The Problem of Mass and Mass Generation Harald Fritzsch
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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). -
Tcomposite Weak Bosons, Leptons and Quarks
Subnuclear Physics: Past, Present and Future Pontifical Academy of Sciences, Scripta Varia 119, Vatican City 2014 www.pas.va/content/dam/accademia/pdf/sv119/sv119-fritzsch.pdf TComposite Weak Bosons, Leptons and Quarks HARALD FRITZSCH University of Munich Faculty of Physics, Arnold Sommerfeld Center for Theoretical Physics, Abstract The weak bosons consist of two fermions, bound by a new confin- ing gauge force. The mass scale of this new interaction is determined. At energies below 0.5 TeV the standard electroweak theory is valid. AneutralisoscalarweakbosonX must exist - its mass is less than 1TeV.Itwilldecaymainlyintoquarkandleptonpairsandintotwo or three weak bosons. Above the mass of 1 TeV one finds excitations of the weak bosons, which mainly decay into pairs of weak bosons. Leptons and quarks consist of a fermion and a scalar. Pairs of leptons and pairs of quarks form resonances at very high energy. 280 Subnuclear Physics: Past, Present and Future COMPOSITE WEAK BOSONS, LEPTONS AND QUARKS In the Standard Model the leptons, quarks and weak bosons are pointlike particles. I shall assume that they are composite particles with a finite size. The present limit on the size of the electron, the muon and of the light quarks is about 10−17 cm. The constituents of the weak bosons and of the leptons and quarks are bound by a new confining gauge interaction. Due to the parity violation in the weak interactions this theory must be a chiral gauge theory, unlike quantum chromodynamics. The Greek translation of ”simple” is ”haplos”. We denote the con- stituents as ”haplons” and the new confining gauge theory as quantum hap- lodynamics ( QHD ). -
Neutrino Mass Models: a Road Map
Neutrino Mass Models: a road map S.F.King School of Physics and Astronomy, University of Southampton, Southampton SO17 1BJ, UK E-mail: [email protected] Abstract. In this talk we survey some of the recent promising developments in the search for the theory behind neutrino mass and mixing, and indeed all fermion masses and mixing. The talk is organized in terms of a neutrino mass models road map according to which the answers to experimental questions provide sign posts to guide us through the maze of theoretical models eventually towards a complete theory of flavour and uni¯cation. 1. Introduction It has been one of the long standing goals of theories of particle physics beyond the Standard Model (SM) to predict quark and lepton masses and mixings. With the discovery of neutrino mass and mixing, this quest has received a massive impetus. Indeed, perhaps the greatest advance in particle physics over the past decade has been the discovery of neutrino mass and mixing involving two large mixing angles commonly known as the atmospheric angle θ23 and the solar angle θ12, while the remaining mixing angle θ13, although unmeasured, is constrained to be relatively small [1]. The largeness of the two large lepton mixing angles contrasts sharply with the smallness of the quark mixing angles, and this observation, together with the smallness of neutrino masses, provides new and tantalizing clues in the search for the origin of quark and lepton flavour. However, before trying to address such questions, it is worth recalling why neutrino mass forces us to go beyond the SM. -
Quantum Gravity from the QFT Perspective
Quantum Gravity from the QFT perspective Ilya L. Shapiro Universidade Federal de Juiz de Fora, MG, Brazil Partial support: CNPq, FAPEMIG ICTP-SAIFR/IFT-UNESP – 1-5 April, 2019 Ilya Shapiro, Quantum Gravity from the QFT perspective April - 2019 Lecture 5. Advances topics in QG Induced gravity concept. • Effective QG: general idea. • Effective QG as effective QFT. • Where we are with QG?. • Bibliography S.L. Adler, Rev. Mod. Phys. 54 (1982) 729. S. Weinberg, Effective Field Theory, Past and Future. arXive:0908.1964[hep-th]; J.F. Donoghue, The effective field theory treatment of quantum gravity. arXive:1209.3511[gr-qc]; I.Sh., Polemic notes on IR perturbative quantum gravity. arXiv:0812.3521 [hep-th]. Ilya Shapiro, Quantum Gravity from the QFT perspective April - 2019 I. Induced gravity. The idea of induced gravity is simple, while its realization may be quite non-trivial, depending on the theory. In any case, the induced gravity concept is something absolutely necessary if we consider an interaction of gravity with matter and quantum theory concepts. I. Induced gravity from cut-off Original simplest version. Ya.B. Zeldovich, Sov. Phys. Dokl. 6 (1967) 883. A.D. Sakharov, Sov. Phys. Dokl. 12 (1968) 1040. Strong version of induced gravity is like that: Suppose that the metric has no pre-determined equations of motion. These equations result from the interaction to matter. Main advantage: Since gravity is not fundamental, but induced interaction, there is no need to quantize metric. Ilya Shapiro, Quantum Gravity from the QFT perspective April - 2019 And we already know that the semiclassical approach has no problems with renormalizability! Suppose we have a theory of quantum matter fields Φ = (ϕ, ψ, Aµ) interacting to the metric gµν . -
Interactions the Newsletter of the UB Department of Physics Volume 4, Issue 2 Fall 2011
Interactions The Newsletter of the UB Department of Physics Volume 4, Issue 2 Fall 2011 established well formulated procedures for all the graduate studies. He continues to be a source of information and ad- vice for our graduate program. Our majors, headed by Alec Cheney, were instrumental in starting a new chapter of the Sigma Pi Sigma, the Phys- ics Honors Society, at UB. They collected signatures and petitioned the Society for a UB chapter. After successfully receiving approval, they also made arrangements for the installation. The President of the Sigma PI Sigma, Dr. Di- ane Jacobs, presided the chapter installation ceremony on November 4. Five students, Alec Cheney, Matthew Gorfien, Connor Gorman, Chun Kwan and Katherine Spoth, were in- Dear alumni and friends, ducted during the ceremony. It was very rewarding to see As I mentioned in the previous issue, the new President and our majors take charge, accomplish their goals and receive the Dean of CAS are now in office. The SUNY2020 legisla- recognition for their outstanding achievements. tion was passed and signed into law, which allows UB for This year’s Homecoming was made special by the return of the first time to plan on a five-year horizon. The new direc- our distinguished alumnus, Dr. Thomas Bogdan (featured tions and initiatives that are being implemented by the new in Alumni in Focus), to give an exciting public lecture on administration are therefore more tangible than symbolic. space weather. He has been the Director of the National This means opportunities for the Department. It is encour- Space Weather Prediction Center, and was recently named aging to see that the President’s plan for the University over- the President of the University Corporation for Atmospheric laps with some of the main concerns and aspirations of the Research, starting January 9, 2012. -
Richard Feynman by Harald Fritzsch
ARTSCIENCE MUSEUM™ PRESENTS ALL POSSIBLE Harald Fritzsch Richard Feynman RICHARD FEYNMAN’S CURIOUS LIFE In 1968, I escaped from East Germany with a folding canoe, crossing the Black In 1975, Feynman bought a Dodge Tradesman Maxivan and had it painted with Sea from Northern Bulgaria to Turkey. Then I worked as a Ph.D. student at the Feynman diagrams. Once, we were going camping with Feynman and his wife Max-Planck-Institute in Munich. In the Fall of 1970, I went for 6 months to the in the Anza Borrego desert park near Palm Springs. Feyman drove his big Stanford Linear Accelerator Center (SLAC) in Palo Alto, California. Since at that camping car. On the way back, Feynman stopped at a gas station in Palm time I collaborated with Murray Gell-Mann, I went twice a month for a few days Springs. The guy at the station asked Feynman: “Why you have these to the California Institute of Technology (Caltech) in Pasadena, about 360 miles Feynman Diagrams on your car?” Feynman told him, that he is Feynman, and south from Palo Alto. the guy answered: “Well, in this case you do not have to pay for the gasoline.” In Caltech I met Richard Feynman for the first time, and we discussed physics Feynman had a house at the beach near Ensenada in Baja California, Mexico. almost every day, in particular his parton model. He assumed that the nucleons He called the house “Casita Barranca”. Feynman invited us to plan a visit to consist of small pointlike constituents, which he called partons. -
Particle & Nuclear Physics Quantum Field Theory
Particle & Nuclear Physics Quantum Field Theory NOW AVAILABLE New Books & Highlights in 2019-2020 ON WORLDSCINET World Scientific Lecture Notes in Physics - Vol 83 Lectures of Sidney Coleman on Quantum Field Field Theory Theory A Path Integral Approach Foreword by David Kaiser 3rd Edition edited by Bryan Gin-ge Chen (Leiden University, Netherlands), David by Ashok Das (University of Rochester, USA & Institute of Physics, Derbes (University of Chicago, USA), David Griffiths (Reed College, Bhubaneswar, India) USA), Brian Hill (Saint Mary’s College of California, USA), Richard Sohn (Kronos, Inc., Lowell, USA) & Yuan-Sen Ting (Harvard University, “This book is well-written and very readable. The book is a self-consistent USA) introduction to the path integral formalism and no prior knowledge of it is required, although the reader should be familiar with quantum “Sidney Coleman was the master teacher of quantum field theory. All of mechanics. This book is an excellent guide for the reader who wants a us who knew him became his students and disciples. Sidney’s legendary good and detailed introduction to the path integral and most of its important course remains fresh and bracing, because he chose his topics with a sure application in physics. I especially recommend it for graduate students in feel for the essential, and treated them with elegant economy.” theoretical physics and for researchers who want to be introduced to the Frank Wilczek powerful path integral methods.” Nobel Laureate in Physics 2004 Mathematical Reviews 1196pp Dec 2018 -
A Fermi National Accelerator Laboratory
a Fermi National Accelerator Laboratory FERMILAB-Pub-83/l&THY January, 1983 Composite Model with Confining SU(N) x SU(2)L x SU(2)K Hypercolor Carl H. Albright Fermi National Accelerator Laboratory P.O. Box 500, Batavia, Illinois 60510 and Department of Physics, Northern Illinois University* DeKalb, Illinois 60115 ABSTRACT A model of composite quarks and leptons is constructed with confining SU(N) x SU(2jL x SU(2)R hypercolor interactions such that only standard quark and lepton families appear in global SU(2)L x SU(2)K doublets. Several generations are admitted by the anomaly-matching conditions and labeled by a discrete axial symmetry. The SU(N) interactions are N independent and play the role Of technicolor. Three conserved U(l)" charges identified with Q, B - L and B + L prohibit qqq + Lc transitions. 3 Oparatrd by Unlvsrsitiae Research Association Inc. under contract with the United States Department of Energy -2- FERMILAB-Pub-83/16-THY With little or no support from the experimental realm, an extensive literature fl on the subject of composite quarks and leptons has emerged over the past few years. Many of the papers are based on the pioneering work of 't Hooft who formulated several criteria which composite models should satisfy in order to explain why quarks and leptons are nearly massless on the large energy scale where the hypercolor forces become sufficiently strong to bind the massless preons together. General searches for candidate preon models have been carried out, or specfific models themselves have been proposed, in which the fundamental preons are either all spinors or spinors and scalars and the weak gauge fields are either fundamental or composite. -
Murray Gell-Mann Hadrons, Quarks And
A Life of Symmetry Dennis Silverman Department of Physics and Astronomy UC Irvine Biographical Background Murray Gell-Mann was born in Manhattan on Sept. 15, 1929, to Jewish parents from the Austro-Hungarian empire. His father taught German to Americans. Gell-Mann was a child prodigy interested in nature and math. He started Yale at 15 and graduated at 18 with a bachelors in Physics. He then went to graduate school at MIT where he received his Ph. D. in physics at 21 in 1951. His thesis advisor was the famous Vicky Weisskopf. His life and work is documented in remarkable detail on videos that he recorded on webofstories, which can be found by just Google searching “webofstories Gell-Mann”. The Young Murray Gell-Mann Gell-Mann’s Academic Career (from Wikipedia) He was a postdoctoral fellow at the Institute for Advanced Study in 1951, and a visiting research professor at the University of Illinois at Urbana– Champaign from 1952 to 1953. He was a visiting associate professor at Columbia University and an associate professor at the University of Chicago in 1954-55, where he worked with Fermi. After Fermi’s death, he moved to the California Institute of Technology, where he taught from 1955 until he retired in 1993. Web of Stories video of Gell-Mann on Fermi and Weisskopf. The Weak Interactions: Feynman and Gell-Mann •Feynman and Gell-Mann proposed in 1957 and 1958 the theory of the weak interactions that acted with a current like that of the photon, minus a similar one that included parity violation. -
Spontaneous Symmetry Breaking and Mass Generation As Built-In Phenomena in Logarithmic Nonlinear Quantum Theory
Vol. 42 (2011) ACTA PHYSICA POLONICA B No 2 SPONTANEOUS SYMMETRY BREAKING AND MASS GENERATION AS BUILT-IN PHENOMENA IN LOGARITHMIC NONLINEAR QUANTUM THEORY Konstantin G. Zloshchastiev Department of Physics and Center for Theoretical Physics University of the Witwatersrand Johannesburg, 2050, South Africa (Received September 29, 2010; revised version received November 3, 2010; final version received December 7, 2010) Our primary task is to demonstrate that the logarithmic nonlinearity in the quantum wave equation can cause the spontaneous symmetry break- ing and mass generation phenomena on its own, at least in principle. To achieve this goal, we view the physical vacuum as a kind of the funda- mental Bose–Einstein condensate embedded into the fictitious Euclidean space. The relation of such description to that of the physical (relativis- tic) observer is established via the fluid/gravity correspondence map, the related issues, such as the induced gravity and scalar field, relativistic pos- tulates, Mach’s principle and cosmology, are discussed. For estimate the values of the generated masses of the otherwise massless particles such as the photon, we propose few simple models which take into account small vacuum fluctuations. It turns out that the photon’s mass can be naturally expressed in terms of the elementary electrical charge and the extensive length parameter of the nonlinearity. Finally, we outline the topological properties of the logarithmic theory and corresponding solitonic solutions. DOI:10.5506/APhysPolB.42.261 PACS numbers: 11.15.Ex, 11.30.Qc, 04.60.Bc, 03.65.Pm 1. Introduction Current observational data in astrophysics are probing a regime of de- partures from classical relativity with sensitivities that are relevant for the study of the quantum-gravity problem [1,2]. -
Magnetic Moment (G-2) and New Physics
Magnetic moment (g − 2)µ and new physics Dominik Stöckinger Dresden Lepton Moments, July 2010 Dominik Stöckinger Magnetic moment (g − 2)µ and new physics Introduction exp SM A3σ deviation for aµ − aµ has been established! Currently: exp SM −11 aµ − aµ = (255 ± 63 ± 49) × 10 Expected with new Fermilab exp. (and th. progress): exp SM −11 aµ − aµ = (?? ± 16 ± 30) × 10 Which types of physics beyond the SM could explain this? What is the impact of aµ on physics beyond the SM? Dominik Stöckinger Magnetic moment (g − 2)µ and new physics Outline 1 Introduction 2 Different types of new physics 3 aµ, parameter measurements and model discrimination SUSY could explain the deviation Littlest Higgs (T-parity) cannot explain the deviation Randall-Sundrum models could explain the deviation 4 Conclusions Dominik Stöckinger Magnetic moment (g − 2)µ and new physics Introduction Outline 1 Introduction 2 Different types of new physics 3 aµ, parameter measurements and model discrimination SUSY could explain the deviation Littlest Higgs (T-parity) cannot explain the deviation Randall-Sundrum models could explain the deviation 4 Conclusions Dominik Stöckinger Magnetic moment (g − 2)µ and new physics Introduction Muon magnetic moment Quantum field theory: Operator: aµ µ¯ σ qνµ mµ L µν R CP-, Flavour-conserving, chirality-flipping, loop-induced 2 Heavy particles contribute ∝ mµ Mheavy Sensitive to all SM interactions Sensitive to TeV-scale new physics in a unique way Dominik Stöckinger Magnetic moment (g − 2)µ and new physics Introduction Why new physics? Big questions EWSB, Higgs, mass generation? hierarchy MPl/MW ? Naturalness? Unification of the Coupling Constants in the SM and the minimal MSSM i i α 60 α 60 1/α 1/ 1/ 1 MSSM 50 50 40 40 α 1/ 2 30 30 20 20 10 10 α 1/ 3 0 0 0 5 10 15 0 5 10 15 10log Q 10log Q dark matter? Grand Unification? . -
Advanced Information on the Nobel Prize in Physics, 5 October 2004
Advanced information on the Nobel Prize in Physics, 5 October 2004 Information Department, P.O. Box 50005, SE-104 05 Stockholm, Sweden Phone: +46 8 673 95 00, Fax: +46 8 15 56 70, E-mail: [email protected], Website: www.kva.se Asymptotic Freedom and Quantum ChromoDynamics: the Key to the Understanding of the Strong Nuclear Forces The Basic Forces in Nature We know of two fundamental forces on the macroscopic scale that we experience in daily life: the gravitational force that binds our solar system together and keeps us on earth, and the electromagnetic force between electrically charged objects. Both are mediated over a distance and the force is proportional to the inverse square of the distance between the objects. Isaac Newton described the gravitational force in his Principia in 1687, and in 1915 Albert Einstein (Nobel Prize, 1921 for the photoelectric effect) presented his General Theory of Relativity for the gravitational force, which generalized Newton’s theory. Einstein’s theory is perhaps the greatest achievement in the history of science and the most celebrated one. The laws for the electromagnetic force were formulated by James Clark Maxwell in 1873, also a great leap forward in human endeavour. With the advent of quantum mechanics in the first decades of the 20th century it was realized that the electromagnetic field, including light, is quantized and can be seen as a stream of particles, photons. In this picture, the electromagnetic force can be thought of as a bombardment of photons, as when one object is thrown to another to transmit a force.