Asymptotic Freedom and QCD–A Historical Perspective
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Asymptotic Freedom, Quark Confinement, Proton Spin Crisis, Neutron Structure, Dark Matters, and Relative Force Strengths
Preprints (www.preprints.org) | NOT PEER-REVIEWED | Posted: 17 February 2021 doi:10.20944/preprints202102.0395.v1 Asymptotic freedom, quark confinement, proton spin crisis, neutron structure, dark matters, and relative force strengths Jae-Kwang Hwang JJJ Physics Laboratory, Brentwood, TN 37027 USA Abstract: The relative force strengths of the Coulomb forces, gravitational forces, dark matter forces, weak forces and strong forces are compared for the dark matters, leptons, quarks, and normal matters (p and n baryons) in terms of the 3-D quantized space model. The quark confinement and asymptotic freedom are explained by the CC merging to the A(CC=-5)3 state. The proton with the (EC,LC,CC) charge configuration of p(1,0,-5) is p(1,0) + A(CC=-5)3. The A(CC=-5)3 state has the 99.6% of the proton mass. The three quarks in p(1,0,-5) are asymptotically free in the EC and LC space of p(1,0) and are strongly confined in the CC space of A(CC=-5)3. This means that the lepton beams in the deep inelastic scattering interact with three quarks in p(1,0) by the EC interaction and weak interaction. Then, the observed spin is the partial spin of p(1,0) which is 32.6 % of the total spin (1/2) of the proton. The A(CC=-5)3 state has the 67.4 % of the proton spin. This explains the proton spin crisis. The EC charge distribution of the proton is the same to the EC charge distribution of p(1,0) which indicates that three quarks in p(1,0) are mostly near the proton surface. -
Hep-Th/9609099V1 11 Sep 1996 ⋆ † Eerhspotdi Atb O Rn DE-FG02-90ER40542
IASSNS 96/95 hep-th/9609099 September 1996 ⋆ Asymptotic Freedom Frank Wilczek† School of Natural Sciences Institute for Advanced Study Olden Lane Princeton, N.J. 08540 arXiv:hep-th/9609099v1 11 Sep 1996 ⋆ Lecture on receipt of the Dirac medal for 1994, October 1994. Research supported in part by DOE grant DE-FG02-90ER40542. [email protected] † ABSTRACT I discuss how the basic phenomenon of asymptotic freedom in QCD can be un- derstood in elementary physical terms. Similarly, I discuss how the long-predicted phenomenon of “gluonization of the proton” – recently spectacularly confirmed at HERA – is a rather direct manifestation of the physics of asymptotic freedom. I review the broader significance of asymptotic freedom in QCD in fundamental physics: how on the one hand it guides the interpretation and now even the design of experiments, and how on the other it makes possible a rational, quantitative theoretical approach to problems of unification and early universe cosmology. 2 I am very pleased to accept your award today. On this occasion I think it is appropriate to discuss with you the circle of ideas around asymptotic freedom. After a few remarks about its setting in intellectual history, I will begin by ex- plaining the physical origin of asymptotic freedom in QCD; then I will show how a recent, spectacular experimental observation – the ‘gluonization’ of the proton – both confirms and illuminates its essential nature; then I will discuss some of its broader implications for fundamental physics. It may be difficult for young people who missed experiencing it, or older people with fading memories, fully to imagine the intellectual atmosphere surrounding the strong interaction in the 1960s and early 1970s. -
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 ). -
1 Introduction
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by CERN Document Server 1 TWENTY FIVE YEARS OF ASYMPTOTIC FREEDOM David J. Gross Institute For Theoretical Physics, UCSB Santa Barbara, California, USA e-mail: [email protected] Abstract th On the o ccasion of the 25 anniversary of Asymptotic Freedom, celebrated at the QCD Euorconference 98 on Quantum Chro dynamics, Montp ellier, July 1998, I describ ed the discovery of Asymptotic Freedom and the emergence of QCD. 1 INTRODUCTION Science progresses in a much more muddled fashion than is often pictured in history b o oks. This is esp ecially true of theoretical physics, partly b ecause history is written by the victorious. Con- sequently, historians of science often ignore the many alternate paths that p eople wandered down, the many false clues they followed, the many misconceptions they had. These alternate p oints of view are less clearly develop ed than the nal theories, harder to understand and easier to forget, esp ecially as these are viewed years later, when it all really do es make sense. Thus reading history one rarely gets the feeling of the true nature of scienti c development, in which the element of farce is as great as the element of triumph. The emergence of QCD is a wonderful example of the evolution from farce to triumph. During a very short p erio d, a transition o ccurred from exp erimental discovery and theoretical confusion to theoretical triumph and exp erimental con rmation. In trying to relate this story, one must be wary of the danger of the p ersonal bias that o ccurs as one lo oks back in time. -
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 -
Color Screening in Quantum Chromodynamics Arxiv
Color Screening in Quantum Chromodynamics Alexei Bazavov, Johannes H. Weber Department of Computational Mathematics, Science and Engineering and Department of Physics and Astronomy, Michigan State University, East Lansing, MI 48824, USA October 6, 2020 Abstract We review lattice studies of the color screening in the quark-gluon plasma. We put the phenomena related to the color screening into the context of similar aspects of other physical systems (electromag- netic plasma or cold nuclear matter). We discuss the onset of the color screening and its signature and significance in the QCD transi- tion region, and elucidate at which temperature and to which extent the weak-coupling picture based on hard thermal loop expansion, po- tential nonrelativistic QCD, or dimensionally-reduced QCD quantita- tively captures the key properties of the color screening. We discuss the different regimes pertaining to the color screening and thermal arXiv:2010.01873v1 [hep-lat] 5 Oct 2020 dissociation of the static quarks in depth for various spatial correla- tion functions that are studied on the lattice, and clarify the status of their asymptotic screening masses. We finally discuss the screening correlation functions of dynamical mesons with a wide range of flavor and spin content, and how they conform with expectations for low- and high-temperature behavior. 1 Contents 1 Introduction3 2 Field theoretical foundations7 2.1 Partition function and Lagrangian . .7 2.2 Finite temperature field theory . 11 2.3 Lattice regularization . 14 2.4 Renormalization and weak coupling . 17 2.5 Light quarks . 19 2.6 Heavy quarks . 21 2.7 Implementation of QCD on the lattice . -
Iasinstitute for Advanced Study
IAInsti tSute for Advanced Study Faculty and Members 2012–2013 Contents Mission and History . 2 School of Historical Studies . 4 School of Mathematics . 21 School of Natural Sciences . 45 School of Social Science . 62 Program in Interdisciplinary Studies . 72 Director’s Visitors . 74 Artist-in-Residence Program . 75 Trustees and Officers of the Board and of the Corporation . 76 Administration . 78 Past Directors and Faculty . 80 Inde x . 81 Information contained herein is current as of September 24, 2012. Mission and History The Institute for Advanced Study is one of the world’s leading centers for theoretical research and intellectual inquiry. The Institute exists to encourage and support fundamental research in the sciences and human - ities—the original, often speculative thinking that produces advances in knowledge that change the way we understand the world. It provides for the mentoring of scholars by Faculty, and it offers all who work there the freedom to undertake research that will make significant contributions in any of the broad range of fields in the sciences and humanities studied at the Institute. Y R Founded in 1930 by Louis Bamberger and his sister Caroline Bamberger O Fuld, the Institute was established through the vision of founding T S Director Abraham Flexner. Past Faculty have included Albert Einstein, I H who arrived in 1933 and remained at the Institute until his death in 1955, and other distinguished scientists and scholars such as Kurt Gödel, George F. D N Kennan, Erwin Panofsky, Homer A. Thompson, John von Neumann, and A Hermann Weyl. N O Abraham Flexner was succeeded as Director in 1939 by Frank Aydelotte, I S followed by J. -
Asymptotic Freedom and Higher Derivative Gauge Theories Arxiv
Asymptotic freedom and higher derivative gauge theories M. Asoreya F. Falcetoa L. Rachwałb aCentro de Astropartículas y Física de Altas Energías, Departamento de Física Teórica Universidad de Zaragoza, C/ Pedro Cerbuna 12, E-50009 Zaragoza, Spain bDepartamento de Física – ICE, Universidade Federal de Juiz de Fora, Rua José Lourenço Kelmer, Campus Universitário, Juiz de Fora, 36036-900, MG, Brazil E-mail: [email protected], [email protected], [email protected] Abstract: The ultraviolet completion of gauge theories by higher derivative terms can dramatically change their behavior at high energies. The requirement of asymp- totic freedom imposes very stringent constraints that are only satisfied by a small family of higher derivative theories. If the number of derivatives is large enough (n > 4) the theory is strongly interacting both at extreme infrared and ultraviolet regimes whereas it remains asymptotically free for a low number of extra derivatives (n 6 4). In all cases the theory improves its ultraviolet behavior leading in some cases to ultraviolet finite theories with vanishing β-function. The usual consistency problems associated to the presence of extra ghosts in higher derivative theories may not harm asymptotically free theories because in that case the effective masses of such ghosts are running to infinity in the ultraviolet limit. Keywords: gauge theories, renormalization group, higher derivatives regulariza- tion, asymptotic freedom arXiv:2012.15693v3 [hep-th] 11 May 2021 1 Introduction Field theories with higher derivatives were first considered as covariant ultraviolet regularizations of gauge theories [1]-[3]. However, in the last years there is a renewed interest in these theories mainly due to the rediscovery that they provide a renormal- izable field theoretical framework for the quantization of gravity [4,5]. -
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. -
Exploring the Fundamental Properties of Matter with an Electron-Ion Collider
Exploring the fundamental properties of matter with an Electron-Ion Collider Jianwei Qiu Theory Center, Jefferson Lab Acknowledgement: Much of the physics presented here are based on the work of EIC White Paper Writing Committee put together by BNL and JLab managements, … Eternal Questions People have long asked Where did we come from? The Big Bang theory? What is the world made of? Basic building blocks? What holds it together? Fundamental forces? Where are we going to? The future? Where did we come from? Can we go back in time or recreate the condition of early universe? Going back in time? Expansion of the universe Little Bang in the Laboratory Create a matter (QGP) with similar temperature and energy density BNL - RHIC CERN - LHC Gold - Gold Lead - Lead Relativistic heavy-ion collisions – the little bang q A virtual Journey of Visible Matter: Lorentz Near Quark-gluon Seen contraction collision plasma Hadronization Freeze-out in the detector q Discoveries – Properties of QGP: ² A nearly perfect quantum fluid – NOT a gas! at 4 trillion degrees Celsius, Not, at 10-5 K like 6Li q Questions: ² How the observed particles were emerged (after collision)? Properties of ² Does the initial condition matter (before collision)? visible matter What the world is made of? Human is only a tiny part of the universe But, human is exploring the whole universe! What hold it together? q Science and technology: Particle & Nuclear Physics Nucleon: Proton, or Neutron Nucleon – building block of all atomic matter q Our understanding of the nucleon evolves 1970s