. N Space of complex structures Σ = parameter space of the 4d • theory. Moore-Seiberg groupoid of Σ = (generalized) 4d S-duality • Vast generalization of “ =4 S-duality as modular group of T 2”. N Review of superconformal index = 2 : A generalized quivers = 2: A generalized quivers = 4 index = 1 N 1 N 2 N N A new paradigm for 4d =2 susy gauge theories N (Gaiotto, . ) Compactification of the (2, 0) 6d theory on a 2d surface Σ, with punctures. = =2 superconformal⇒ theories in four dimensions. N Space of complex structures Σ = parameter space of the 4d • theory. -
Non-Holomorphic Cycles and Non-BPS Black Branes Arxiv
Non-Holomorphic Cycles and Non-BPS Black Branes Cody Long,1;2 Artan Sheshmani,2;3;4 Cumrun Vafa,1 and Shing-Tung Yau2;5 1Jefferson Physical Laboratory, Harvard University Cambridge, MA 02138, USA 2Center for Mathematical Sciences and Applications, Harvard University Cambridge, MA 02139, USA 3Institut for Matematik, Aarhus Universitet 8000 Aarhus C, Denmark 4 National Research University Higher School of Economics, Russian Federation, Laboratory of Mirror Symmetry, Moscow, Russia, 119048 5Department of Mathematics, Harvard University Cambridge, MA 02138, USA We study extremal non-BPS black holes and strings arising in M-theory compactifica- tions on Calabi-Yau threefolds, obtained by wrapping M2 branes on non-holomorphic 2-cycles and M5 branes on non-holomorphic 4-cycles. Using the attractor mechanism we compute the black hole mass and black string tension, leading to a conjectural for- mula for the asymptotic volumes of connected, locally volume-minimizing representa- tives of non-holomorphic, even-dimensional homology classes in the threefold, without arXiv:2104.06420v1 [hep-th] 13 Apr 2021 knowledge of an explicit metric. In the case of divisors we find examples where the vol- ume of the representative corresponding to the black string is less than the volume of the minimal piecewise-holomorphic representative, predicting recombination for those homology classes and leading to stable, non-BPS strings. We also compute the central charges of non-BPS strings in F-theory via a near-horizon AdS3 limit in 6d which, upon compactification on a circle, account for the asymptotic entropy of extremal non- supersymmetric 5d black holes (i.e., the asymptotic count of non-holomorphic minimal 2-cycles). -
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. -
Black Brane Evaporation Through D-Brane Bubble Nucleation
HIP-2021-20/TH Black brane evaporation through D-brane bubble nucleation Oscar Henriksson∗ Department of Physics and Helsinki Institute of Physics P.O. Box 64, FI-00014 University of Helsinki, Finland Abstract We study the process of black brane evaporation through the emission of D-branes. Gravi- tational solutions describing black branes in asymptotically anti-de Sitter spacetimes, which are holographically dual to field theory states at finite temperature and density, have previously been found to exhibit an instability due to brane nucleation. Working in the setting of D3-branes on the conifold, we construct static Euclidean solutions describing this nucleation to leading order | D3-branes bubbling off the horizon. Furthermore, we analyze the late-time dynamics of such a D3-brane bubble as it expands and find a steady-state solution including the wall profile and its speed. CONTENTS I. Introduction 2 II. Gravity solutions and field theory dual 3 III. The D3-brane effective action 4 IV. Bubble nucleation 6 arXiv:2106.13254v1 [hep-th] 24 Jun 2021 V. Late time expansion 8 VI. Discussion 11 Acknowledgments 12 References 12 ∗ oscar.henriksson@helsinki.fi 1 I. INTRODUCTION Black holes are unstable to evaporation due to Hawking radiation. Though this fact is on firm theoretical footing, there are still many open questions regarding the precise details of this evaporation, some of which may require a complete theory of quantum gravity to settle. String theory is a strong candidate for such a theory. Besides strings, this framework also introduces other extended objects known as branes. These dynamical objects also gravitate, and a large number of them can be described in the supergravity limit of string theory as a black brane. -
Lectures on N = 2 String Theory
See discussions, stats, and author profiles for this publication at: https://www.researchgate.net/publication/266390735 Lectures on N = 2 String Theory Article · June 1989 CITATIONS READS 29 236 1 author: Doron Gepner Weizmann Institute of Science 69 PUBLICATIONS 3,252 CITATIONS SEE PROFILE All content following this page was uploaded by Doron Gepner on 04 October 2014. The user has requested enhancement of the downloaded file. April, 1989 PUPT-1121 Lectures on N = 2 String Theoryz Doron Gepner Joseph Henry Laboratories Princeton University Princeton, New Jersey 08544 ABSTRACT Starting from an arbitrary N = 2 superconformal field theory it is described how a fully consistent, space{time supersymmetric heterotic{like string theory in an even number of dimensions is constructed. Four dimensional theories which arise in this construction have a gauge group which contains E8 × E6 with chiral fermions in the 27 and 27¯ representations of E6, and thus are phenomenologically viable. The explicit massless spectrum is studied for particular solvable examples. It is shown that such spectra are the typical ones expected from the field theory compactification on manifolds of vanishing first Chern class. It is concluded that all `N=2 string theories' describe string propagation on such manifolds. An explicit calculation of the Yukawa couplings 273 is described for all the string theories in which the N = 2 superconformal theory affords a scalar description. The result of this calculation is shown to be geometric. z Lectures given at the Spring School on Superstrings, Trieste, Italy, 3-11 April, 1989. To appear in the proceedings. .1. Introduction The study of four dimensional string theory is central to the idea that strings might provide a framework for unification. -
Intertwining Operator Superalgebras and Vertex Tensor Categories for Superconformal Algebras, Ii
TRANSACTIONS OF THE AMERICAN MATHEMATICAL SOCIETY Volume 354, Number 1, Pages 363{385 S 0002-9947(01)02869-0 Article electronically published on August 21, 2001 INTERTWINING OPERATOR SUPERALGEBRAS AND VERTEX TENSOR CATEGORIES FOR SUPERCONFORMAL ALGEBRAS, II YI-ZHI HUANG AND ANTUN MILAS Abstract. We construct the intertwining operator superalgebras and vertex tensor categories for the N = 2 superconformal unitary minimal models and other related models. 0. Introduction It has been known that the N = 2 Neveu-Schwarz superalgebra is one of the most important algebraic objects realized in superstring theory. The N =2su- perconformal field theories constructed from its discrete unitary representations of central charge c<3 are among the so-called \minimal models." In the physics liter- ature, there have been many conjectural connections among Calabi-Yau manifolds, Landau-Ginzburg models and these N = 2 unitary minimal models. In fact, the physical construction of mirror manifolds [GP] used the conjectured relations [Ge1] [Ge2] between certain particular Calabi-Yau manifolds and certain N =2super- conformal field theories (Gepner models) constructed from unitary minimal models (see [Gr] for a survey). To establish these conjectures as mathematical theorems, it is necessary to construct the N = 2 unitary minimal models mathematically and to study their structures in detail. In the present paper, we apply the theory of intertwining operator algebras developed by the first author in [H3], [H5] and [H6] and the tensor product theory for modules for a vertex operator algebra developed by Lepowsky and the first author in [HL1]{[HL6], [HL8] and [H1] to construct the intertwining operator algebras and vertex tensor categories for N = 2 superconformal unitary minimal models. -
Chaos in Matrix Models and Black Hole Evaporation
LLNL-JRNL-681857 UCB-PTH-16/01 SU-ITP-16/02 YITP-16-5 Chaos in Matrix Models and Black Hole Evaporation Evan Berkowitz,a1 Masanori Hanadabcd2 and Jonathan Maltzeb3 a Nuclear and Chemical Sciences Division, Lawrence Livermore National Laboratory, Livermore CA 94550, USA bStanford Institute for Theoretical Physics, Stanford University, Stanford, CA 94305, USA cYukawa Institute for Theoretical Physics, Kyoto University, Kitashirakawa Oiwakecho, Sakyo-ku, Kyoto 606-8502, Japan dThe Hakubi Center for Advanced Research, Kyoto University, Yoshida Ushinomiyacho, Sakyo-ku, Kyoto 606-8501, Japan e Berkeley Center for Theoretical Physics, University of California at Berkeley, Berkeley, CA 94720, USA Abstract Is the evaporation of a black hole described by a unitary theory? In order to shed light on this question |especially aspects of this question such as a black hole's negative specific heat|we consider the real-time dynamics of a solitonic object in matrix quantum mechanics, which can be interpreted as a black hole (black zero-brane) via holography. We point out that the chaotic nature of the system combined with the flat directions of its potential naturally leads to the emission of D0-branes from the black brane, which is suppressed in the large N limit. Simple arguments show that the black zero-brane, like the Schwarzschild black hole, arXiv:1602.01473v3 [hep-th] 15 Jan 2019 has negative specific heat, in the sense that the temperature goes up when it evaporates by emitting D0-branes. While the largest Lyapunov exponent grows during the evaporation, the Kolmogorov-Sinai entropy decreases. These are consequences of the generic properties of matrix models and gauge theory. -
What Lattice Theorists Can Do for Superstring/M-Theory
July 26, 2016 0:28 WSPC/INSTRUCTION FILE review˙2016July23 International Journal of Modern Physics A c World Scientific Publishing Company What lattice theorists can do for superstring/M-theory MASANORI HANADA Yukawa Institute for Theoretical Physics Kyoto University, Kyoto 606-8502, JAPAN The Hakubi Center for Advanced Research Kyoto University, Kyoto 606-8501, JAPAN Stanford Institute for Theoretical Physics Stanford University, Stanford, CA 94305, USA [email protected] The gauge/gravity duality provides us with nonperturbative formulation of superstring/M-theory. Although inputs from gauge theory side are crucial for answering many deep questions associated with quantum gravitational aspects of superstring/M- theory, many of the important problems have evaded analytic approaches. For them, lattice gauge theory is the only hope at this moment. In this review I give a list of such problems, putting emphasis on problems within reach in a five-year span, including both Euclidean and real-time simulations. Keywords: Lattice Gauge Theory; Gauge/Gravity Duality; Quantum Gravity. PACS numbers:11.15.Ha,11.25.Tq,11.25.Yb,11.30.Pb Preprint number:YITP-16-28 1. Introduction During the second superstring revolution, string theorists built a beautiful arXiv:1604.05421v2 [hep-lat] 23 Jul 2016 framework for quantum gravity: the gauge/gravity duality.1, 2 It claims that superstring/M-theory is equivalent to certain gauge theories, at least about certain background spacetimes (e.g. black brane background, asymptotically anti de-Sitter (AdS) spacetime). Here the word ‘equivalence’ would be a little bit misleading, be- cause it is not clear how to define string/M-theory nonperturbatively; superstring theory has been formulated based on perturbative expansions, and M-theory3 is defined as the strong coupling limit of type IIA superstring theory, where the non- perturbative effects should play important roles. -
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. -
VISCOSITY and BLACK HOLES 1 Introduction the Discovery Of
VISCOSITY AND BLACK HOLES D.T. SON Institute for Nuclear Theory, University of Washington, Seattle, WA 98195-1550, USA We review recent applications of the AdS/CFT correspondence in strongly coupled systems, in particular the quark gluon plasma. 1 Introduction The discovery of Hawking radiation1 confirmed that black holes are endowed with thermody- namic properties such as entropy and temperature, as first suggested by Bekenstein2 based on the analogy between black hole physics and equilibrium thermodynamics. For black branes, i.e., black holes with translationally invariant horizons, thermodynamics can be extended to hydrodynamics|the theory that describes long-wavelength deviations from thermal equilibrium. Thus, black branes possess hydrodynamic properties of continuous fluids and can be character- ized by kinetic coefficients such as viscosity, diffusion constants, etc. From the perspective of the holographic principle3;4, the hydrodynamic behavior of a black-brane horizon is identified with the hydrodynamic behavior of the dual theory. In this talk, we argue that in theories with gravity duals, the ratio of the shear viscosity to the volume density of entropy is equal to a universal value of ~=4π. A lot of attention has been given to this fact due to the discovery of a perfect liquid behavior at RHIC. We will also review recent attempts to extend AdS/CFT correspondence to nonrelativistic systems. 2 Dimension of η=s The standard textbook definition of the shear viscosity is as follows. Take two large parallel plates separated by a distance d. The space between the two plates is filled with a fluid. Let one plate moves relative to the other with a velocity v. -
LIE SUPERALGEBRAS of STRING THEORIES Introduction I.1. The
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by CERN Document Server LIE SUPERALGEBRAS OF STRING THEORIES PAVEL GROZMAN1, DIMITRY LEITES1 AND IRINA SHCHEPOCHKINA2 Abstract. We describe simple complex Lie superalgbras of vector fields on “supercircles” — stringy su- peralgebras. There are four series of such algebras (one depends on a complex parameter as well as on an integer one) and four exceptional stringy superalgebras. Two of the exceptional algebras are new in the literature. The 13 of the simple stringy Lie superalgebras are distinguished: only they have nontrivial central extensions and since two of the distinguish algebras have 3 nontrivial central extensions each, there are exactly 16 superizations of the Liouville action, Schr¨odinger equation, KdV hierarchy, etc. We also present the three nontrivial cocycles on the N = 4 extended Neveu–Schwarz and Ramond superalgebras in terms of primary fields. We also describe the classical stringy superalgebras, close to the simple ones. One of these stringy superalgebras is a Kac–Moody superalgebra g(A) with a nonsymmetrizable Cartan matrix A. Unlike the Kac–Moody superalgebras of polynomial growth with symmetrizable Cartan matrix, it can not be interpreted as a central extension of a twisted loop algebra. In the litterature the stringy superalgebras are often referred to as superconformal ones. We discuss how superconformal stringy superalgebras really are. Introduction I.1. The discovery of stringy Lie superalgebras. The discovery of stringy superalgebras was not a one- time job and their further study was not smooth either. Even the original name of these Lie superalgebras is unfortunate. -
The First Law of Black Brane Mechanics
DAMTP-2001-67 hep-th/0107228 THE FIRST LAW OF BLACK BRANE MECHANICS Paul K. Townsend and Marija Zamaklar DAMTP, University of Cambridge, Centre for Mathematical Sciences, Wilberforce Road, Cambridge CB3 0WA, UK ABSTRACT We obtain ADM and Komar surface integrals for the energy density, tension and angular momentum density of stationary p-brane solutions of Einstein’s equations. We use them to derive a Smarr-type formula for the energy den- sity and thence a first law of black brane mechanics. The intensive variable conjugate to the worldspace p-volume is an ‘effective’ tension that equals the ADM tension for uncharged branes, but vanishes for isotropic boost-invariant charged branes. 1 Introduction The status of energy in General Relativity is rather special because, for a general space- time, there is no coordinate-independent meaning to the energy in a given local region of a spacelike hypersurface. However, if the spacetime is asymptotically flat then it is possible to define a total energy, which can be expressed as an integral at spatial infinity: the ADM integral [1]. Consider an asymptotically flat spacetime, of d =1+n dimensions, for which the asymptotic form of the metric, in cartesian coordinates xM =(t; xi)(i =1;:::;n)is g η + h (1) MN ∼ MN MN where η is the Minkowski metric and h is a perturbation with the appropriate fall-off at spatial infinity needed to make the energy integral converge. We shall suppose that the action takes the form1 1 I = ddx det gR + I(mat) : (2) 2 Z p− The matter stress-tensor is 2 δI(mat) T (mat) = ; (3) MN −√ det g δgMN − and the Einstein field equation is (mat) GMN = TMN : (4) The ADM energy integral in these conventions is 1 E = dSi (@jhij @ihjj) : (5) 2 I − ∞ In the special case of a stationary asymptotically flat spacetime, for which there exists a normalized timelike Killing vector field k, the energy in any volume V with boundary @V can be expressed as the Komar integral [2] n 1 M N E(V )= − dSMND k : (6) − 4(n 2) Z − @V where dSMN is the co-dimension 2 surface element on the (n 1)-dimensional boundary @V of V .