The Impact of the Sakata Model
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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. -
The Eightfold Way Model, the SU(3)-flavour Model and the Medium-Strong Interaction
The Eightfold Way model, the SU(3)-flavour model and the medium-strong interaction Syed Afsar Abbas Jafar Sadiq Research Institute AzimGreenHome, NewSirSyed Nagar, Aligarh - 202002, India (e-mail : [email protected]) Abstract Lack of any baryon number in the Eightfold Way model, and its intrin- sic presence in the SU(3)-flavour model, has been a puzzle since the genesis of these models in 1961-1964. In this paper we show that this is linked to the way that the adjoint representation is defined mathematically for a Lie algebra, and how it manifests itself as a physical representation. This forces us to distinguish between the global and the local charges and between the microscopic and the macroscopic models. As a bonus, a consistent under- standing of the hitherto mysterious medium-strong interaction is achieved. We also gain a new perspective on how confinement arises in Quantum Chro- modynamics. Keywords: Lie Groups, Lie Algegra, Jacobi Identity, adjoint represen- tation, Eightfold Way model, SU(3)-flavour model, quark model, symmetry breaking, mass formulae 1 The Eightfold Way model was proposed independently by Gell-Mann and Ne’eman in 1961, but was very quickly transformed into the the SU(3)- flavour model ( as known to us at present ) in 1964 [1]. We revisit these models and look into the origin of the Eightfold Way model and try to un- derstand as to how it is related to the SU(3)-flavour model. This allows us to have a fresh perspective of the mysterious medium-strong interaction [2], which still remains an unresolved problem in the theory of the strong interaction [1,2,3]. -
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. -
Sakata Model Precursor 2: Eightfold Way, Discovery of Ω- Quark Model: First Three Quarks A
Introduction to Elementary Particle Physics. Note 20 Page 1 of 17 THREE QUARKS: u, d, s Precursor 1: Sakata Model Precursor 2: Eightfold Way, Discovery of ΩΩΩ- Quark Model: first three quarks and three colors Search for free quarks Static evidence for quarks: baryon magnetic moments Early dynamic evidence: - πππN and pN cross sections - R= σσσee →→→ hadrons / σσσee →→→ µµµµµµ - Deep Inelastic Scattering (DIS) and partons - Jets Introduction to Elementary Particle Physics. Note 20 Page 2 of 17 Sakata Model 1956 Sakata extended the Fermi-Yang idea of treating pions as nucleon-antinucleon bound states, e.g. π+ = (p n) All mesons, baryons and their resonances are made of p, n, Λ and their antiparticles: Mesons (B=0): Note that there are three diagonal states, pp, nn, ΛΛ. p n Λ Therefore, there should be 3 independent states, three neutral mesons: π0 = ( pp - nn ) / √2 with isospin I=1 - - p ? π K X0 = ( pp + nn ) / √2 with isospin I=0 0 ΛΛ n π+ ? K0 Y = with isospin I=0 Or the last two can be mixed again… + 0 Λ K K ? (Actually, later discovered η and η' resonances could be interpreted as such mixtures.) Baryons (B=1): S=-1 Σ+ = ( Λ p n) Σ0 = ( Λ n n) mixed with ( Λ p p) what is the orthogonal mixture? Σ- = ( Λ n p) S=-2 Ξ- = ( Λ Λp) Ξ- = ( Λ Λn) S=-3 NOT possible Resonances (B=1): ∆++ = (p p n) ∆+ = (p n n) mixed with (p p p) what is the orthogonal mixture? ∆0 = (n n n) mixed with (n p p) what is the orthogonal mixture? ∆- = (n n p) Sakata Model was the first attempt to come up with some plausible internal structure that would allow systemizing the emerging zoo of hadrons. -
An Introduction to the Quark Model Arxiv:1205.4326V2 [Hep-Ph]
An introduction to the quark model Jean-Marc Richard Université de Lyon & Institut de Physique Nucléaire de Lyon IN2P3-CNRS & UCB, 4 rue Enrico Fermi, 69622 Villeurbanne, France [email protected] May 25, 2012 Abstract This document contains a review on the quark model, prepared for lectures at the Niccolò Cabeo School at Ferrara in May 2012. It includes some historical aspects, the spectral properties of the 2-body and 3-body Schrödinger operators applied to mesons and baryons, the link between meson and baryon spectra, the role of flavour independence, and the speculations about stable or metastable multiquarks. The analogies between few-charge systems and few-quark bound states will be under- lined. Contents 1 Prelude: few charge systems in atomic physics 3 1.1 Introduction . .3 1.2 The atomic two-body problem . .3 1.3 Three-unit-charge ions . .5 arXiv:1205.4326v2 [hep-ph] 24 May 2012 1.4 Three-body exotic ions . .5 1.5 Molecules with four unit charges . .6 2 A brief historical survey 7 2.1 Prehistory . .7 2.2 Early hadrons . .7 2.3 Generalised isospin . .9 2.4 The success of the eightfold way . 10 2.5 The fundamental representation: quarks . 10 2.6 The OZI rule . 12 2.7 First quark models . 13 2.8 Heavy quarks . 14 2.9 Confirmation . 15 1 2 AN INTRODUCTION TO THE QUARK MODEL 3 The quark–antiquark model of mesons 16 3.1 Introduction . 16 3.2 Quantum numbers . 16 3.3 Spin averaged spectrum . 17 3.4 Improvements to the potential . -
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. -
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. -
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. -
With Toshihide Maskawa Interviewer: Shigeki Sugimoto
IPMU Interview with Toshihide Maskawa Interviewer: Shigeki Sugimoto 1 My rst paper was a Ph.D. Professor Sakata’s group. thesis There I was often teased about Sugimoto How are you? First behaving as if I were some I’d like to ask kind of big shot, even though your graduate I hadn’t written any papers. student days. (Laughs). Actually, my rst Maskawa Well, paper was my doctoral thesis. during those days at Once Yoichi Iwasaki2 came Nagoya University, to Nagoya with the intention graduate students who of observing us because he were theoretically oriented thought people from the were not assigned to any Nagoya group were standing particular group. Instead, they out and attracting his interest went around different theory in places like summer school. groups during the rst year Unfortunately, we were very or so. By the time they were busy at that time preparing about ready to write their for things like the Beijing master’s theses, they were Symposium, a student version assigned to the groups of of the Japan-China Academic their choice. Anyway, I joined Exchange Program, and for summer school. So, poor Toshihide Maskawa was awarded Iwasaki had to go back after the 2008 Nobel Prize in Physics having hardly any discussion jointly with Makoto Kobayashi for “the discovery of the origin of the with us. Subsequently, broken symmetry which predicts the 3 existence of at least three families Professor Shoichiro Otsuki of quarks in nature,” or, for the gave us a good scolding. “Kobayashi-Maskawa theory” of CP violation. He has also received He said that he was really many other distinguished awards, in particular the 1985 Japan Academy ashamed of us, as we had Prize and the 2008 Order of Cultural missed the opportunity to talk Merit. -
On the Wave Equation of Meson. Mitsuo TAKETANI And
On the Wave Equation of Meson. Mitsuo TAKETANIand Shoichi SAKATA. (Read April4,and July 13, 1940). Introduction. Up to the present much work on meson theory has. been done by considering it as a field theory, and the equation of meson as a field equation. This situation has its origin in the fact that the meson was found originally as a field of the heavy particles. However, if we re- strict ourselves to the problems of the interaction between the meson and the electromagnetic field, it seems more adequate to treat the meson equation in the form of a wave equation just like the cases of other charged particles(1), i.e. electron, positron and proton. Using the usual field equation for the meson as a wave equation, Laporte(2) has developed this stand point and calculated the elastic scattering of meson by a static electric field as a one body problem. The authors themselves, when they were engaging in the establish- ment of the vector meson theory, tried to write the meson equation in the form analogous to Dirac's electron equation. But before they could finish this task, certain circumstances prevented one of the authors (M. T.) from working in this problem and in the meantime Duffin's(3) paper appeared. Recently an important development of Duffin's theory was carried out by Kemmer(4). The authors have investigated in this paper in I some properties of Duffin's equation and in II developed the perturbation theory ana- logous to the case of Dirac electron, and finally in III with some restriction they were able to reduce the representation of Duffin's matrix ring from 10-rowed matrices to 6-rowed, and removed some (1) Kemmer's reasoning(4) for a particle theory of the meson, however, seems to be inadequate from the epistemological point of view, because it is to be noted that, contrary to Kemmer's statement, the meson was found originaly as a field and later as a particle, just as, in the case of electromagnetic field, the Coulomb field was found first and then the photon.