Glimpses of Superhistory
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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. -
Dual Fields and E {11}
KCL-MTH-06-14 hep-th/0612001 Dual fields and E11 Fabio Riccioni and Peter West Department of Mathematics King’s College, London WC2R 2LS, UK Abstract We show that the adjoint representation of E11 contains generators corresponding to the infinite possible dual descriptions of the bosonic on-shell degrees of freedom of eleven dimensional supergravity. We also give an interpretation for the fields corresponding to many of the other generators in the adjoint representation. arXiv:hep-th/0612001v1 1 Dec 2006 1 A few years ago it was conjectured [1] that a rank eleven Kac-Moody algebra, which was called E11, was a symmetry of M theory. The non-linear realisation of this algebra at its lowest levels was shown to contain the fields of eleven dimensional supergravity and to have the equations of motion of this theory [1] when one made use of the earlier results of reference [2]. The physical field content is extracted by decomposing the adjoint representation of E11 into the representations of its A10, or Sl(11), sub-algebra which is associated in the non-linear realisation with eleven dimensional gravity. Non-linear realisations of E11 can also be used to describe ten dimensional theories, but in this case the adjoint representation is decomposed into representations of A9, or Sl(10), associated with ten dimensional gravity. There are only two such A9 subalgebras and the two different choices were found to lead to non-linear realisations which at low levels are the IIA and IIB supergravity theories in references [1] and [3] respectively. It is striking to examine tables of the generators [4] listed in terms of increasing level and see how the generators associated with the field content of the IIA and IIB supergravity theories occupy precisely all the lower levels before an infinite sea of generators whose physical significance was unknown at the time the tables of reference [4] were constructed. -
The Making of the Standard Theory
August 11, 2016 9:28 The Standard Theory of Particle Physics - 9.61in x 6.69in b2471-ch02 page 29 Chapter 2 The Making of the Standard Theory John Iliopoulos Laboratoire de Physique Th´eorique, Ecole´ Normale Sup´erieure, 24 rue Lhomond, 75005 Paris, France 1. Introduction The construction of the Standard Model, which became gradually the Standard Theory of elementary particle physics, is, probably, the most remarkable achieve- ment of modern theoretical physics. In this Chapter we shall deal mostly with the weak interactions. It may sound strange that a revolution in particle physics was initiated by the study of the weakest among them (the effects of the gravitational interactions are not measurable in high energy physics), but we shall see that the weak interactions triggered many such revolutions and we shall have the occasion to meditate on the fundamental significance of “tiny” effects. We shall outline the various steps, from the early days of the Fermi theory to the recent experimental discoveries, which confirmed all the fundamental predictions of the Theory. We shall follow a phenomenological approach, in which the introduction of every new concept is motivated by the search of a consistent theory which agrees with experiment. As we shall explain, this is only part of the story, the other part being the requirement of mathematical consistency. Both went in parallel and the real history requires the understanding of both. In fact, as we intend to show, the initial motivation was not really phenomenological. It is one of these rare cases in which a revolution in physics came from theorists trying to go beyond a simple phenomenological model, The Standard Theory of Particle Physics Downloaded from www.worldscientific.com not from an experimental result which forced them to do so. -
Lectures on D-Branes
CPHT/CL-615-0698 hep-th/9806199 Lectures on D-branes Constantin P. Bachas1 Centre de Physique Th´eorique, Ecole Polytechnique 91128 Palaiseau, FRANCE [email protected] ABSTRACT This is an introduction to the physics of D-branes. Topics cov- ered include Polchinski’s original calculation, a critical assessment of some duality checks, D-brane scattering, and effective worldvol- ume actions. Based on lectures given in 1997 at the Isaac Newton Institute, Cambridge, at the Trieste Spring School on String The- ory, and at the 31rst International Symposium Ahrenshoop in Buckow. arXiv:hep-th/9806199v2 17 Jan 1999 June 1998 1Address after Sept. 1: Laboratoire de Physique Th´eorique, Ecole Normale Sup´erieure, 24 rue Lhomond, 75231 Paris, FRANCE, email : [email protected] Lectures on D-branes Constantin Bachas 1 Foreword Referring in his ‘Republic’ to stereography – the study of solid forms – Plato was saying : ... for even now, neglected and curtailed as it is, not only by the many but even by professed students, who can suggest no use for it, never- theless in the face of all these obstacles it makes progress on account of its elegance, and it would not be astonishing if it were unravelled. 2 Two and a half millenia later, much of this could have been said for string theory. The subject has progressed over the years by leaps and bounds, despite periods of neglect and (understandable) criticism for lack of direct experimental in- put. To be sure, the construction and key ingredients of the theory – gravity, gauge invariance, chirality – have a firm empirical basis, yet what has often catalyzed progress is the power and elegance of the underlying ideas, which look (at least a posteriori) inevitable. -
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. -
Hep-Th/0304246. (Cit
University of Groningen Kac-Moody Symmetries and Gauged Supergravity Nutma, Teake Aant IMPORTANT NOTE: You are advised to consult the publisher's version (publisher's PDF) if you wish to cite from it. Please check the document version below. Document Version Publisher's PDF, also known as Version of record Publication date: 2010 Link to publication in University of Groningen/UMCG research database Citation for published version (APA): Nutma, T. A. (2010). Kac-Moody Symmetries and Gauged Supergravity. s.n. Copyright Other than for strictly personal use, it is not permitted to download or to forward/distribute the text or part of it without the consent of the author(s) and/or copyright holder(s), unless the work is under an open content license (like Creative Commons). Take-down policy If you believe that this document breaches copyright please contact us providing details, and we will remove access to the work immediately and investigate your claim. Downloaded from the University of Groningen/UMCG research database (Pure): http://www.rug.nl/research/portal. For technical reasons the number of authors shown on this cover page is limited to 10 maximum. Download date: 26-09-2021 Bibliography [6] Richard L. Arnowitt, Stanley Deser, and Charles W. Misner. \The dynamics of general relativity". In: Gravitation: an introduction to current research (1962), 227264. eprint: gr-qc/0405109. (Cit. on p. 107). [7] V. A. Belinsky, I. M. Khalatnikov, and E. M. Lifshitz. \Oscillatory approach to a singular point in the relativistic cosmology". In: Adv. Phys. 19 (1970), pp. 525{573. doi: 10.1080/00018737000101171. -
The Charm of Theoretical Physics (1958– 1993)?
Eur. Phys. J. H 42, 611{661 (2017) DOI: 10.1140/epjh/e2017-80040-9 THE EUROPEAN PHYSICAL JOURNAL H Oral history interview The Charm of Theoretical Physics (1958{ 1993)? Luciano Maiani1 and Luisa Bonolis2,a 1 Dipartimento di Fisica and INFN, Piazzale A. Moro 5, 00185 Rome, Italy 2 Max Planck Institute for the History of Science, Boltzmannstraße 22, 14195 Berlin, Germany Received 10 July 2017 / Received in final form 7 August 2017 Published online 4 December 2017 c The Author(s) 2017. This article is published with open access at Springerlink.com Abstract. Personal recollections on theoretical particle physics in the years when the Standard Theory was formed. In the background, the remarkable development of Italian theoretical physics in the second part of the last century, with great personalities like Bruno Touschek, Raoul Gatto, Nicola Cabibbo and their schools. 1 Apprenticeship L. B. How did your interest in physics arise? You enrolled in the late 1950s, when the period of post-war reconstruction of physics in Europe was coming to an end, and Italy was entering into a phase of great expansion. Those were very exciting years. It was the beginning of the space era. L. M. The beginning of the space era certainly had a strong influence on many people, absolutely. The landing on the moon in 1969 was for sure unforgettable, but at that time I was already working in Physics and about to get married. My interest in physics started well before. The real beginning was around 1955. Most important for me was astronomy. It is not surprising that astronomy marked for many people the beginning of their interest in science. -
Doing Electroweak Physics with Roberto
IL NUOVO CIMENTO 40 C (2017) 153 DOI 10.1393/ncc/i2017-17153-y Colloquia: PRZ Memorial Doing electroweak physics with Roberto ∗ Luciano Maiani(1)(2)(3)( ) (1) INFN, Sezione di Roma - Roma, Italy (2) Dipartimento di Fisica, Universit`adiRoma-Roma,Italy (3) CERN - Gen`eve, Switzerland received 27 November 2017 Summary. — Friendship and Collaboration with Roberto, while the Standard Theory was unfolding under our eyes. At the end of the sixties, dual models dominated the scene as the theory of strong interactions. However, the years 1971-1973 brought decisive discoveries [1]. • 1971, ’t Hooft and Veltman showed that the Weinberg-Salam theory is renormalisable; • 1972, Bouchiat, Iliopoulos and Meyer proved the cancellation of Adler anomalies in the electroweak theory with four quarks. In a letter from John, there must be charm, quarks have color and are fractionally charged; • 1973 the discovery of neutral currents by Gargamelle at CERN; • ... and in the same year came the discovery of asymptotic freedom of the Yang-Mills theory by Gross and Wilczeck and Politzer. Shortly after, the idea of color interaction of quarks was put forward by Fritzsch, Gell-Mann and Leutwyler. In three years, the paradigm of particle interactions shifted completely towards field theory, a shining example of what Thomas Kuhn in 1962 had called a scientific revolution. In 1974, the discovery of the J/Ψ opened another chapter: heavy fermions, initiated with charm and later continued with the heavy lepton, beauty and top. The Standard Theory was taking form, everybody became electroweak & free, at least asymptotically. ∗ ( ) E-mail: [email protected] Creative Commons Attribution 4.0 License (http://creativecommons.org/licenses/by/4.0) 1 2 LUCIANO MAIANI 1. -
NEW PHYSICS at the LHC John Iliopoulos
FOLLOWING THE PATH OF CHARM: NEW PHYSICS AT THE LHC John Iliopoulos To cite this version: John Iliopoulos. FOLLOWING THE PATH OF CHARM: NEW PHYSICS AT THE LHC. 2008. hal-00283706 HAL Id: hal-00283706 https://hal.archives-ouvertes.fr/hal-00283706 Preprint submitted on 30 May 2008 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-08/27 FOLLOWING THE PATH OF CHARM: NEW PHYSICS AT THE LHC JOHN ILIOPOULOS Laboratoire de Physique Th´eorique de L’Ecole Normale Sup´erieure 75231 Paris Cedex 05, France Talk presented at the ICTP on the occasion of the Dirac medal award ceremony Trieste, 27/03/08 hal-00283706, version 1 - 30 May 2008 It is a great honour for me to speak on this occasion and I want to ex- press my gratitude to the Abdus Salam International Centre for Theoretical Physics as well as the Selection Committee of the Dirac Medal. It is also a great pleasure to be here with Luciano Maiani and discuss the consequences of our common work with Sheldon Glashow on charmed particles [1]. I will argue in this talk that the same kind of reasoning, which led us to predict the opening of a new chapter in hadron physics, may shed some light on the existence of new physics at the as yet unexplored energy scales of LHC. -
The Making of the Standard Theory
Chapter 2 The Making of the Standard Theory John Iliopoulos Laboratoire de Physique Th´eorique, Ec´ ole Normale Sup´erieure, 24 rue Lhomond, 75005 Paris, France 1. Introduction The construction of the Standard Model, which became gradually the Standard Theory of elementary particle physics, is, probably, the most remarkable achieve- ment of modern theoretical physics. In this Chapter we shall deal mostly with the weak interactions. It may sound strange that a revolution in particle physics was initiated by the study of the weakest among them (the effects of the gravitational interactions are not measurable in high energy physics), but we shall see that the weak interactions triggered many such revolutions and we shall have the occasion to meditate on the fundamental significance of “tiny” effects. We shall outline the various steps, from the early days of the Fermi theory to the recent experimental discoveries, which confirmed all the fundamental predictions of the Theory. We shall follow a phenomenological approach, in which the introduction of every new concept is motivated by the search of a consistent theory which agrees with experiment. As we shall explain, this is only part of the story, the other part being the requirement of mathematical consistency. Both went in parallel and the real history requires the understanding of both. In fact, as we intend to show, the initial motivation was not really phenomenological. It is one of these rare cases in which a revolution in physics came from theorists trying to go beyond a simple phenomenological model, The Standard Theory of Particle Physics Downloaded from www.worldscientific.com not from an experimental result which forced them to do so. -
E11 Must Be a Symmetry of Strings and Branes ∗ Alexander G
Physics Letters B 759 (2016) 663–671 Contents lists available at ScienceDirect Physics Letters B www.elsevier.com/locate/physletb E11 must be a symmetry of strings and branes ∗ Alexander G. Tumanov, Peter West Department of Mathematics, King’s College, London WC2R 2LS, UK a r t i c l e i n f o a b s t r a c t Article history: We construct the dynamical equations, at low levels, that are contained in the non-linear realisation of Received 4 February 2016 the semi-direct product of E11 and its vector representation in five and eleven dimensions. Restricting Received in revised form 5 April 2016 these equations to contain only the usual fields of supergravity and the generalised space–time to be Accepted 6 June 2016 the usual space–time we find the equations of motion of the five and eleven dimensional maximal Available online 8 June 2016 supergravity theories. Since this non-linear realisation contains effects that are beyond the supergravity Editor: N. Lambert approximation and are thought to be present in an underlying theory we conclude that the low energy effective action of string and branes should possess an E11 symmetry. © 2016 The Authors. 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 maximal supergravity theories. These is one in eleven dimensions, two in ten dimensions and one in each dimension below ten. In It has been conjectured that the low energy effective action for addition there also a substantial number of so called gauged su- strings and branes is the non-linear realisation of the semi-direct pergravity theories which are obtained by adding a cosmological product of E11 and its vector (l1) representation, denoted E11 ⊗s l1 constant to a massless maximal supergravity theory in a given [1,2]. -
Reflections on a Revolution John Iliopoulos, Reply by Sheldon Lee Glashow
INFERENCE / Vol. 5, No. 3 Reflections on a Revolution John Iliopoulos, reply by Sheldon Lee Glashow In response to “The Yang–Mills Model” (Vol. 5, No. 2). Internal Symmetries As Glashow points out, particle physicists distinguish To the editors: between space-time and internal symmetry transforma- tions. The first change the point of space and time, leaving Gauge theories brought about a profound revolution in the the fundamental equations unchanged. The second do not way physicists think about the fundamental forces. It is this affect the space-time point but transform the dynamic vari- revolution that is the subject of Sheldon Glashow’s essay. ables among themselves. This fundamentally new concept Gauge theories, such as the Yang–Mills model, use two was introduced by Werner Heisenberg in 1932, the year mathematical concepts: group theory, which is the natural the neutron was discovered, but the real history is more language to describe the physical property of symmetry, complicated.3 Heisenberg’s 1932 papers are an incredible and differential geometry, which connects in a subtle way mixture of the old and the new. For many people at that symmetry and dynamics. time, the neutron was a new bound state of a proton and Although there exist several books, and many more an electron, like a small hydrogen atom. Heisenberg does articles, relating historical aspects of these theories,1 a not reject this idea. Although for his work he considers real history has not yet been written. It may be too early. the neutron as a spin one-half Dirac fermion, something When a future historian undertakes this task, Glashow’s incompatible with a proton–electron bound state, he notes precise, documented, and authoritative essay will prove that “under suitable circumstances [the neutron] can invaluable.