Ads/CFT Correspondence and the Quark-Gluon Plasma
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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 .. -
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). -
Duality and Strings Dieter Lüst, LMU and MPI München
Duality and Strings Dieter Lüst, LMU and MPI München Freitag, 15. März 13 Luis made several very profound and important contributions to theoretical physics ! Freitag, 15. März 13 Luis made several very profound and important contributions to theoretical physics ! Often we were working on related subjects and I enjoyed various very nice collaborations and friendship with Luis. Freitag, 15. März 13 Luis made several very profound and important contributions to theoretical physics ! Often we were working on related subjects and I enjoyed various very nice collaborations and friendship with Luis. Duality of 4 - dimensional string constructions: • Covariant lattices ⇔ (a)symmetric orbifolds (1986/87: W. Lerche, D.L., A. Schellekens ⇔ L. Ibanez, H.P. Nilles, F. Quevedo) • Intersecting D-brane models ☞ SM (?) (2000/01: R. Blumenhagen, B. Körs, L. Görlich, D.L., T. Ott ⇔ G. Aldazabal, S. Franco, L. Ibanez, F. Marchesano, R. Rabadan, A. Uranga) Freitag, 15. März 13 Luis made several very profound and important contributions to theoretical physics ! Often we were working on related subjects and I enjoyed various very nice collaborations and friendship with Luis. Duality of 4 - dimensional string constructions: • Covariant lattices ⇔ (a)symmetric orbifolds (1986/87: W. Lerche, D.L., A. Schellekens ⇔ L. Ibanez, H.P. Nilles, F. Quevedo) • Intersecting D-brane models ☞ SM (?) (2000/01: R. Blumenhagen, B. Körs, L. Görlich, D.L., T. Ott ⇔ G. Aldazabal, S. Franco, L. Ibanez, F. Marchesano, R. Rabadan, A. Uranga) ➢ Madrid (Spanish) Quiver ! Freitag, 15. März 13 Luis made several very profound and important contributions to theoretical physics ! Often we were working on related subjects and I enjoyed various very nice collaborations and friendship with Luis. -
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. -
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). -
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 .......................... -
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. -
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. -
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.