Spontaneously Broken Space-Time Supersymmetry in Open String
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Off-Shell Interactions for Closed-String Tachyons
Preprint typeset in JHEP style - PAPER VERSION hep-th/0403238 KIAS-P04017 SLAC-PUB-10384 SU-ITP-04-11 TIFR-04-04 Off-Shell Interactions for Closed-String Tachyons Atish Dabholkarb,c,d, Ashik Iqubald and Joris Raeymaekersa aSchool of Physics, Korea Institute for Advanced Study, 207-43, Cheongryangri-Dong, Dongdaemun-Gu, Seoul 130-722, Korea bStanford Linear Accelerator Center, Stanford University, Stanford, CA 94025, USA cInstitute for Theoretical Physics, Department of Physics, Stanford University, Stanford, CA 94305, USA dDepartment of Theoretical Physics, Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai 400005, India E-mail:[email protected], [email protected], [email protected] Abstract: Off-shell interactions for localized closed-string tachyons in C/ZN super- string backgrounds are analyzed and a conjecture for the effective height of the tachyon potential is elaborated. At large N, some of the relevant tachyons are nearly massless and their interactions can be deduced from the S-matrix. The cubic interactions be- tween these tachyons and the massless fields are computed in a closed form using orbifold CFT techniques. The cubic interaction between nearly-massless tachyons with different charges is shown to vanish and thus condensation of one tachyon does not source the others. It is shown that to leading order in N, the quartic contact in- teraction vanishes and the massless exchanges completely account for the four point scattering amplitude. This indicates that it is necessary to go beyond quartic inter- actions or to include other fields to test the conjecture for the height of the tachyon potential. Keywords: closed-string tachyons, orbifolds. -
H ( Ff^L°9 . INTERNATIONAL CENTRE for \ | THEORETICAL PHYSICS
IC/87/420 H ( ff^l°9 . INTERNATIONAL CENTRE FOR I 'V. ': \| THEORETICAL PHYSICS HARMONIC SUPERSTRING AND COVARIANT QUANTIZATION OF THE GREEN-SCHWARZ SUPERSTRING E. Nissimov S. Pacheva and INTERNATIONAL ATOMIC ENERGY S. Solomon AGENCY UNITED NATIONS EDUCATIONAL, SCIENTIFIC AND CULTURAL ORGANIZATION T T IC/87/420 ABSTRACT International Atomic Energy Agency Based on our recent work, we describe a new generalized model of space- and United Nations Educational Scientific and Cultural Organization time supersymmetric strings - the harmonic superstring. It has the same phys- ical content as the original Green-Schwarz (GS) superstring but it is defined on INTERNATIONAL CENTRE FOR THEORETICAL PHYSICS an enlarged superspace: the D=10 harmonic superspace and incorporates addi- tional fennionic string coordinates. The main feature of the harmonic superstring model is that it contains covariant and irreducible first-class constraints only. This allows for a straight- HARMONIC SUPERSTRING AND COVARIANT QUANTIZATION forward manifestly super-Poincaie'covariant Batalin-Fradkin-Vilkoviski (BFV) OF THE GREEN-SCHWARZ SUPERSTRING * - Becchi-Rouet-Stora-Tyutin (BRST) quantization. The BRST charge has a re- markably simple form and the corresponding BFV hamiltonian exhibits manifest Parisi-Sourlas O5p(l,l|2) symmetry. E. Nissinsov ** In a particular Lorentz-covariant gauge we find the covariant vertex opera- International Centre for Theoretical Physics, Trieste, Italy, tors for the emission of the massless states which closely resemble the covariant "classical" expressions previously guessed by Green and Schwarz. S. Pacheva Institute of Nuclear Research and Nuclear Energy, Boul. Lenin 72, 1784 Sofia, Bulgaria and S. Solomon Physics Department, Weizmann Institute, Hehovot 76100, Israel. MIRAMARE - TRIESTE December 1987 •' To appear in "Perspectives In String Theories" (Proceedings of the Copenhagen Workshop, Denmark, October 1987). -
The Quantized Fermionic String
Class 2: The quantized fermionic string Canonical quantization Light-cone quantization Spectrum of the fermionic string, GSO projection . The super-Virasoro constraints, which allow to eliminate the ghosts, are implemented and analyzed in essentially the same way as in the bosonic string. One new feature is the existence of two sectors: bosonic and fermionic, which have to be studied separately. To remove the tachyon one has to perform the so-called GSO projection, which guarantees space-time supersymmetry of the ten-dimensional theory. There are two possible space-time supersymmetric GSO projections which result in the Type IIA and Type IIB superstring. Summary The fermionic string is quantized analogously to the bosonic string, although now we'll find the critical dimension is 10 . One new feature is the existence of two sectors: bosonic and fermionic, which have to be studied separately. To remove the tachyon one has to perform the so-called GSO projection, which guarantees space-time supersymmetry of the ten-dimensional theory. There are two possible space-time supersymmetric GSO projections which result in the Type IIA and Type IIB superstring. Summary The fermionic string is quantized analogously to the bosonic string, although now we'll find the critical dimension is 10 The super-Virasoro constraints, which allow to eliminate the ghosts, are implemented and analyzed in essentially the same way as in the bosonic string. To remove the tachyon one has to perform the so-called GSO projection, which guarantees space-time supersymmetry of the ten-dimensional theory. There are two possible space-time supersymmetric GSO projections which result in the Type IIA and Type IIB superstring. -
Abdus Salam United Nations Educational, Scientific and Cultural XA9952968 Organization International Centre
the IC/99/74 abdus salam united nations educational, scientific and cultural XA9952968 organization international centre international atomic energy agency for theoretical physics D = 4 YANG-MILLS CORRELATORS 5 FROM NSR STRINGS ON AdS5 x S Dimitri Polyakov 30-47 Available at: http://www.ictp.trieste.it/~pub-off IC/99/74 United Nations Educational Scientific and Cultural Organization and International Atomic Energy Agency THE ABDUS SALAM INTERNATIONAL CENTRE FOR THEORETICAL PHYSICS D = 4 YANG-MILLS CORRELATORS 5 FROM NSR STRINGS ON AdS5 x S Dimitri Polyakov^ The Abdus Salam International Centre for Theoretical Physics, Trieste, Italy. Abstract In our previous work (hep-th/9812044) we have proposed the sigma-model action, conjectured to be the NSR analogue of superstring theory on AdS$ x S5. This sigma- model is the NSR superstring action with potential term corresponding to the exotic 5- form vertex operator (branelike state). This 5-form potential plays the role of cosmological term, effectively curving the flat space-time geometry to that of AdS$ x S5. In this paper we study this ansatz in more detail and provide the derivation of the correlators of the four- dimensional super Yang-Mills theory from the above mentioned sigma-model. In particular, we show that the correlation function of two dilaton vertex operators in such a model reproduces the well-known result for the two-point function in N = 4 four-dimensional 2 2 super Yang-Mills theory: < F (x)F (y) >~ \JLy\» • MIRAMARE - TRIESTE July 1999 E-mail: [email protected] Introduction One of the most profound questions with regard to critical superstring theory in ten dimensions is its relation to our four-dimensional world. -
Brane Effective Actions, Kappa-Symmetry and Applications
Living Rev. Relativity, 15, (2012), 3 LIVINGREVIEWS http://www.livingreviews.org/lrr-2012-3 in relativity Brane Effective Actions, Kappa-Symmetry and Applications Joan Sim´on School of Mathematics, The University of Edinburgh, and Maxwell Institute for Mathematical Sciences Edinburgh EH9 3JZ, U.K. email: [email protected] Accepted on 9 January 2012 Published on 27 February 2012 Abstract This is a review on brane effective actions, their symmetries and some of their applications. Its first part covers the Green{Schwarz formulation of single M- and D-brane effective actions focusing on kinematical aspects: the identification of their degrees of freedom, the importance of world volume diffeomorphisms and kappa symmetry to achieve manifest spacetime covari- ance and supersymmetry, and the explicit construction of such actions in arbitrary on-shell supergravity backgrounds. Its second part deals with applications. First, the use of kappa symmetry to determine supersymmetric world volume solitons. This includes their explicit construction in flat and curved backgrounds, their interpretation as Bogomol'nyi{Prasad–Sommerfield (BPS) states carrying (topological) charges in the supersymmetry algebra and the connection between su- persymmetry and Hamiltonian BPS bounds. When available, I emphasise the use of these solitons as constituents in microscopic models of black holes. Second, the use of probe approx- imations to infer about the non-trivial dynamics of strongly-coupled gauge theories using the anti de Sitter/conformal field theory (AdS/CFT) correspondence. This includes expectation values of Wilson loop operators, spectrum information and the general use of D-brane probes to approximate the dynamics of systems with small number of degrees of freedom interacting with larger systems allowing a dual gravitational description. -
Introduction to Path Integral Methods in String Theory
Introduction to path integral methods in string theory Sergio Ernesto Aguilar Guti´errez1 1Instituto de F´ısica Te´orica, Universidade Estadual Paulista, Rua Dr. Bento Teobaldo Ferraz 271, 01140-070 S~aoPaulo, SP, Brazil∗ (Dated: November 30, 2018) Contents I. Introduction 1 II. Functional methods in bosonic string theory 2 A. Polyakov action 2 B. Symmetries 3 C. Equations of motion and boundary conditions 4 D. Polyakov path integral 6 E. BRST quantization 10 F. Representation theory 11 III. Functional methods in the RNS formalism 12 A. Superstring theory in the RNS formalism 12 B. R and NS sectors 14 C. Local symmetries of the action 16 D. Path integrals in RNS 17 References 19 I. INTRODUCTION The fundamentals of path integral methods in string theory are reviewed with emphasis in the development of the Faddeev Popov ghost that emerge from overcounting of configurations and the conditions that the string theory requires for maintaining Weyl invariance. Since the lecture is presented for a course that does not assume previous knowledge in string theory, I include an introduction to both bosonic and superstring theory (in the RNS formalism). This text begins with an introduction to bosonic string theory, we study the symmetries of the Polyakov action, we work out the canonical quantization of the theory to calculate its central charge. Later the path integral formulation is introduced with the appearance of Faddeev-Popov ghosts, we consider their canonical quantization for computing the central charge. The total central charge generates an anomaly in the Weyl invariance of the theory. The vanishing of such term has powerful implications that yield conditions related with the possible physical states and the dimensions of the theory. -
Introduction to Superstring Theory
Introduction to Superstring theory Carmen Nunez Instituto de Astronomia y Física del Espacio C.C. 67 - Sue. 28, 1428 Buenos Aires, Argentina and Physics Department, University of Buenos Aires [email protected] Abstract 1 Overview The bosonic string theory, despite all its beautiful features, has a number of short comings. The most obvious of these are the absence of fermions and the presence of tachyons in spacetime. The tachyon is not an actual physical inconsistency; it indicates at least that the calculations are being performed in an unstable vacuum state. More over, tachyon exchange contributes infrarred divergences in loop diagrams and these divergences make it hard to isolate the ultraviolet behaviour of the "unified quan tum theory" the bosonic string theory gives rise to and determine whether it is really satisfactory. Historically, the solution to the tachyon problem appeared with the solution to the other problem, the absence of fermions. The addition of a new ingredient, supersym- metry on the world-sheet, improves substantially the general picture. In 1977 Gliozzi, Scherk and Olive showed that it was possible to get a model with no tachyons and with equal masses and multiplicities for bosons and fermions. In 1980, Green and Schwarz proved that this model had spacetime supersymmetry. In the completely consisten- t tachyon free form of the superstring theory it was then possible to show that the one-loop diagrams were completely finite and free of ultraviolet divergences. While most workers on the subject believe that the finiteness will also hold to all orders of perturbation theory, complete and universally accepted proofs have not appeared so far. -
Superstrings ETH Proseminar in Theoretical Physics
Neveu{Schwarz{Ramond formulation Modular invariance Green{Schwarz formulation Superstrings ETH Proseminar in Theoretical Physics ImRe Majer May 13th, 2013 ImRe Majer | Superstrings 1/42 Neveu{Schwarz{Ramond formulation Modular invariance Green{Schwarz formulation Outline 1 Neveu{Schwarz{Ramond formulation Building up the spectrum GSO projection 2 Modular invariance Spin structures Partition function 3 Green{Schwarz formulation Supersymmetry Building up the spectrum ImRe Majer | Superstrings 2/42 Neveu{Schwarz{Ramond formulation Modular invariance Green{Schwarz formulation Outline 1 Neveu{Schwarz{Ramond formulation Building up the spectrum GSO projection 2 Modular invariance Spin structures Partition function 3 Green{Schwarz formulation Supersymmetry Building up the spectrum ImRe Majer | Superstrings 3/42 Neveu{Schwarz{Ramond formulation Modular invariance Green{Schwarz formulation NSR action Light cone gauge fixing The Neveu{Schwarz{Ramond action in light cone gauge 1 Z S l:c: = − d 2σ @ X i @αX i − i ¯i ρα@ i NSR 2π α α transverse coordinates i = 1;:::; 8 i is a worldsheet Majorana 2-spinor i is a spacetime vector i SO(8) rotational symmetry =) is an 8v representation of SO(8) ImRe Majer | Superstrings 4/42 Neveu{Schwarz{Ramond formulation Modular invariance Green{Schwarz formulation Building up the spectrum Tools for generating the spectrum Open string or the right-moving part of a closed string. Creation and annihilation operators: i i i X : α−n and αn n 2 Z i i i d−m and dm m 2 Z for R-sector : i i 1 b−r and br r 2 Z + 2 for NS-sector The mass2 operator: X X 1 α0m2 = αi αi + md i d i − for NS-sector −n n −m m 2 n>0 m>0 | {z } | {z } N(α) N(d) 0 2 X i i X i i α m = α−nαn + rb−r br for R-sector n>0 r>0 | {z } | {z } N(α) N(b) ImRe Majer | Superstrings 5/42 Neveu{Schwarz{Ramond formulation Modular invariance Green{Schwarz formulation Building up the spectrum Ground states NSR formulation: All creation/annihilation operators are spacetime vectors. -
Introduction to Superstring Theory
Introduction to Superstring Theory Carmen N´u~nez IAFE (UBA-CONICET) & PHYSICS DEPT. (University of Buenos Aires) VI ICTP LASS 2015 Mexico, 26 October- 6 November 2015 . Programme Class 1: The classical fermionic string Class 2: The quantized fermionic string Class 3: Partition Function Class 4: Interactions . Outline Class 1: The classical fermionic string The action and its symmetries Gauge fixing and constraints Equations of motion and boundary conditions Oscillator expansions . The spectra of bosonic strings contain a tachyon ! it might indicate the vacuum has been incorrectly identified. The mass squared of a particle T is the quadratic term in the 2 @2V (T ) j − 4 ) action: M = @T 2 T =0 = α0 = we are expanding around a maximum of V . If there is some other stable vacuum, this is not an actual inconsistency. Why superstrings? . The mass squared of a particle T is the quadratic term in the 2 @2V (T ) j − 4 ) action: M = @T 2 T =0 = α0 = we are expanding around a maximum of V . If there is some other stable vacuum, this is not an actual inconsistency. Why superstrings? The spectra of bosonic strings contain a tachyon ! it might indicate the vacuum has been incorrectly identified. If there is some other stable vacuum, this is not an actual inconsistency. Why superstrings? The spectra of bosonic strings contain a tachyon ! it might indicate the vacuum has been incorrectly identified. The mass squared of a particle T is the quadratic term in the 2 @2V (T ) j − 4 ) action: M = @T 2 T =0 = α0 = we are expanding around a maximum of V . -
String Theory and M-Theory: a Modern Introduction Katrin Becker, Melanie Becker, and John H
Cambridge University Press 978-0-521-86069-7 - String Theory and M-Theory: A Modern Introduction Katrin Becker, Melanie Becker, and John H. Schwarz Frontmatter More information STRING THEORY AND M-THEORY A MODERN INTRODUCTION String theory is one of the most exciting and challenging areas of modern theoretical physics. This book guides the reader from the basics of string theory to very recent developments at the frontier of string theory research. The book begins with the basics of perturbative string theory, world-sheet supersymmetry, space-time supersymmetry, conformal field theory and the heterotic string, and moves on to describe modern developments, including D-branes, string dualities and M-theory. It then covers string geometry (including Calabi–Yau compactifications) and flux compactifications, and applications to cosmology and particle physics. One chapter is dedicated to black holes in string theory and M-theory, and the microscopic origin of black-hole entropy. The book concludes by presenting matrix theory, AdS/CFT duality and its generalizations. This book is ideal for graduate students studying modern string theory, and it will make an excellent textbook for a 1-year course on string theory. It will also be useful for researchers interested in learning about developments in modern string theory. The book contains about 120 solved exercises, as well as about 200 homework problems, solutions of which are available for lecturers on a pass- word protected website at www.cambridge.org/9780521860697. K ATRIN B ECKER is a Professor of physics at Texas A & M University. She was awarded the Radcliffe Fellowship from Harvard University in 2006 and received the Alfred Sloan Fellowship in 2003. -
PHYS 652: String Theory II Homework 2
PHYS 652: String Theory II Homework 2 Due 2/27/2017 (Assigned 2/15/2017) 1 Heterotic Strings Last semester, you constructed the closed bosonic string by combining left- and right-moving copies of the open bosonic string subject to the level-matching condition. In this class we repeated that construction to obtain the type-II closed superstrings from two copies of the open type-I superstring. In the RNS formalism we employed a GSO projection to remove the tachyon and computed the massless spectrum in lightcone gauge. In the GS formalism spacetime supersymmetry extends the lightcone gauge to superspace and there is no tachyon. Despite the differences between the two formulations, the massless spectra agree. The heterotic strings are closed superstrings obtained by combining the bosonic string for the left-movers with the type-I superstring for the right-movers, again subject to level-matching. Split the 26 coordinates of the critical bosonic string into 10 X's and 16 Y 's and treat the X's as the left-moving side of the spacetime coordinate with the right-moving side identified with the 10 X's of the critical type-I superstring. Using level-matching, construct the massless spectrum in both the RNS and GS formalisms and interpret it in terms of gauge and gravity multiplets. At this point, it is not possible to determine the gauge group of this theory but you can deduce the rank. If, in addition, you were told that the gauge algebra is semi-simple and its dimension is 496, what are the possibilities for the heterotic strings? Why is this string called \heterotic"? 2 Fermionization and Picture Fixing reparameterization-invariance of the bosonic string to conformal gauge requires the in- clusion of the bc ghost system. -
Superstrings
Eidgenossische¨ Technische Hochschule Zurich¨ Swiss Federal Institute of Technology Zurich Report for Proseminar in Theoretical Physics Superstrings Author: Supervisor: Imre Majer Cristian Vergu Abstract During the course of the previous chapters of the proseminar, we introduced and quantized both the bosonic and fermionic strings and determined that the theory only containing bosonic strings requires D = 26 dimensions, whereas if it contains fermionic strings as well, the critical dimension is D = 10. We have also seen that the latter is formulated such that it incorporates manifest worldsheet supersymmetry (Neveu{ Schwarz{Ramond formulation). By na¨ıvely building up the spectrum of states using the tools previously introduced, we will see that this theory in itself is inconsistent and contains several unwanted features. To fix these, a procedure called the GSO projec- tion is needed. We will first define and use it to obtain a spacetime supersymmetric spectrum which is free from the mentioned inconsistencies. Then, we will justify the seemingly arbitrary GSO conditions by requiring that the theory be modular invariant. In the final part of this report, we take a completely different approach, and formulate another theory with manifest spacetime supersymmetry (Green{Schwarz fomulation). Spacetime supersymmetry is an elegant property, and so, many constraints and restric- tions are imposed in both formulations merely for the sake of a supersymmetric result. Without rigorous proof, we will show that with these constraints, the two formulations are actually equivalent. 1 Contents 1 Neveu{Schwarz{Ramond Formulation 3 1.1 Quick Revision . .3 1.2 The Na¨ıve Spectrum . .4 1.2.1 The NS-Sector Ground State .