D-Brane Actions and N = 2 Supergravity Solutions
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On the Holographic S–Matrix
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by CERN Document Server On the Holographic S{matrix I.Ya.Aref’eva Steklov Mathematical Institute, Russian Academy of Sciences Gubkin St.8, GSP-1, 117966, Moscow, Russia Centro Vito Volterra, Universita di Roma Tor Vergata, Italy [email protected] Abstract The recent proposal by Polchinski and Susskind for the holographic flat space S– matrix is discussed. By using Feynman diagrams we argue that in principle all the information about the S–matrix in the interacting field theory in the bulk of the anti- de Sitter space is encoded into the data on the timelike boundary. The problem of locality of interpolating field is discussed and it is suggested that the interpolating field lives in a quantum Boltzmannian Hilbert space. 1 According to the holographic principle [1, 2] one should describe a field theory on a manifold M which includes gravity by a theory which lives on the boundary of M.Two prominent examples of the holography are the Matrix theory [3] and the AdS/CFT corre- spondence [4, 5, 6]. The relation between quantum gravity in the anti-de Sitter space and the gauge theory on the boundary could be useful for better understanding of both theories. In principle CFT might teach us about quantum gravity in the bulk of AdS. Correlation functions in the Euclidean formulation are the subject of intensive study (see for example [7]-[21]). The AdS/CFT correspondence in the Lorentz formulation is considered in [22]-[29]. -
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. -
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. -
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. -
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. -
String Theory University of Cambridge Part III Mathematical Tripos
Preprint typeset in JHEP style - HYPER VERSION January 2009 String Theory University of Cambridge Part III Mathematical Tripos Dr David Tong Department of Applied Mathematics and Theoretical Physics, Centre for Mathematical Sciences, Wilberforce Road, Cambridge, CB3 OWA, UK http://www.damtp.cam.ac.uk/user/tong/string.html [email protected] –1– Recommended Books and Resources J. Polchinski, String Theory • This two volume work is the standard introduction to the subject. Our lectures will more or less follow the path laid down in volume one covering the bosonic string. The book contains explanations and descriptions of many details that have been deliberately (and, I suspect, at times inadvertently) swept under a very large rug in these lectures. Volume two covers the superstring. M. Green, J. Schwarz and E. Witten, Superstring Theory • Another two volume set. It is now over 20 years old and takes a slightly old-fashioned route through the subject, with no explicit mention of conformal field theory. How- ever, it does contain much good material and the explanations are uniformly excellent. Volume one is most relevant for these lectures. B. Zwiebach, A First Course in String Theory • This book grew out of a course given to undergraduates who had no previous exposure to general relativity or quantum field theory. It has wonderful pedagogical discussions of the basics of lightcone quantization. More surprisingly, it also has some very clear descriptions of several advanced topics, even though it misses out all the bits in between. P. Di Francesco, P. Mathieu and D. S´en´echal, Conformal Field Theory • This big yellow book is a↵ectionately known as the yellow pages. -
M-Theory Solutions and Intersecting D-Brane Systems
M-Theory Solutions and Intersecting D-Brane Systems A Thesis Submitted to the College of Graduate Studies and Research in Partial Fulfillment of the Requirements for the degree of Doctor of Philosophy in the Department of Physics and Engineering Physics University of Saskatchewan Saskatoon By Rahim Oraji ©Rahim Oraji, December/2011. All rights reserved. Permission to Use In presenting this thesis in partial fulfilment of the requirements for a Postgrad- uate degree from the University of Saskatchewan, I agree that the Libraries of this University may make it freely available for inspection. I further agree that permission for copying of this thesis in any manner, in whole or in part, for scholarly purposes may be granted by the professor or professors who supervised my thesis work or, in their absence, by the Head of the Department or the Dean of the College in which my thesis work was done. It is understood that any copying or publication or use of this thesis or parts thereof for financial gain shall not be allowed without my written permission. It is also understood that due recognition shall be given to me and to the University of Saskatchewan in any scholarly use which may be made of any material in my thesis. Requests for permission to copy or to make other use of material in this thesis in whole or part should be addressed to: Head of the Department of Physics and Engineering Physics 116 Science Place University of Saskatchewan Saskatoon, Saskatchewan Canada S7N 5E2 i Abstract It is believed that fundamental M-theory in the low-energy limit can be described effectively by D=11 supergravity. -
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. -
A Note on Six-Dimensional Gauge Theories
ILL-(TH)-97-09 hep-th/9712168 A Note on Six-Dimensional Gauge Theories Robert G. Leigh∗† and Moshe Rozali‡ Department of Physics University of Illinois at Urbana-Champaign Urbana, IL 61801 July 9, 2018 Abstract We study the new “gauge” theories in 5+1 dimensions, and their non- commutative generalizations. We argue that the θ-term and the non-commutative torus parameters appear on an equal footing in the non-critical string theories which define the gauge theories. The use of these theories as a Matrix descrip- tion of M-theory on T 5, as well as a closely related realization as 5-branes in type IIB string theory, proves useful in studying some of their properties. arXiv:hep-th/9712168v2 14 Apr 1998 ∗U.S. Department of Energy Outstanding Junior Investigator †e-mail: [email protected] ‡e-mail: [email protected] 0 1 Introduction Matrix theory[1] is an attempt at a non-perturbative formulation of M-theory in the lightcone frame. Compactifying it on a torus T d has been shown to be related to the large N limit of Super-Yang-Mills (SYM) theory in d + 1 dimensions[2]. This description is necessarily only partial for d > 3, since the SYM theory is then not renormalizable. The SYM theory is defined, for d = 4 by the (2,0) superconformal field theory in 5+1 dimensions [3, 4], and for d = 5 by a non-critical string theory in 5+1 dimensions [4, 5]. The situation of compactifications to lower dimensions is unclear for now (for recent reviews see [7, 8]). -
Random Matrix Theory in Physics
RANDOM MATRIX THEORY IN PHYSICS π π Thomas Guhr, Lunds Universitet, Lund, Sweden p(W)(s) = s exp s2 : (2) 2 − 4 As shown in Figure 2, the Wigner surmise excludes de- Introduction generacies, p(W)(0) = 0, the levels repel each other. This is only possible if they are correlated. Thus, the Poisson We wish to study energy correlations of quantum spec- law and the Wigner surmise reflect the absence or the tra. Suppose the spectrum of a quantum system has presence of energy correlations, respectively. been measured or calculated. All levels in the total spec- trum having the same quantum numbers form one par- ticular subspectrum. Its energy levels are at positions 1.0 xn; n = 1; 2; : : : ; N, say. We assume that N, the num- ber of levels in this subspectrum, is large. With a proper ) s smoothing procedure, we obtain the level density R1(x), ( 0.5 i.e. the probability density of finding a level at the energy p x. As indicated in the top part of Figure 1, the level density R1(x) increases with x for most physics systems. 0.0 In the present context, however, we are not so interested 0 1 2 3 in the level density. We want to measure the spectral cor- s relations independently of it. Hence, we have to remove FIG. 2. Wigner surmise (solid) and Poisson law (dashed). the level density from the subspectrum. This is referred to as unfolding. We introduce a new dimensionless en- Now, the question arises: If these correlation patterns ergy scale ξ such that dξ = R (x)dx. -
Refined Topological Branes Arxiv:1805.00993V1 [Hep-Th] 2 May 2018
ITEP-TH-08/18 IITP-TH-06/18 Refined Topological Branes Can Koz¸caza;b;c;1 Shamil Shakirovd;e;f;2 Cumrun Vafac and Wenbin Yang;b;c;3 aDepartment of Physics, Bo˘gazi¸ciUniversity 34342 Bebek, Istanbul, Turkey bCenter of Mathematical Sciences and Applications, Harvard University 20 Garden Street, Cambridge, MA 02138, USA cJefferson Physical Laboratory, Harvard University 17 Oxford Street, Cambridge, MA 02138, USA dSociety of Fellows, Harvard University Cambridge, MA 02138, USA eInstitute for Information Transmission Problems, Moscow 127994, Russia f Mathematical Sciences Research Institute, Berkeley, CA 94720, USA gYau Mathematical Sciences Center, Tsinghua University, Haidian district, Beijing, China, 100084 Abstract: We study the open refined topological string amplitudes using the refined topological vertex. We determine the refinement of holonomies necessary to describe the boundary conditions of open amplitudes (which in particular satisfy the required integrality properties). We also derive the refined holonomies using the refined Chern- Simons theory. arXiv:1805.00993v1 [hep-th] 2 May 2018 1Current affiliation Bo˘gazi¸ciUniversity 2Current affiliation Mathematical Sciences Research Institute 3Current affiliation Yau Mathematical Sciences Center Contents 1 Introduction1 2 Topological Branes3 2.1 External topological branes5 2.2 Internal topological branes7 2.2.1 Topological t-branes8 2.2.2 Topological q-branes 10 3 Topological Branes from refined Chern-Simons Theory 11 3.1 Topological t-branes from refined Chern-Simons theory 13 3.2 Topological q-branes from refined Chern-Simons theory 15 3.3 Duality relation and brane changing operator 15 4 Application: Double compactified toric Calabi-Yau 3-fold 17 4.1 Generic case 19 4.2 Case Qτ = 0 20 4.3 Case Qρ = 0 21 5 Discussion and Outlook 22 A Appenix A: Useful Identities 23 1 Introduction Gauge theories with N = 2 supersymmetry in 4d have been important playground for theoretical physics since the celebrated solution of Seiberg and Witten [1,2]. -
Classical String Theory
PROSEMINAR IN THEORETICAL PHYSICS Classical String Theory ETH ZÜRICH APRIL 28, 2013 written by: DAVID REUTTER Tutor: DR.KEWANG JIN Abstract The following report is based on my talk about classical string theory given at April 15, 2013 in the course of the proseminar ’conformal field theory and string theory’. In this report a short historical and theoretical introduction to string theory is given. This is fol- lowed by a discussion of the point particle action, leading to the postulation of the Nambu-Goto and Polyakov action for the classical bosonic string. The equations of motion from these actions are derived, simplified and generally solved. Subsequently the Virasoro modes appearing in the solution are discussed and their algebra under the Poisson bracket is examined. 1 Contents 1 Introduction 3 2 The Relativistic String4 2.1 The Action of a Classical Point Particle..........................4 2.2 The General p-Brane Action................................6 2.3 The Nambu Goto Action..................................7 2.4 The Polyakov Action....................................9 2.5 Symmetries of the Action.................................. 11 3 Wave Equation and Solutions 13 3.1 Conformal Gauge...................................... 13 3.2 Equations of Motion and Boundary Terms......................... 14 3.3 Light Cone Coordinates................................... 15 3.4 General Solution and Oscillator Expansion......................... 16 3.5 The Virasoro Constraints.................................. 19 3.6 The Witt Algebra in Classical String Theory........................ 22 2 1 Introduction In 1969 the physicists Yoichiro Nambu, Holger Bech Nielsen and Leonard Susskind proposed a model for the strong interaction between quarks, in which the quarks were connected by one-dimensional strings holding them together. However, this model - known as string theory - did not really succeded in de- scribing the interaction.