Murray Gell-Mann (1929–2019) and the Story of Strong Interactions∗
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Nucleon Resonances and Quark Structure
Nucleon Resonances and Quark Structure J.T. Londergan Physics Dept and Nuclear Theory Center, Indiana University, Bloomington, IN 47405, USA. [email protected] (Dated: October 25, 2018) A pedagogical review of the past 50 years of study of resonances, leading to our understanding of the quark content of baryons and mesons. The level of this review is intended for undergraduates or first-year graduate students. Topics covered include: the quark structure of the proton as revealed through deep inelastic scattering; structure functions and what they reveal about proton structure; and prospects for further studies with new and upgraded facilities, particularly a proposed electron- ion collider. Keywords: I. INTRODUCTION These lectures were given at Aligarh Muslim University, Aligarh India, at a nuclear physics workshop attended by Indian graduate students and postdocs. These lectures provide a pedagogical review of the past 50 years of experimental and theoretical studies of the quark and gluon structure of the nucleon. Since many speakers at this workshop will discuss structure functions extracted from deep inelastic scattering reactions, we define these quantities and review what can be extracted from them. We hope that specialists in this field will tolerate our brief and superficial summary of many years' study of strongly-interacting systems. FIG. 1: Richard H. Dalitz, 1925-2006. arXiv:0907.3431v1 [hep-ph] 20 Jul 2009 These lectures are dedicated to my mentor, Richard Dalitz, who was from 1963-2000 Royal Society Professor of Physics at Oxford University and who made seminal contributions in particle phenomenology. Dalitz pairs (electron- positron pairs from decay of a high-energy photon) and the Dalitz plot were named after him. -
Quantum Mechanics Quantum Chromodynamics (QCD)
Quantum Mechanics_quantum chromodynamics (QCD) In theoretical physics, quantum chromodynamics (QCD) is a theory ofstrong interactions, a fundamental forcedescribing the interactions between quarksand gluons which make up hadrons such as the proton, neutron and pion. QCD is a type of Quantum field theory called a non- abelian gauge theory with symmetry group SU(3). The QCD analog of electric charge is a property called 'color'. Gluons are the force carrier of the theory, like photons are for the electromagnetic force in quantum electrodynamics. The theory is an important part of the Standard Model of Particle physics. A huge body of experimental evidence for QCD has been gathered over the years. QCD enjoys two peculiar properties: Confinement, which means that the force between quarks does not diminish as they are separated. Because of this, when you do split the quark the energy is enough to create another quark thus creating another quark pair; they are forever bound into hadrons such as theproton and the neutron or the pion and kaon. Although analytically unproven, confinement is widely believed to be true because it explains the consistent failure of free quark searches, and it is easy to demonstrate in lattice QCD. Asymptotic freedom, which means that in very high-energy reactions, quarks and gluons interact very weakly creating a quark–gluon plasma. This prediction of QCD was first discovered in the early 1970s by David Politzer and by Frank Wilczek and David Gross. For this work they were awarded the 2004 Nobel Prize in Physics. There is no known phase-transition line separating these two properties; confinement is dominant in low-energy scales but, as energy increases, asymptotic freedom becomes dominant. -
Scaling Laws in Particle Physics and Astrophysics
SCALING LAWS IN PARTICLE PHYSICS AND ASTROPHYSICS RUDOLF MURADYAN Dedicated to the Golden Jubilee (1961-2011) of publication of the article by Geoffrey Chew and Steven Frautschi in Phys. Rev. Lett. 7, 394, 1961, where a celebrated scaling law J m2 has been conjectured for spin/mass dependence of hadrons. G. Chew S. Frautschi 1. INTRODUCTION: WHAT IS SCALING? Any polynomial power law f() x c xn , where constant c has a dimension dim f dimc (dimx )n exhibits the property of scaling or scale invariance. Usually n is called scaling exponent. The word scaling express the fact that function f is shape-invariant with respect to the dilatation transformation x x f ( x) c ( x)n n f() x and this transformation preserves the shape of function f . We say, following Leonhard Euler, that f is homogeneous of degree “n” if for any value of parameter f ( x) n f() x . Differentiating this relation with respect to and putting 1we obtain simple differential equation x f() x n f() x solution of which brings back to the polynomial power scaling law. There are tremendously many different scaling laws in Nature. The most important of them can be revealed by Google search of scaling site:nobelprize.org in the official site of Nobel Foundation, where nearly 100 results appears. Ten of them are shown below: 1. Jerome I. Friedman - Nobel Lecture 2. Daniel C. Tsui - Nobel Lecture 3. Gerardus 't Hooft - Nobel Lecture 4. Henry W. Kendall - Nobel Lecture 5. Pierre-Gilles de Gennes - Nobel Lecture 6. Jack Steinberger - Nobel Lecture 7. -
Nobel Lecture by Toshihide Maskawa
WHAT DOES CP VIOLATION TELL US? Nobel Lecture, December 8, 2008 by Toshihide Maskawa Kyoto Sangyo University, Kyoto 603-8555, Japan. I would first like to thank the Royal Swedish Academy of Sciences and the Nobel Foundation for awarding me this honour, of which I had never even dreamt. I was born in 1940, the son of a furniture craftsman in the city of Nagoya, in Japan. My father wanted to change his job and was taking a correspondence course to become an electrical engineer, while he was a trainee furniture craftsman. However, he told me that he could not really understand sine and cosine, since he had not received a basic education. Eventually, though, he did manage a small furniture factory employing a few craftsmen and worked there himself. But this came to nothing because of the War, that reckless and miserable war which our country caused. After the War, he displayed in front of his house the door hinges, wood screws and other pieces of furniture, which remained at hand. They sold quite well. Getting a taste for selling, he became a merchant dealing with sugar as an ingredient for cakes. He still wanted to boast of his knowledge of electricity, but he could not find anyone suitable to explain it to. One day, though, he found a good tar- get: his son. In those poor days after the war, almost all the houses were without bath- rooms and so people went to the public bath. On his way to and from the public bath, he boasted of his knowledge: Why do three-phase current mo- tors rotate? Why don’t the solar and lunar eclipses occur every month? He explained proudly that it was because of the revolution planes of the earth around the sun, and of the moon around the earth, which are tilted at an angle of 5 degrees. -
Fellowships for US Lab Directors
CCEMarFACES33-38 14/2/06 12:21 Page 33 FACES AND PLACES AWARDS Fellowships for US lab directors Two associate directors of US particle-physics laboratories were among the members of the American Association for the Advancement of Science (AAAS) to receive awards as new fellows at the 2006 AAAS Annual Meeting in St Louis, Missouri, on 18 February. They join other leading figures in US particle physics and related fields that were elected as new fellows by the AAAS Council during 2005. Swapan Chattopadhyay, associate director for accelerators at the Thomas Jefferson National Accelerator Facility (Jefferson Lab), was awarded the distinction of fellow for his “fundamental contributions to accelerator science, including phase-space cooling, innovative collider designs and pioneering Swapan Chattopadhyay, left, and Samuel Aronson, received AAAS fellowships in February. femto-sources, and for mentoring accelerator scientists at facilities worldwide, especially in Accelerator Department, the Physics professor at the University of Chicago, was developing countries”. He is responsible for Department, the Superconducting Magnet honoured “for his exceptional research in the all aspects of Jefferson Lab’s accelerator and Division, the Instrumentation Division and the evolution of the earliest universe, explaining Free-Electron Laser (FEL) programmes, Center for Accelerator Physics. its significance to the public, and for including R&D and operations, maintenance Neil V Baggett, advisor for planning and co-founding the interdisciplinary field of and upgrades of the Continuous Electron communication in the high-energy physics particle physics and cosmology”. Beam Accelerator Facility and the FEL. programme of the Office of Science of the US Lastly, C W Francis Everitt, research professor Samuel Aronson, associate laboratory Department of Energy, was also elected as a at the Hansen Experimental Physics Laboratory director for high-energy and nuclear physics fellow. -
UK News from CERN Issue 17: 26 March 2013
UK news from CERN Issue 17: 26 March 2013 In this issue: LHCb’s extra dimension – seeing data in a different way An holistic approach to improving accelerator performance Educating the united nations – maintaining continuity and broadening horizons Northern Ireland Assembly visits CERN Dates for the diary LHCb’s extra dimension Precision is key. LHCb provides the opportunity Predictability can be both reassuring, and a bit for unprecedented precision – it is a detector dull. For physicists at CERN, the Standard especially built for exploiting the vast number of Model of particle physics is like a jigsaw into b and c quarks (heavy cousins of the ‘everyday’ which they are gradually fitting pieces. Some quarks you find inside protons and neutrons) pieces seem to be fitting – measurements of the produced at the LHC, which are ideal for these Higgs boson seem to be pointing towards a precision measurements. Higgs that fits beautifully. But most physicists prefer living life on the edge, and they are The b and c quarks produced in LHCb collisions hoping to find pieces that just won’t fit. This associate with other quarks to form various would mean that the Standard Model isn’t right. types of short-lived particles that decay in a And it would force a radical (and exciting) number of ways; two-body, three-body or four- rethink; one that could lead to a theory that body, with the name relating to the number of answers questions that the Standard Model pieces of particle debris produced in the leaves open. For example, why there is only explosion. -
Arxiv:Hep-Ph/0703178V1 16 Mar 2007 Eta Eorn Huddcyt Htn I H Following the Via Photons to Decay Should S Mesotrons Force
FERMILAB-CONF-07-48-T Mesotron Decays and the Role of Anomalies William A. Bardeen Theoretical Physics Department Fermilab, MS 106, P.O. Box 500 Batavia, IL 60510, USA March 15, 2007 Puzzles associated with Yukawa’s mesotron theory of nuclear interactions led to the dis- covery of “anomalies” in quantum field theory. I will discuss some of the remarkable conse- quences of these anomalies in the physics of elementary particles. In 1935 Hideki Yukawa postulated that nuclear forces were ascribed to a new massive scalar field that coupled to neutrons to protons. To explain the saturation of the nuclear forces, the new mesotrons were required to have a mass of order 200 me, and a coupling a few times larger than that associated with the electric charge. The terms mesotron was used to describe a particle of intermediate mass, much heavier than the light electron and much lighter than the neutron and proton, the constituents of the atomic nucleus. Indeed, in 1937, a new meson of intermediate mass was discovered as the dominant part of the hard component of cosmic rays. It was natural to associate this meson with the field that Yukawa had proposed to explain the nuclear force. Shoichi Sakata played an important role in the struggle to understand the physics of the new Yukawa mesotrons and their relation to the new mesons seen in cosmic rays. arXiv:hep-ph/0703178v1 16 Mar 2007 Early estimates of the lifetime of the mesotron were based on Fermi’s theory of β-decay. These estimates, in the range of 10−8 to 10−7 sec, were considerably shorter than the lifetime observed for the cosmic ray mesons, ∼2 10−6 sec. -
People and Things
People and things Jean-Pierre Gourber will be Leader of the Miguel Virasoro becomes Director of the CERN's new LHC Division for three years from International Centre for Theoretical Physics 1 January 1996. (ICTP), Trieste. CERN elections and appointments A t its meeting on 23 June, XI CERN's governing body, the Council, decided to create an LHC Division as from 1 January 1996. The LHC Division will focus on the core activities related to the construction of the machine, namely supercon ducting magnets, cryogenics and vacuum together with supporting activities. Jean-Pierre Gourber was appointed Leader of the new LHC Division for three years from 1 January 1996. Council also appointed Bo Angerth as Leader of Personnel Division for three years from 1 January 1996, succeeding Willem Middelkoop. Jiri Niederle (Czech Republic) was elected Vice-President of Council for one year from 1 July 1995. tion, demonstrated that the gluons of EPS Prizes the strong interactions were a physi cal reality. The prestigious High Energy and The existence of such three-jet Particle Physics Prize of the Euro events in electron-positron collisions pean Physical Society for 1995 goes had been predicted in a pioneer to Paul Soding, Bjorn Wiik and ICTP Trieste Director CERN Theory Division paper by John Gunter Wolf of DESY and Sau Lan Ellis, Mary K. Gaillard and Graham Distinguished theorist Miguel Wu of Wisconsin for their milestone Ross. work in providing 'first evidence for Virasoro becomes Director of the There has always been keen rivalry three-jet events in electron-positron International Centre for Theoretical between the four 1979 PETRA colla collisions at PETRA' (DESY's elec Physics (ICTP), Trieste, succeeding borations - JADE, MARK-J, PLUTO tron-positron collider). -
Neutrino Mass and Mixing – the Beginning and Future –
Nuclear Physics B Proceedings Supplement Nuclear Physics B Proceedings Supplement 00 (2012) 1–4 Neutrino mass and mixing – The beginning and future – M. Kobayashi High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan Abstract The early history of neutrino mixing will be discussed with a focus on the birth of the MNS theory. Keywords: two neutrinos, MNS matrix 1. Sakata Model Another important aspect of the Sakata model is the fact that the weak interactions of hadrons can be ex- The first evidence of strange particles was found in plained by two types of transitions among the funda- cosmic ray events in 1947. Much progress in under- mental triplets: standing these particles was made in the early 1950’s, in particular after the operation of accelerators started. p The discovery of strange particles made it difficult to ↑↓-& . (1) regard all of the known hadrons as fundamental objects n Λ since there were so many. This pattern of the weak interaction is similar to the In 1956, Sakata proposed a model known as the weak interaction of the leptons, Sakata model [1], in which all the hadrons, both strange and non-strange, are composite states of a fundamental ν triplet formed from the proton, the neutron, and the Λ ↑↓-& . (2) particle. e µ Shoichi Sakata was born in 1911. He was a collabora- tor of Yukawa for some time. He was appointed profes- At that time the neutrino was thought to consist of a sor of Nagoya University when its physics department single species. This similarity of the weak interaction was established in 1942. -
Dalitz Analyses: a Tool for Physics Within and Beyond the Standard
DCPT/06/112 IPPP/06/56 DALITZ ANALYSES: A TOOL FOR PHYSICS WITHIN AND BEYOND THE STANDARD MODEL M.R. PENNINGTON Institute for Particle Physics Phenomenology, Durham University, Durham DH1 3LE, United Kingdom Abstract Dalitz analyses are introduced as the method for studying hadronic decays. An accurate description of hadron final states is critical not only to an understanding of the strong coupling regime of QCD, but also to the precision extraction of CKM matrix elements. The relation of such final state interactions to scattering processes is discussed. 1 Motivation This serves as the introduction to following talks on Dalitz plot analyses. I will first remind arXiv:hep-ph/0608016v1 2 Aug 2006 you of the motivation for such analyses and discuss some aspects of how to perform them and I leave it to others to describe detailed results. We know that there is physics beyond the Standard Model but we do not yet know what this is. Insight is provided by precision measurements of the CKM matrix elements, and in particular the length of the sides and the angles of the CKM Unitarity triangle. Such measurements in heavy flavour decays probe the structure of the weak interaction at distance scales of 0.01fm. However, the detector centimetres away records mainly pions and kaons as the outcome of a typical process like B → D(→ Kππ)K decay. Consequently, the very short distance interaction we wish to study is only seen through a fog of strong interactions, in which the quarks that are created exchange gluons, bind to form hadrons and then these hadrons interact for times a 100 times longer than the basic weak interaction. -
The Eightfold
THE EIGHTFOLD WAY 1 Jonathan L. Rosner The Eightfold Way is the name coined by Murray Gell-Mann (1961) to de- scribe a classification scheme of the elementary particles devised by him and Yuval Ne’eman (1961). The name, adopted from the Eightfold Path of Bud- dhism, refers to the eight-member families to which many sets of particle belong. In the 1950s Gell-Mann and Kazuo Nishijima invented a scheme to explain a “strange” feature of certain particles; they appeared to be easily produced in cosmic-ray and accelerator reactions, but decayed slowly, as if something were hindering their decays. These particles were assumed to carry a property known as strangeness which would be preserved in production but could be changed in decays. Two examples of plots of electric charge (in units of the fundamental charge |e|) versus strangeness for particles known in the late 1950s are the following: Mesons: Baryons: Strangeness: Particle: Strangeness: Particle: 1 K0 K+ 0 n p 0 π− π0 π+ −1 Σ− Σ0, Λ Σ+ −1 K− K¯ 0 −2 Ξ− Ξ0 arXiv:hep-ph/0109241v2 15 Oct 2001 Charge: −1 0 1 Charge: −1 0 1 Mesons include the π particles, known as pions, whose existence was pro- posed by Hideki Yukawa in 1935 to explain the strong nuclear force, and the K particles (also known as kaons), discovered in cosmic radiation in the 1940s. Pions and kaons weigh about one-seventh and one-half as much as protons, re- spectively. Baryons (the prefix bary- is Greek for heavy) include the proton p, the neutron n, and heavier relatives Λ (lambda), Σ (sigma), and Ξ (xi), collec- tively known as hyperons and discovered in the 1940s and 1950s. -
Where Is the New Physics at the LHC ?
Where is the new physics at the LHC ? M. E. Peskin Sakata100, Nagoya October, 2011 I am honored to be invited to lecture at the celebration of the 100th birthday of Shoichi Sakata. My topic will be the current state of searches for new physics beyond the Standard Model at the LHC. I hope to discuss this topic in the spirit of Sakata, in a sense that I will explain. Sakata, Ohnuki, and Maki in Nagoya Morris Low Nagoya 2006 No signs of new physics have turned up yet at the LHC. Not everyone considers this to be a problem, but many people are impatient. There are good reasons to be impatient, which I will explain later. I add that the press is impatient, and eager to say that the theorists have it wrong ... New York Times (Claudia Dreyfus) interview with Stephen Hawking May 9, 2011 (w. public LHC results from 0.04 fb-1/experiment) Q. About the Large Hadron Collider, the supercollider in Switzerland, there were such high hopes for it when it was opened. Are you disappointed in it? A. It is too early to know what the LHC will reveal. It will be two years before it reaches full power. When it does, it will work at energies five times greater than previous particle accelerators. We can guess at what this will reveal, but our experience has been that when we open up a new range of observations, we often find what we had not expected. That is when physics becomes really exciting, because we are learning something new about the universe.