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The Pursuit of Quantum Gravity
The Pursuit of Quantum Gravity Cécile DeWitt-Morette The Pursuit of Quantum Gravity Memoirs of Bryce DeWitt from 1946 to 2004 123 Cécile DeWitt-Morette Department of Physics Center for Relativity University of Texas at Austin Austin Texas USA [email protected] ISBN 978-3-642-14269-7 e-ISBN 978-3-642-14270-3 DOI 10.1007/978-3-642-14270-3 Springer Heidelberg Dordrecht London New York Library of Congress Control Number: 2011921724 c Springer-Verlag Berlin Heidelberg 2011 This work is subject to copyright. All rights are reserved, whether the whole or part of the material is con- cerned, specifically the rights of translation, reprinting, reuse of illustrations, recitation, broadcasting, reproduction on microfilm or in any other way, and storage in data banks. Duplication of this publica- tion or parts thereof is permitted only under the provisions of the German Copyright Law of September 9, 1965, in its current version, and permission for use must always be obtained from Springer. Violations are liable to prosecution under the German Copyright Law. The use of general descriptive names, registered names, trademarks, etc. in this publication does not imply, even in the absence of a specific statement, that such names are exempt from the relevant protec- tive laws and regulations and therefore free for general use. Cover design:WMXDesignGmbH,Heidelberg Printed on acid-free paper Springer is part of Springer Science+Business Media (www.springer.com) Dedicated to our daughters, Nicolette, Jan, Christiane, Abigail Preface This book is written for the curious reader. I hope it will also be a good read for the professional physicist. -
Supergravity and Its Legacy Prelude and the Play
Supergravity and its Legacy Prelude and the Play Sergio FERRARA (CERN – LNF INFN) Celebrating Supegravity at 40 CERN, June 24 2016 S. Ferrara - CERN, 2016 1 Supergravity as carved on the Iconic Wall at the «Simons Center for Geometry and Physics», Stony Brook S. Ferrara - CERN, 2016 2 Prelude S. Ferrara - CERN, 2016 3 In the early 1970s I was a staff member at the Frascati National Laboratories of CNEN (then the National Nuclear Energy Agency), and with my colleagues Aurelio Grillo and Giorgio Parisi we were investigating, under the leadership of Raoul Gatto (later Professor at the University of Geneva) the consequences of the application of “Conformal Invariance” to Quantum Field Theory (QFT), stimulated by the ongoing Experiments at SLAC where an unexpected Bjorken Scaling was observed in inclusive electron- proton Cross sections, which was suggesting a larger space-time symmetry in processes dominated by short distance physics. In parallel with Alexander Polyakov, at the time in the Soviet Union, we formulated in those days Conformal invariant Operator Product Expansions (OPE) and proposed the “Conformal Bootstrap” as a non-perturbative approach to QFT. S. Ferrara - CERN, 2016 4 Conformal Invariance, OPEs and Conformal Bootstrap has become again a fashionable subject in recent times, because of the introduction of efficient new methods to solve the “Bootstrap Equations” (Riccardo Rattazzi, Slava Rychkov, Erik Tonni, Alessandro Vichi), and mostly because of their role in the AdS/CFT correspondence. The latter, pioneered by Juan Maldacena, Edward Witten, Steve Gubser, Igor Klebanov and Polyakov, can be regarded, to some extent, as one of the great legacies of higher dimensional Supergravity. -
Chaos, Scaling and Existence of a Continuum Limit in Classical Non-Abelian Lattice Gauge Theory
LA-UR- 9 6 " 4 43"6" Los Alamos National Laboratory is operated by the University of Caiifomia for the United States Department of Energy under contract W-7405-ENG-36 TITLE: CHAOS, SCALING AND EXISTENCE OF A CONTINUUM Q&TJ LIMIT IN CLASSICAL NON-ABELIAN LATTICE GAUGE THEORY AUTHOR(S): Holger Nielsen, Niels Bohr Institute Hans Rugh, Universty of Warwick Svend Rugh, T-6 SUBMITTED TO: 28TH INTERNATIONAL CONFERENCE ON HIGH ENERGY PHYSICS, WARSAW POLAND, JULY 1996 By acceptance of this article, the publisher recognizes that the U.S. Government retains a nonexclusive, royalty-free license to publish or reproduce the published form of this contribution, or to allow others to do so, for U.S. Government purposes. The Los Alamos National Laboratory requests that the publisher identify this article as work performed under the auspices of the U.S. Department of Energy. Los Alamos National Laboratory L< Los Alamos, New Mexico 87545 FORM NO. 836 R4 ST. NO. 2629 5/81 DISTRIBUTION OF THIS DOCUMENT IS UNLIMITED DISCLAIMER Portions of this document may be illegible in electronic image products. Images are produced from the best available original document DISCLAIMER This report was prepared as an account of work sponsored by an agency of the United States Government Neither the United States Government nor any agency thereof, nor any of their employees, makes any warranty, express or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or use- fulness of any information, apparatus, product, or process disclosed, or represents that its use would not infringe privately owned rights. -
Pos(CORFU2019)049 ∗ -Ray Excess
Several degenerate vacua and a model for Dark Matter in the pure Standard Model PoS(CORFU2019)049 Holger Bech Nielsen∗ Niels Bohr Institute, Blegdamsvej 15 -21, Copenhagen E-mail: [email protected] Colin D. Froggatt Glasgow University E-mail: [email protected] We return to a model of ours for what the dark matter can be with the property that it is compatible with the Standard Model alone. The only genuine new physics is a principle imposing restrictions on the parameters/couplings in the Standard Model. They are required to lead to several vacua being degenerate in energy density with each other. We especially look for some of the signals from the dark matter, which are not just gravitational: The 3.55 keV X-ray radiation, the positron excess and further g-ray excess. The picture of ours for dark matter has it being cm-size pearls of 100000 ton mass in order of magnitude. Corfu Summer Institute 2019 "School and Workshops on Elementary Particle Physics and Gravity" (CORFU2019) 31 August - 25 September 2019 Corfu, Greece ∗Speaker. ⃝c Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0). http://pos.sissa.it/ Dark matter, pure S.M. Holger Bech Nielsen 1. Introduction Several degenerate vacua and a model for Dark Matter in the pure Standard Model We believe in the pure Standard Model further up in energy than most physicists, except for see-saw neutrinos and the baryon number excess for which we accept the need for new physics: • No new fundamental particles, except see-saw neutrinos and possibly particles almost at the Planck scale; but we shall not talk about such high energies today. -
Download Report 2010-12
RESEARCH REPORt 2010—2012 MAX-PLANCK-INSTITUT FÜR WISSENSCHAFTSGESCHICHTE Max Planck Institute for the History of Science Cover: Aurora borealis paintings by William Crowder, National Geographic (1947). The International Geophysical Year (1957–8) transformed research on the aurora, one of nature’s most elusive and intensely beautiful phenomena. Aurorae became the center of interest for the big science of powerful rockets, complex satellites and large group efforts to understand the magnetic and charged particle environment of the earth. The auroral visoplot displayed here provided guidance for recording observations in a standardized form, translating the sublime aesthetics of pictorial depictions of aurorae into the mechanical aesthetics of numbers and symbols. Most of the portait photographs were taken by Skúli Sigurdsson RESEARCH REPORT 2010—2012 MAX-PLANCK-INSTITUT FÜR WISSENSCHAFTSGESCHICHTE Max Planck Institute for the History of Science Introduction The Max Planck Institute for the History of Science (MPIWG) is made up of three Departments, each administered by a Director, and several Independent Research Groups, each led for five years by an outstanding junior scholar. Since its foundation in 1994 the MPIWG has investigated fundamental questions of the history of knowl- edge from the Neolithic to the present. The focus has been on the history of the natu- ral sciences, but recent projects have also integrated the history of technology and the history of the human sciences into a more panoramic view of the history of knowl- edge. Of central interest is the emergence of basic categories of scientific thinking and practice as well as their transformation over time: examples include experiment, ob- servation, normalcy, space, evidence, biodiversity or force. -
David Olive: His Life and Work
David Olive his life and work Edward Corrigan Department of Mathematics, University of York, YO10 5DD, UK Peter Goddard Institute for Advanced Study, Princeton, NJ 08540, USA St John's College, Cambridge, CB2 1TP, UK Abstract David Olive, who died in Barton, Cambridgeshire, on 7 November 2012, aged 75, was a theoretical physicist who made seminal contributions to the development of string theory and to our understanding of the structure of quantum field theory. In early work on S-matrix theory, he helped to provide the conceptual framework within which string theory was initially formulated. His work, with Gliozzi and Scherk, on supersymmetry in string theory made possible the whole idea of superstrings, now understood as the natural framework for string theory. Olive's pioneering insights about the duality between electric and magnetic objects in gauge theories were way ahead of their time; it took two decades before his bold and courageous duality conjectures began to be understood. Although somewhat quiet and reserved, he took delight in the company of others, generously sharing his emerging understanding of new ideas with students and colleagues. He was widely influential, not only through the depth and vision of his original work, but also because the clarity, simplicity and elegance of his expositions of new and difficult ideas and theories provided routes into emerging areas of research, both for students and for the theoretical physics community more generally. arXiv:2009.05849v1 [physics.hist-ph] 12 Sep 2020 [A version of section I Biography is to be published in the Biographical Memoirs of Fellows of the Royal Society.] I Biography Childhood David Olive was born on 16 April, 1937, somewhat prematurely, in a nursing home in Staines, near the family home in Scotts Avenue, Sunbury-on-Thames, Surrey. -
Curriculum Vitae
CURRICULUM VITAE Raman Sundrum July 26, 2019 CONTACT INFORMATION Physical Sciences Complex, University of Maryland, College Park, MD 20742 Office - (301) 405-6012 Email: [email protected] CAREER John S. Toll Chair, Director of the Maryland Center for Fundamental Physics, 2012 - present. Distinguished University Professor, University of Maryland, 2011-present. Elkins Chair, Professor of Physics, University of Maryland, 2010-2012. Alumni Centennial Chair, Johns Hopkins University, 2006- 2010. Full Professor at the Department of Physics and Astronomy, The Johns Hopkins University, 2001- 2010. Associate Professor at the Department of Physics and Astronomy, The Johns Hop- kins University, 2000- 2001. Research Associate at the Department of Physics, Stanford University, 1999- 2000. Advisor { Prof. Savas Dimopoulos. 1 Postdoctoral Fellow at the Department of Physics, Boston University. 1996- 1999. Postdoc advisor { Prof. Sekhar Chivukula. Postdoctoral Fellow in Theoretical Physics at Harvard University, 1993-1996. Post- doc advisor { Prof. Howard Georgi. Postdoctoral Fellow in Theoretical Physics at the University of California at Berke- ley, 1990-1993. Postdoc advisor { Prof. Stanley Mandelstam. EDUCATION Yale University, New-Haven, Connecticut Ph.D. in Elementary Particle Theory, May 1990 Thesis Title: `Theoretical and Phenomenological Aspects of Effective Gauge Theo- ries' Thesis advisor: Prof. Lawrence Krauss Brown University, Providence, Rhode Island Participant in the 1988 Theoretical Advanced Summer Institute University of Sydney, Australia B.Sc with First Class Honours in Mathematics and Physics, Dec. 1984 AWARDS, DISTINCTIONS J. J. Sakurai Prize in Theoretical Particle Physics, American Physical Society, 2019. Distinguished Visiting Research Chair, Perimeter Institute, 2012 - present. 2 Moore Fellow, Cal Tech, 2015. American Association for the Advancement of Science, Fellow, 2011. -
Born-Infeld Action, Supersymmetry and String Theory
Imperial/TP/98-99/67 hep-th/9908105 Born-Infeld action, supersymmetry and string theory ⋆ A.A. Tseytlin † Theoretical Physics Group, Blackett Laboratory, Imperial College, London SW7 2BZ, U.K. Abstract We review and elaborate on some aspects of Born-Infeld action and its supersymmetric generalizations in connection with string theory. Contents: BI action from string theory; some properties of bosonic D = 4 BI action; = 1 and = 2 supersymmetric BI actions with manifest linear D = 4 supersymmetry; four-derivativeN N terms in = 4 supersymmetric BI action; BI actions with ‘deformed’ supersymmetry from D-braneN actions; non-abelian generalization of BI action; derivative corrections to BI action in open superstring theory. arXiv:hep-th/9908105v5 11 Dec 1999 To appear in the Yuri Golfand memorial volume, ed. M. Shifman, World Scientific (2000) August 1999 ⋆ e-mail address: [email protected] † Also at Lebedev Physics Institute, Moscow. 1. Introduction It is a pleasure for me to contribute to Yuri Golfand’s memorial volume. I met Yuri several times during his occasional visits of Lebedev Institute in the 80’s. Two of our discussions in 1985 I remember quite vividly. Golfand found appealing the interpretation of string theory as a theory of ‘quantized coordinates’, viewing it as a generalization of some old ideas of noncommuting coordinates. In what should be an early spring of 1985 he read our JETP Letter [1] which was a brief Russian version of our approach with Fradkin [2] to string theory effective action based on representation of generating functional for string amplitudes as Polyakov string path integral with a covariant 2-d sigma model in the exponent. -
Stanley Mandelstam
I knew very early of Stanley Mandelstam I started physics as a t Prisoner of the s u Mandelstam Triangle I escaped from the Mandelstam Triangle only to be ensnared in Light-Cone Superspace A Note of Personal Gratitude 1971 NAL Visit SuperConformal Theories P. Ramond (with S. Ananth, D. Belyaev, L. Brink and S.-S. Kim) Light-Cone Superspaces N=4 Super Yang-Mills N=8 SuperConformal N=8 SuperGravity and E7(7) N=16 SuperGravity and E8(8) N=8 Light-Cone Superspace houses D=11: N=1 SuperGravity SO(9); F4/SO(9) D=4: N=8 SuperGravity SO(2)x E7(7) D=3: N=16 SuperGravity E8(8) D=2: N=16 Theory E9(9) N=4 Light-Cone Superspace habitat for D=10: N=1 Super Yang-Mills SO(8) D=4: N=4 Super Yang-Mills PSU(2,2|4) D=3: N=8 Super Conformal OSp(2,2|8) 1 i 1 ϕ (y) = 1 A (y) + i θm θn C (y) + 1θm θn θp θq $ ∂+ A¯ (y) + m n mn m n p mnpqq + ¯ ϕ (y) = +∂A (y) + √2θ θ Cmn (y) +12 θ θ θ θ $mnpq ∂ A (y) ∂ √2 √ 12 1 i 1 i m 2 m n p q m n m n p q + i+ +¯ θ χ¯m(y) + √2θ θ θ $mnpq χ (y) ϕ (y) = + A (y) + θ θ Cmn (y) + θ θ θ θ $mnpq ∂ ∂Am(y) 6 m n p q ∂ √2 12 + θ χ¯m(y) + θ θ θ $mnpq χ (y) 1 i m n 1 m n p ∂q+ + ¯ 6 ϕ (y) = A (y) + √θ θ C L(C2y) + Fθorθ maθ θ $lmnpqism∂ A (y) ∂+i m √ 2 m nmnp q12 + θ χ¯m(y) +2 θ θ θ $mnpq χ (y) 1 0 3 ∂+ 6 x± = (x x ) i √2 √ m m n p q 12 0± 3 + + θ χ¯m(y) + θ θ θ $mnpq χ (y) x± = (x x ) ∂ 6 √2 ± Light-Cone Co1ordina0 3tes: 1 0 3 x± = (x x ) ∂± = ( ∂ ∂ ) √2 ± √2 − ± 1 0 3 1 0 3 x± = (x x ) ∂± = ( ∂ ∂ ) 1 0√ 3 ± 1 1 2√2 − ±1 1 2 ∂± = ( ∂ 2∂ ) x = (x + ix ) x = (x ix ) √2 − ± √2 √2 − m m + 1 1 2 1 1 2 1 q+ , q¯+ n =1 i√2δ n ∂ x = 1(x + ix -
Personal Recollections of the Early Days Before and After the Birth of Supergravity
Personal recollections of the early days before and after the birth of Supergravity Peter van Nieuwenhuizen I March 29, 1976: Dan Freedman, Sergio Ferrara and I submit first paper on Supergravity to Physical Review D. I April 28: Stanley Deser and Bruno Zumino: elegant reformulation that stresses the role of torsion. I June 2, 2016 at 1:30pm: 5500 papers with Supergravity in the title have appeared, and 15000 dealing with supergravity. I Supergravity has I led to the AdS/CFT miracle, and I made breakthroughs in longstanding problems in mathematics. I Final role of supergravity? (is it a solution in search of a problem?) I 336 papers in supergravity with 126 collaborators I Now: many directions I can only observe in awe from the sidelines I will therefore tell you my early recollections and some anecdotes. I will end with a new research program that I am enthusiastic about. In 1972 I was a Joliot Curie fellow at Orsay (now the Ecole Normale) in Paris. Another postdoc (Andrew Rothery from England) showed me a little book on GR by Lawden.1 I was hooked. That year Deser gave lectures at Orsay on GR, and I went with him to Brandeis. In 1973, 't Hooft and Veltman applied their new covariant quantization methods and dimensional regularization to pure gravity, using the 't Hooft lemma (Gilkey) for 1-loop divergences and the background field formalism of Bryce DeWitt. They found that at one loop, pure gravity was finite: 1 2 2 ∆L ≈ αRµν + βR = 0 on-shell. But what about matter couplings? 1\An Introduction to Tensor Calculus and Relativity". -
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. -
Julian Schwinger: Nuclear Physics, the Radiation Laboratory, Renormalized QED, Source Theory, and Beyond
Julian Schwinger: Nuclear Physics, the Radiation Laboratory, Renormalized QED, Source Theory, and Beyond Kimball A. Milton∗ Homer L. Dodge Department of Physics and Astronomy University of Oklahoma, Norman, OK 73019 USA October 9, 2006 Abstract Julian Schwinger’s influence on twentieth century science is pro- found and pervasive. Of course, he is most famous for his renormal- ization theory of quantum electrodynamics, for which he shared the Nobel Prize with Richard Feynman and Sin-itiro Tomonaga. But al- though this triumph was undoubtedly his most heroic work, his legacy lives on chiefly through subtle and elegant work in classical electrody- namics, quantum variational principles, proper-time methods, quan- tum anomalies, dynamical mass generation, partial symmetry, and more. Starting as just a boy, he rapidly became the pre-eminent nu- clear physicist in the late 1930s, led the theoretical development of radar technology at MIT during World War II, and then, soon after the war, conquered quantum electrodynamics, and became the leading quantum field theorist for two decades, before taking a more icono- clastic route during his last quarter century. Keywords: Julian Schwinger, nuclear physics, waveguides, quan- tum electrodynamics, renormalization, quantum action principle, source theory, axial-vector anomaly ∗K.A. Milton is Professor of Physics at the University of Oklahoma. He was a Ph.D. stu- dent of Julian Schwinger from 1968–71, and his postdoc at UCLA for the rest of the 1970s. He has written a scientific biography of Schwinger, edited two volumes of Schwinger’s se- lected works, and co-authored two textbooks based on Schwinger’s lectures.