Supergravity, Ads/Cft Correspondence and Conformal Bootstrap
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Quantum Groups and Algebraic Geometry in Conformal Field Theory
QUANTUM GROUPS AND ALGEBRAIC GEOMETRY IN CONFORMAL FIELD THEORY DlU'KKERU EI.INKWIJK BV - UTRECHT QUANTUM GROUPS AND ALGEBRAIC GEOMETRY IN CONFORMAL FIELD THEORY QUANTUMGROEPEN EN ALGEBRAISCHE MEETKUNDE IN CONFORME VELDENTHEORIE (mrt em samcnrattint] in hit Stdirlands) PROEFSCHRIFT TER VERKRIJGING VAN DE GRAAD VAN DOCTOR AAN DE RIJKSUNIVERSITEIT TE UTRECHT. OP GEZAG VAN DE RECTOR MAGNIFICUS. TROF. DR. J.A. VAN GINKEI., INGEVOLGE HET BESLUIT VAN HET COLLEGE VAN DE- CANEN IN HET OPENBAAR TE VERDEDIGEN OP DINSDAG 19 SEPTEMBER 1989 DES NAMIDDAGS TE 2.30 UUR DOOR Theodericus Johannes Henrichs Smit GEBOREN OP 8 APRIL 1962 TE DEN HAAG PROMOTORES: PROF. DR. B. DE WIT PROF. DR. M. HAZEWINKEL "-*1 Dit proefschrift kwam tot stand met "•••; financiele hulp van de stichting voor Fundamenteel Onderzoek der Materie (F.O.M.) Aan mijn ouders Aan Saskia Contents Introduction and summary 3 1.1 Conformal invariance and the conformal bootstrap 11 1.1.1 Conformal symmetry and correlation functions 11 1.1.2 The conformal bootstrap program 23 1.2 Axiomatic conformal field theory 31 1.3 The emergence of a Hopf algebra 4G The modular geometry of string theory 56 2.1 The partition function on moduli space 06 2.2 Determinant line bundles 63 2.2.1 Complex line bundles and divisors on a Riemann surface . (i3 2.2.2 Cauchy-Riemann operators (iT 2.2.3 Metrical properties of determinants of Cauchy-Ricmann oper- ators 6!) 2.3 The Mumford form on moduli space 77 2.3.1 The Quillen metric on determinant line bundles 77 2.3.2 The Grothendieck-Riemann-Roch theorem and the Mumford -
M Theory As a Holographic Field Theory
hep-th/9712130 CALT-68-2152 M-Theory as a Holographic Field Theory Petr Hoˇrava California Institute of Technology, Pasadena, CA 91125, USA [email protected] We suggest that M-theory could be non-perturbatively equivalent to a local quantum field theory. More precisely, we present a “renormalizable” gauge theory in eleven dimensions, and show that it exhibits various properties expected of quantum M-theory, most no- tably the holographic principle of ’t Hooft and Susskind. The theory also satisfies Mach’s principle: A macroscopically large space-time (and the inertia of low-energy excitations) is generated by a large number of “partons” in the microscopic theory. We argue that at low energies in large eleven dimensions, the theory should be effectively described by arXiv:hep-th/9712130 v2 10 Nov 1998 eleven-dimensional supergravity. This effective description breaks down at much lower energies than naively expected, precisely when the system saturates the Bekenstein bound on energy density. We show that the number of partons scales like the area of the surface surrounding the system, and discuss how this holographic reduction of degrees of freedom affects the cosmological constant problem. We propose the holographic field theory as a candidate for a covariant, non-perturbative formulation of quantum M-theory. December 1997 1. Introduction M-theory has emerged from our understanding of non-perturbative string dynamics, as a hypothetical quantum theory which has eleven-dimensional supergravity [1] as its low- energy limit, and is related to string theory via various dualities [2-4] (for an introduction and references, see e.g. -
Structure, Classification, and Conformal Symmetry, of Elementary
Lett Math Phys (2009) 89:171–182 DOI 10.1007/s11005-009-0351-2 Structure, Classification, and Conformal Symmetry, of Elementary Particles over Non-Archimedean Space–Time V. S. VARADARAJAN and JUKKA VIRTANEN Department of Mathematics, UCLA, Los Angeles, CA 90095-1555, USA. e-mail: [email protected]; [email protected] Received: 3 April 2009 / Revised: 12 September 2009 / Accepted: 12 September 2009 Publishedonline:23September2009–©TheAuthor(s)2009. This article is published with open access at Springerlink.com Abstract. It is known that no length or time measurements are possible in sub-Planckian regions of spacetime. The Volovich hypothesis postulates that the micro-geometry of space- time may therefore be assumed to be non-archimedean. In this letter, the consequences of this hypothesis for the structure, classification, and conformal symmetry of elementary particles, when spacetime is a flat space over a non-archimedean field such as the p-adic numbers, is explored. Both the Poincare´ and Galilean groups are treated. The results are based on a new variant of the Mackey machine for projective unitary representations of semidirect product groups which are locally compact and second countable. Conformal spacetime is constructed over p-adic fields and the impossibility of conformal symmetry of massive and eventually massive particles is proved. Mathematics Subject Classification (2000). 22E50, 22E70, 20C35, 81R05. Keywords. Volovich hypothesis, non-archimedean fields, Poincare´ group, Galilean group, semidirect product, cocycles, affine action, conformal spacetime, conformal symmetry, massive, eventually massive, massless particles. 1. Introduction In the 1970s many physicists, concerned about the divergences in quantum field theories, started exploring the micro-structure of space–time itself as a possible source of these problems. -
Census Taking
Current Logic of String Theory • Pick an asymptotically cold background. • Calculate the low energy S-matrix (or boundary correlators). • Find a semiclassical action that gives the same amplitudes. • Use the semiclassical action (perhaps non-perturbatively) to construct low energy bulk physics. Background Independence? Bundling different asymptotically cold backgrounds into a single quantum system (Hilbert Space) does not appear to make sense. This is a BIG problem: Real cosmology is NOT asymptotically cold. De Sitter space is asymptotically warm. Finite Hilbert space for every diamond. Banks, Fischler Quantum description ????????????????? Do we have a set of principles that we can rely on? No. Do we need them? Yes. Do we have a set of principles that we can rely on? No. Do we need them? Yes. The measure problem Solve equations of motion in freely falling frame and express A in terms of operators in the remote past. † Ain = U A U Ain Using the S-matrix we can run the operator to the remote future † Aout = S Ain S = (S U†) Ain (U S†) Aout is an operator in the outgoing space of states that has the same statistics as the behind-the-horizon operator A. That is the meaning of Black Hole Complementarity: Conjugation by (S U†). Transition to a “Hat” (supersymmetric bubble with Λ=0) Asymptotically cold at T Æ∞ but not as R Æ∞ Hat Complementarity? The CT’s backward light cone intersects each space- like hypersurface. The hypersurfaces are uniformly negatively curved spaces. Space-like hypersurface intersects the CT’s backward light-cone. In the limit tCT Æ∞ the CT’s Hilbert space becomes infinite. -
Conformal Bootstrap Signatures of the Tricritical Ising Universality Class
PHYSICAL REVIEW D 101, 116020 (2020) Conformal bootstrap signatures of the tricritical Ising universality class Chethan N. Gowdigere , Jagannath Santara, and Sumedha School of Physical Sciences, National Institute of Science Education and Research, Jatni 752050, India and Homi Bhabha National Institute, Training School Complex, Anushakti Nagar, Mumbai 400094, India (Received 28 November 2018; revised manuscript received 17 April 2020; accepted 12 June 2020; published 30 June 2020) We study the tricritical Ising universality class using conformal bootstrap techniques. By studying bootstrap constraints originating from multiple correlators on the conformal field theory (CFT) data of multiple operator product expansions (OPEs), we are able to determine the scaling dimension of the spin field Δσ in various noninteger dimensions 2 ≤ d ≤ 3. Here, Δσ is connected to the critical exponent η that governs the (tri)critical behavior of the two-point function via the relation η ¼ 2 − d þ 2Δσ. Our results for Δσ match with the exactly known values in two and three dimensions and are a conjecture for noninteger 3 dimensions. We also compare our CFT results for Δσ with ϵ-expansion results, available up to ϵ order. Our techniques can be naturally extended to study higher-order multicritical points. DOI: 10.1103/PhysRevD.101.116020 I. INTRODUCTION the restrictions imposed by conformal invariance and found that the conformal field theory corresponding to The consequences of the conformal hypothesis which the Ising universality class sits on the boundary of the posits conformal invariance to the behavior of physical allowed region at a kinklike point in the space of scaling systems at criticality, in addition to scale invariance, are dimensions of the only two relevant operators. -
WILLY FISCHLER Born: May 30, 1949 Antwerp, Belgium Education
WILLY FISCHLER Born: May 30, 1949 Antwerp, Belgium Education: Universite Libre de Bruxelles Licence in Physics with \grande distinction", 1972 (Equivalent to the American Masters degree). Universite Libre de Bruxelles Ph.D., 1976 with \la plus grande distinction". Austin Community College Emergency Medical Services Professions EMT Paramedic Certificate, 2009. Nationally Certified Paramedic, 2009- Texas Department of State Health Services Licensed EMT-P, 2009- Present Position: University of Texas at Austin Jane and Roland Blumberg Centennial Professor in Physics 2000- Professor of Physics 1983-2000 Associate Director Theory Group 2003- Marble Falls Area EMS Licensed Paramedic 2009- Past Positions: CERN Geneva 1975-77 Postdoctoral Fellow Los Alamos Scientific Lab, 1977-1979 Postdoctoral Fellow University of Pennsylvania, 1979-1983 Assistant Professor Institute for Advanced Study, Princeton Official Visitor, September 1980 - May 1981 1 On leave - Belgian Army, June 1981 - May 1982 Awards: CERN Fellowship 1975-77 1979-1980 Recipient of Outstanding Junior Researcher Award, DOE 1987-88 Fellow to the Jane and Roland Blumberg Centennial Professorship in Physics Dean's Fellow, Fall 1997 2000{ Jane and Roland Blumberg Centennial Professor in Physics Volunteer: Children's Hospital PACU, 2005-7 Westlake Fire Department, EMT 2006- PUBLICATIONS 1. Gauge invariance in spontaneously broken symmetries: (with R. Brout) Phys. Rev. D11, 905 (1975). 2. Effective potential instabilities and bound-state formation: (with E. Gunzig, and R. Brout) Il Nuovo Cimento 29A, 504 (1975); 3. Effective potential, instabilities and bound state formation: (Adden- dum) (with E. Gunzig, and R. Brout) Il Nuovo Cimento 32A, 125 (1976). 4. Magnetic confinement in non-Abelian gauge field theory: (with F. -
Solving the 3D Ising Model with the Conformal Bootstrap Sheer El-Showk, Miguel Paulos, David Poland, Slava Rychkov, David Simmons-Duffin, Alessandro Vichi
Solving the 3D Ising model with the conformal bootstrap Sheer El-Showk, Miguel Paulos, David Poland, Slava Rychkov, David Simmons-Duffin, Alessandro Vichi To cite this version: Sheer El-Showk, Miguel Paulos, David Poland, Slava Rychkov, David Simmons-Duffin, et al.. Solving the 3D Ising model with the conformal bootstrap. Physical Review D, American Physical Society, 2012, 86 (2), pp.25022. 10.1103/PhysRevD.86.025022. cea-00825766 HAL Id: cea-00825766 https://hal-cea.archives-ouvertes.fr/cea-00825766 Submitted on 17 Oct 2019 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. This is the accepted manuscript made available via CHORUS. The article has been published as: Solving the 3D Ising model with the conformal bootstrap Sheer El-Showk, Miguel F. Paulos, David Poland, Slava Rychkov, David Simmons-Duffin, and Alessandro Vichi Phys. Rev. D 86, 025022 — Published 20 July 2012 DOI: 10.1103/PhysRevD.86.025022 LPTENS{12/07 Solving the 3D Ising Model with the Conformal Bootstrap Sheer El-Showka, Miguel F. Paulosb, David Polandc, Slava Rychkovd, David Simmons-Duffine, -
3D Ising Model and Conformal Bootstrap
3D Ising Model and Conformal Bootstrap Slava Rychkov (ENS Paris & CERN) CERN Winter School on Supergravity, Strings, and Gauge Theory 2013 see also “Lectures on CFT in D≥3” @ sites.google.com/site/slavarychkov Part 1 Conformal symmetry (Physical foundations & Basics, Ising model as an example) 2 /60 The subject of these lectures is: The simplest - experimentally relevant - unsolved Conformal Field Theory is 3D Ising Model @ T=Tc It’s also an ideal playground to explain the technique of conformal bootstrap... 3 /60 Basics on the Ising Model cubic lattice → Paradigmatic model of ferromagnetism M- spont. magnetization Tc T Critical temperature (Curie point) 4 /60 Correlation length Critical point can also be detected by looking at the spin-spin correlations For T>Tc : correlation length At T=Tc: Critical theory is scale invariant: It is also conformally invariant [conjectured by Polyakov’71] 5 /60 2D Ising Model • free energy solved by Onsager’44 on the lattice and for any T • Polyakov noticed that is conf. inv. at T=Tc • In 1983 Belavin-Polyakov-Zamolodchikov identified the critical 2D Ising model with the first unitary minimal model 6 /60 3D Ising Model • Lattice model at generic T is probably not solvable [many people tried] • Critical theory (T=Tc) in the continuum limit might be solvable [few people tried, conformal invariance poorly used] 7 /60 Existing approaches to 3D Ising • Lattice Monte-Carlo • High-T expansion on the lattice [~strong coupling expansion] Expand exponential in Converges for T>> Tc , extrapolate for T→ Tc by Pade -
Lie Group and Geometry on the Lie Group SL2(R)
INDIAN INSTITUTE OF TECHNOLOGY KHARAGPUR Lie group and Geometry on the Lie Group SL2(R) PROJECT REPORT – SEMESTER IV MOUSUMI MALICK 2-YEARS MSc(2011-2012) Guided by –Prof.DEBAPRIYA BISWAS Lie group and Geometry on the Lie Group SL2(R) CERTIFICATE This is to certify that the project entitled “Lie group and Geometry on the Lie group SL2(R)” being submitted by Mousumi Malick Roll no.-10MA40017, Department of Mathematics is a survey of some beautiful results in Lie groups and its geometry and this has been carried out under my supervision. Dr. Debapriya Biswas Department of Mathematics Date- Indian Institute of Technology Khargpur 1 Lie group and Geometry on the Lie Group SL2(R) ACKNOWLEDGEMENT I wish to express my gratitude to Dr. Debapriya Biswas for her help and guidance in preparing this project. Thanks are also due to the other professor of this department for their constant encouragement. Date- place-IIT Kharagpur Mousumi Malick 2 Lie group and Geometry on the Lie Group SL2(R) CONTENTS 1.Introduction ................................................................................................... 4 2.Definition of general linear group: ............................................................... 5 3.Definition of a general Lie group:................................................................... 5 4.Definition of group action: ............................................................................. 5 5. Definition of orbit under a group action: ...................................................... 5 6.1.The general linear -
Black Hole Production and Graviton Emission in Models with Large Extra Dimensions
Black hole production and graviton emission in models with large extra dimensions Dissertation zur Erlangung des Doktorgrades der Naturwissenschaften vorgelegt beim Fachbereich Physik der Johann Wolfgang Goethe–Universit¨at in Frankfurt am Main von Benjamin Koch aus N¨ordlingen Frankfurt am Main 2007 (D 30) vom Fachbereich Physik der Johann Wolfgang Goethe–Universit¨at als Dissertation angenommen Dekan ........................................ Gutachter ........................................ Datum der Disputation ................................ ........ Zusammenfassung In dieser Arbeit wird die m¨ogliche Produktion von mikroskopisch kleinen Schwarzen L¨ochern und die Emission von Gravitationsstrahlung in Modellen mit großen Extra-Dimensionen untersucht. Zun¨achst werden der theoretisch-physikalische Hintergrund und die speziel- len Modelle des behandelten Themas skizziert. Anschließend wird auf die durchgefuhrten¨ Untersuchungen zur Erzeugung und zum Zerfall mikrosko- pisch kleiner Schwarzer L¨ocher in modernen Beschleunigerexperimenten ein- gegangen und die wichtigsten Ergebnisse zusammengefasst. Im Anschluss daran wird die Produktion von Gravitationsstrahlung durch Teilchenkollisio- nen diskutiert. Die daraus resultierenden analytischen Ergebnisse werden auf hochenergetische kosmische Strahlung angewandt. Die Suche nach einer einheitlichen Theorie der Naturkr¨afte Eines der großen Ziele der theoretischen Physik seit Einstein ist es, eine einheitliche und m¨oglichst einfache Theorie zu entwickeln, die alle bekannten Naturkr¨afte beschreibt. -
Pulling Yourself up by Your Bootstraps in Quantum Field Theory
Pulling Yourself Up by Your Bootstraps in Quantum Field Theory Leonardo Rastelli Yang Institute for Theoretical Physics Stony Brook University ICTP and SISSA Trieste, April 3 2019 A. Sommerfeld Center, Munich January 30 2019 Quantum Field Theory in Fundamental Physics Local quantum fields ' (x) f i g x = (t; ~x), with t = time, ~x = space The language of particle physics: for each particle species, a field Quantum Field Theory for Collective Behavior Modelling N degrees of freedom in statistical mechanics. Example: Ising! model 1 (uniaxial ferromagnet) σi = 1, spin at lattice site i ± P Energy H = J σiσj − (ij) Near Tc, field theory description: magnetization '(~x) σ(~x) , ∼ h i Z h i H = d3x ~ ' ~ ' + m2'2 + λ '4 + ::: r · r 2 m T Tc ∼ − Z h i H = d3x ~ ' ~ ' + m2'2 + λ '4 + ::: r · r The dots stand for higher-order \operators": '6, (~ ' ~ ')'2, '8, etc. r · r They are irrelevant for the large-distance physics at T T . ∼ c Crude rule of thumb: an operator is irrelevant if its scaling weight [ ] > 3 (3 d, dimension of space). O O ≡ Basic assignments: ['] = 1 d 1 and [~x] = 1 = [~ ] = 1. 2 ≡ 2 − − ) r So ['2] = 1, ['4] = 2, [~ ' ~ '] =3, while ['8] = 4 etc. r · r First hint of universality: critical exponents do not depend on details. E.g., C T T −α, ' (T T )β for T < T , etc. T ∼ j − cj h i ∼ c − c QFT \Theory of fluctuating fields” (Duh!) ≡ Traditionally, QFT is formulated as a theory of local \quantum fields”: Z H['(x)] Y − Z = d'(x) e g x In particle physics, x spacetime and g = ~ (quantum) 2 In statistical mechanics, x space and g = T (thermal). -
Feynman Diagrams and the Large Charge Expansion in 3−Ε Dimensions
Physics Letters B 802 (2020) 135202 Contents lists available at ScienceDirect Physics Letters B www.elsevier.com/locate/physletb Feynman diagrams and the large charge expansion in 3 − ε dimensions ∗ ∗ ∗ ∗ Gil Badel a, , Gabriel Cuomo a, , Alexander Monin a,b, , Riccardo Rattazzi a, a Theoretical Particle Physics Laboratory (LPTP), Institute of Physics, EPFL, Lausanne, Switzerland b Department of Theoretical Physics, University of Geneva, 24 quai Ernest-Ansermet, 1211 Geneva, Switzerland a r t i c l e i n f o a b s t r a c t Article history: In arXiv:1909 .01269 it was shown that the scaling dimension of the lightest charge n operator in the Received 12 December 2019 U (1) model at the Wilson-Fisher fixed point in D = 4 − ε can be computed semiclassically for arbitrary Accepted 6 January 2020 values of λn, where λ is the perturbatively small fixed point coupling. Here we generalize this result to Available online 10 January 2020 the fixed point of the U (1) model in 3 − ε dimensions. The result interpolates continuously between Editor: N. Lambert diagrammatic calculations and the universal conformal superfluid regime for CFTs at large charge. In 0 particular it reproduces the expectedly universal O(n ) contribution to the scaling dimension of large charge operators in 3D CFTs. © 2020 Published by Elsevier B.V. This is an open access article under the CC BY license 3 (http://creativecommons.org/licenses/by/4.0/). Funded by SCOAP . 1. Introduction EFT construction, or, in fact, deriving it. This was recently illus- trated in [13], by focusing on the two-point function of the charge n It is known that, even in a weakly coupled Quantum Field n operator φ in the U (1) invariant Wilson-Fisher fixed point in Theory (QFT), there exist situations where the ordinary Feynman 4 − ε dimensions.