Confinement in Yang{Mills: Elements of a Big Picture
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M2-Branes Ending on M5-Branes
M2-branes ending on M5-branes Vasilis Niarchos Crete Center for Theoretical Physics, University of Crete 7th Crete Regional Meeting on String Theory, 27/06/2013 based on recent work with K. Siampos 1302.0854, ``The black M2-M5 ring intersection spins’‘ Proceedings Corfu Summer School, 2012 1206.2935, ``Entropy of the self-dual string soliton’’, JHEP 1207 (2012) 134 1205.1535, ``M2-M5 blackfold funnels’’, JHEP 1206 (2012) 175 and older work with R. Emparan, T. Harmark and N. A. Obers ➣ blackfold theory 1106.4428, ``Blackfolds in Supergravity and String Theory’’, JHEP 1108 (2011) 154 0912.2352, ``New Horizons for Black Holes and Branes’’, JHEP 1004 (2010) 046 0910.1601, ``Essentials of Blackfold Dynamics’’, JHEP 1003 (2010) 063 0902.0427, ``World-Volume Effective Theory for Higher-Dimensional Black Holes’’, PRL 102 (2009)191301 0708.2181, ``The Phase Structure of Higher-Dimensional Black Rings and Black Holes’‘ + M.J. Rodriguez JHEP 0710 (2007) 110 2 Important lessons about the fundamentals of string/M-theory (and QFT) are obtained by studying the low-energy theories on D-branes and M-branes. Most notably in M-theory, recent progress has clarified the low-energy QFT on N M2-brane and the N3/2 dof that it exhibits. Bagger-Lambert ’06, Gustavsson ’07, ABJM ’08 Drukker-Marino-Putrov ’10 Our understanding of the M5-brane theory is more rudimentary, but efforts to identify analogous properties, e.g. the N3 scaling of the massless dof, is underway. Douglas ’10 Lambert,Papageorgakis,Schmidt-Sommerfeld ’10 Hosomichi-Seong-Terashima ’12 Kim-Kim ’12 Kallen-Minahan-Nedelin-Zabzine ’12 .. -
Bosonization and Mirror Symmetry Arxiv:1608.05077V1 [Hep-Th]
Bosonization and Mirror Symmetry Shamit Kachru1, Michael Mulligan2,1, Gonzalo Torroba3, and Huajia Wang4 1Stanford Institute for Theoretical Physics, Stanford University, Stanford, CA 94305, USA 2Department of Physics and Astronomy, University of California, Riverside, CA 92511, USA 3Centro At´omico Bariloche and CONICET, R8402AGP Bariloche, ARG 4Department of Physics, University of Illinois, Urbana-Champaign, IL 61801, USA Abstract We study bosonization in 2+1 dimensions using mirror symmetry, a duality that relates pairs of supersymmetric theories. Upon breaking supersymmetry in a controlled way, we dynamically obtain the bosonization duality that equates the theory of a free Dirac fermion to QED3 with a single scalar boson. This duality may be used to demonstrate the bosonization duality relating an O(2)-symmetric Wilson-Fisher fixed point to QED3 with a single Dirac fermion, Peskin-Dasgupta-Halperin duality, and the recently conjectured duality relating the theory of a free Dirac fermion to fermionic QED3 with a single flavor. Chern-Simons and BF couplings for both dynamical and background gauge fields play a central role in our approach. In the course of our study, we describe a \chiral" mirror pair that may be viewed as the minimal supersymmetric generalization of the two bosonization dualities. arXiv:1608.05077v1 [hep-th] 17 Aug 2016 Contents 1 Introduction 1 2 Mirror symmetry and its deformations 4 2.1 Superfields and lagrangians . .5 2.2 = 4 mirror symmetry . .7 N 2.3 Deformations by U(1)A and U(1)R backgrounds . 10 2.4 General mirror duality . 11 3 Chiral mirror symmetry 12 3.1 Chiral theory A . -
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. -
Arxiv:2002.11085V1 [Hep-Th]
On-Shell Electric-Magnetic Duality and the Dual Graviton 1,2 2 Nathan Moynihan and Jeff Murugan ∗ 1High Energy Physics, Cosmology & Astrophysics Theory group, 2The Laboratory for Quantum Gravity & Strings Department of Mathematics and Applied Mathematics, University of Cape Town, Rondebosch, Cape Town 7700, South Africa Using on-shell amplitude methods, we explore 4-dimensional Electric-Magnetic duality and its double copy. We show explicitly that the on-shell scattering amplitudes know about ‘dual’ photons (and dual gravitons), that the off-shell photon propagator double copies to the graviton propagator and that the magnetic part of the propagator is essential for the double copy to hold. We also show that there is an equivalent gravito-magnetic part of the graviton propagator which is essential in giving rise to solutions with either angular momentum or NUT charge. Furthermore, we comment on the so-called Weinberg paradox, which states that scattering amplitudes involving the mixing of electric and magnetic monopoles cannot be Lorentz invariant, and would seem to preclude the existence of the ’t Hooft-Polyakov (topological) monopole. We trace this paradox to the magnetic part of the propagator, showing that it can be eliminated if one restricts to proper orthochronous Lorentz transformations. Finally, we compute the fully relativistic cross-section for arbitrary spin dyons using the recently formulated on-shell duality transformation and show that this is always fully Lorentz invariant. INTRODUCTION field theory without a Dirac string singularity necessitates the introduction of a second four-vector potential: the The boostrap program of the 1960’s received considerable dual photon [3–6]. -
The Fuzzball Proposal for Black Holes: an Elementary Review
hep-th/0502050 The fuzzball proposal for black holes: an elementary review1 Samir D. Mathur Department of Physics, The Ohio State University, Columbus, OH 43210, USA [email protected] Abstract We give an elementary review of black holes in string theory. We discuss BPS holes, the microscopic computation of entropy and the ‘fuzzball’ picture of the arXiv:hep-th/0502050v1 3 Feb 2005 black hole interior suggested by microstates of the 2-charge system. 1Lecture given at the RTN workshop ‘The quantum structure of space-time and the geometric nature of fundamental interactions’, in Crete, Greece (September 2004). 1 Introduction The quantum theory of black holes presents many paradoxes. It is vital to ask how these paradoxes are to be resolved, for the answers will likely lead to deep changes in our understanding of quantum gravity, spacetime and matter. Bekenstein [1] argued that black holes should be attributed an entropy A S = (1.1) Bek 4G where A is the area of the horizon and G is the Newton constant of gravitation. (We have chosen units to set c = ~ = 1.) This entropy must be attributed to the hole if we are to prevent a violation of the second law of thermodynamics. We can throw a box of gas with entropy ∆S into a black hole, and see it vanish into the central singularity. This would seem to decrease the entropy of the Universe, but we note that the area of the horizon increases as a result of the energy added by the box. It turns out that if we assign (1.1) as the entropy of the hole then the total entropy is nondecreasing dS dS Bek + matter 0 (1.2) dt dt ≥ This would seem to be a good resolution of the entropy problem, but it leads to another problem. -
String Theory for Pedestrians
String Theory for Pedestrians – CERN, Jan 29-31, 2007 – B. Zwiebach, MIT This series of 3 lecture series will cover the following topics 1. Introduction. The classical theory of strings. Application: physics of cosmic strings. 2. Quantum string theory. Applications: i) Systematics of hadronic spectra ii) Quark-antiquark potential (lattice simulations) iii) AdS/CFT: the quark-gluon plasma. 3. String models of particle physics. The string theory landscape. Alternatives: Loop quantum gravity? Formulations of string theory. 1 Introduction For the last twenty years physicists have investigated String Theory rather vigorously. Despite much progress, the basic features of the theory remain a mystery. In the late 1960s, string theory attempted to describe strongly interacting particles. Along came Quantum Chromodynamics (QCD)– a theory of quarks and gluons – and despite their early promise, strings faded away. This time string theory is a credible candidate for a theory of all interactions – a unified theory of all forces and matter. Additionally, • Through the AdS/CFT correspondence, it is a valuable tool for the study of theories like QCD. • It has helped understand the origin of the Bekenstein-Hawking entropy of black holes. • Finally, it has inspired many of the scenarios for physics Beyond the Standard Model of Particle physics. 2 Greatest problem of twentieth century physics: the incompatibility of Einstein’s General Relativity and the principles of Quantum Mechanics. String theory appears to be the long-sought quantum mechanical 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. -
Three Duality Symmetries Between Photons and Cosmic String Loops, and Macro and Micro Black Holes
Symmetry 2015, 7, 2134-2149; doi:10.3390/sym7042134 OPEN ACCESS symmetry ISSN 2073-8994 www.mdpi.com/journal/symmetry Article Three Duality Symmetries between Photons and Cosmic String Loops, and Macro and Micro Black Holes David Jou 1;2;*, Michele Sciacca 1;3;4;* and Maria Stella Mongiovì 4;5 1 Departament de Física, Universitat Autònoma de Barcelona, Bellaterra 08193, Spain 2 Institut d’Estudis Catalans, Carme 47, Barcelona 08001, Spain 3 Dipartimento di Scienze Agrarie e Forestali, Università di Palermo, Viale delle Scienze, Palermo 90128, Italy 4 Istituto Nazionale di Alta Matematica, Roma 00185 , Italy 5 Dipartimento di Ingegneria Chimica, Gestionale, Informatica, Meccanica (DICGIM), Università di Palermo, Viale delle Scienze, Palermo 90128, Italy; E-Mail: [email protected] * Authors to whom correspondence should be addressed; E-Mails: [email protected] (D.J.); [email protected] (M.S.); Tel.: +34-93-581-1658 (D.J.); +39-091-23897084 (M.S.). Academic Editor: Sergei Odintsov Received: 22 September 2015 / Accepted: 9 November 2015 / Published: 17 November 2015 Abstract: We present a review of two thermal duality symmetries between two different kinds of systems: photons and cosmic string loops, and macro black holes and micro black holes, respectively. It also follows a third joint duality symmetry amongst them through thermal equilibrium and stability between macro black holes and photon gas, and micro black holes and string loop gas, respectively. The possible cosmological consequences of these symmetries are discussed. Keywords: photons; cosmic string loops; black holes thermodynamics; duality symmetry 1. Introduction Thermal duality relates high-energy and low-energy states of corresponding dual systems in such a way that the thermal properties of a state of one of them at some temperature T are related to the properties of a state of the other system at temperature 1=T [1–6]. -
Large N Free Energy of 3D N=4 Scfts and Ads/CFT Benjamin Assel, John Estes, Masahito Yamazaki
Large N Free Energy of 3d N=4 SCFTs and AdS/CFT Benjamin Assel, John Estes, Masahito Yamazaki To cite this version: Benjamin Assel, John Estes, Masahito Yamazaki. Large N Free Energy of 3d N=4 SCFTs and AdS/CFT. Journal of High Energy Physics, Springer, 2012, pp.074. 10.1007/JHEP09(2012)074. hal-00718824 HAL Id: hal-00718824 https://hal.archives-ouvertes.fr/hal-00718824 Submitted on 18 Jul 2012 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. LPTENS-12/23 PUPT-2418 Large N Free Energy of 3d = 4 SCFTs and N AdS4/CFT3 Benjamin Assel\, John Estes[ and Masahito Yamazaki] \ Laboratoire de Physique Th´eoriquede l'Ecole´ Normale Sup´erieure, 24 rue Lhomond, 75231 Paris cedex, France [ Instituut voor Theoretische Fysica, KU Leuven, Celestijnenlaan 200D B-3001 Leuven, Belgium ] Princeton Center for Theoretical Science, Princeton University, Princeton, NJ 08544, USA Abstract We provide a non-trivial check of the AdS4/CFT3 correspondence recently proposed in [1] by verifying the GKPW relation in the large N limit. The CFT free energy is obtained from the previous works [2, 3] on the S3 partition function for 3-dimensional = 4 SCFT T [SU(N)]. -
Ads₄/CFT₃ and Quantum Gravity
AdS/CFT and quantum gravity Ioannis Lavdas To cite this version: Ioannis Lavdas. AdS/CFT and quantum gravity. Mathematical Physics [math-ph]. Université Paris sciences et lettres, 2019. English. NNT : 2019PSLEE041. tel-02966558 HAL Id: tel-02966558 https://tel.archives-ouvertes.fr/tel-02966558 Submitted on 14 Oct 2020 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Prepar´ ee´ a` l’Ecole´ Normale Superieure´ AdS4/CF T3 and Quantum Gravity Soutenue par Composition du jury : Ioannis Lavdas Costas BACHAS Le 03 octobre 2019 Ecole´ Normale Superieure Directeur de These Guillaume BOSSARD Ecole´ Polytechnique Membre du Jury o Ecole´ doctorale n 564 Elias KIRITSIS Universite´ Paris-Diderot et Universite´ de Rapporteur Physique en ˆIle-de-France Crete´ Michela PETRINI Sorbonne Universite´ President´ du Jury Nicholas WARNER University of Southern California Membre du Jury Specialit´ e´ Alberto ZAFFARONI Physique Theorique´ Universita´ Milano-Bicocca Rapporteur Contents Introduction 1 I 3d N = 4 Superconformal Theories and type IIB Supergravity Duals6 1 3d N = 4 Superconformal Theories7 1.1 N = 4 supersymmetric gauge theories in three dimensions..............7 1.2 Linear quivers and their Brane Realizations...................... 10 1.3 Moduli Space and Symmetries............................ -
Arxiv:Hep-Th/9902033V2 1 Apr 1999
IASSNS–HEP–99/15 hep-th/9902033 On Mirror Symmetry in Three Dimensional Abelian Gauge Theories Anton Kapustin and Matthew J. Strassler School of Natural Sciences, Institute for Advanced Study, Olden Lane, Princeton, NJ 08540, USA kapustin, [email protected] Abstract We present an identity relating the partition function of = 4 supersym- N metric QED to that of its dual under mirror symmetry. The identity is a gen- eralized Fourier transform. Many known properties of abelian theories can be derived from this formula, including the mirror transforms for more general gauge and matter content. We show that = 3 Chern-Simons QED and N = 4 QED with BF-type couplings are conformal field theories with exactly N marginal couplings. Mirror symmetry acts on these theories as strong-weak coupling duality. After identifying the mirror of the gauge coupling (some- times called the “magnetic coupling”) we construct a theory which is exactly mirror — at all scales — to = 4 SQED. We also study vortex-creation N operators in the large Nf limit. arXiv:hep-th/9902033v2 1 Apr 1999 1 I. INTRODUCTION Major advances in supersymmetric field theory and string theory in various dimensions have led to the understanding that it is common for apparently different quantum field theories to be quantum-mechanically equivalent. Two theories which are “dual” in this way may be thought of as two choices of variables in a path integral representation for the same generating functional. Not that such “duality relations” are new; the relation between position space and momentum space representations of quantum mechanical systems are of this type; the order-disorder-fermion representations of the Ising model, the identity of the sine-Gordon model and the Thirring model, and target-space duality in two-dimensional sigma-models are well known from two dimensions; and it has long been conjectured that = 4 supersymmetric Yang-Mills theory in four dimensions is a conformal field theory with aN duality symmetry. -
Spontaneous Symmetry Breaking in Free Theories with Boundary
SciPost Phys. 11, 035 (2021) Spontaneous symmetry breaking in free theories with boundary potentials Vladimir Procházka? and Alexander Söderberg† Department of Physics and Astronomy, Uppsala University, Box 516, SE-751 20 Uppsala, Sweden ? [email protected],† [email protected] Abstract Patterns of symmetry breaking induced by potentials at the boundary of free O(N)- models in d = 3 ε dimensions are studied. We show that the spontaneous symmetry breaking in these− theories leads to a boundary RG flow ending with N 1 Neumann modes in the IR. The possibility of fluctuation-induced symmetry breaking− is examined and we derive a general formula for computing one-loop effective potentials at the boundary. Using the ε-expansion we test these ideas in an O(N) O(N)-model with boundary in- teractions. We determine the RG flow diagram of this⊕ theory and find that it has an IR- stable critical point satisfying conformal boundary conditions. The leading correction to the effective potential is computed and we argue the existence of a phase boundary separating the region flowing to the symmetric fixed point from the region flowing to a symmetry-broken phase with a combination of Neumann and Dirchlet boundary condi- tions. Copyright V.Procházka and A. Söderberg. Received 08-04-2021 This work is licensed under the Creative Commons Accepted 28-07-2021 Check for Attribution 4.0 International License. Published 19-08-2021 updates Published by the SciPost Foundation. doi:10.21468/SciPostPhys.11.2.035 Contents 1 Introduction2 2 One loop effective boundary potentials5 3 O(Nφ) O(Nχ ) scalar model7 3.1 The⊕ model7 3.2 Coleman-Weinberg mechanism9 4 Conclusion 12 A Propagators in boundary quantum field theories 13 A.1 In spacetime coordinates 14 A.2 Momentum propagator 16 B β-function 18 C Functional determinants 20 References 22 1 SciPost Phys. -
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).