The Eightfold Way Model, the SU(3)-flavour Model and the Medium-Strong Interaction
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The Eightfold Way John C
The Eightfold Way John C. Baez, May 27 2003 It is natural to group the eight lightest mesons into 4 irreps of isospin SU(2) as follows: mesons I3 Y Q pions (complexified adjoint rep) π+ +1 0 +1 π0 0 0 0 π− -1 0 -1 kaons (defining rep) K+ +1/2 1 +1 K0 -1/2 1 0 antikaons (dual of defining rep) K0 +1/2 -1 0 K− -1/2 -1 -1 eta (trivial rep) η 0 0 0 (The dual of the defining rep of SU(2) is isomorphic to the defining rep, but it's always nice to think of antiparticles as living in the dual of the rep that the corresponding particles live in, so above I have said that the antikaons live in the dual of the defining rep.) In his theory called the Eightfold Way, Gell-Mann showed that these eight mesons could be thought of as a basis for the the complexified adjoint rep of SU(3) | that is, its rep on the 8- dimensional complex Hilbert space su(3) C = sl(3; C): ⊗ ∼ He took seriously the fact that 3 3 sl(3; C) C[3] = C (C )∗ ⊂ ∼ ⊗ 3 3 where C is the defining rep of SU(3) and (C )∗ is its dual. Thus, he postulated particles called quarks forming the standard basis of C3: 1 0 0 u = 0 0 1 ; d = 0 1 1 ; s = 0 0 1 ; @ 0 A @ 0 A @ 1 A 3 and antiquarks forming the dual basis of (C )∗: u = 1 0 0 ; d = 0 1 0 ; s = 0 0 1 : This let him think of the eight mesons as being built from quarks and antiquarks. -
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 . -
PARTICLE DECAYS the First Kaons from the New DAFNE Phi-Meson
PARTICLE DECAYS K for KLi The first kaons from the new DAFNE phi-meson factory at Frascati underline a fascinating chapter in the evolution of particle physics. As reported in the June issue (p7), in mid-April the new DAFNE phi-meson factory at Frascati began operation, with the KLOE detector looking at the physics. The DAFNE electron-positron collider operates at a total collision energy of 1020 MeV, the mass of the phi- meson, which prefers to decay into pairs of kaons.These decays provide a new stage to investigate CP violation, the subtle asymmetry that distinguishes between mat ter and antimatter. More knowledge of CP violation is the key to an increased understanding of both elemen tary particles and Big Bang cosmology. Since the discovery of CP violation in 1964, neutral kaons have been the classic scenario for CP violation, produced as secondary beams from accelerators. This is now changing as new CP violation scenarios open up with B particles, containing the fifth quark - "beauty", "bottom" or simply "b" (June p22). Although still on the neutral kaon beat, DAFNE offers attractive new experimental possibilities. Kaons pro duced via electron-positron annihilation are pure and uncontaminated by background, and having two kaons produced coherently opens up a new sector of preci sion kaon interferometry.The data are eagerly awaited. Strange decay At first sight the fact that the phi prefers to decay into pairs of kaons seems strange. The phi (1020 MeV) is only slightly heavier than a pair of neutral kaons (498 MeV each), and kinematically this decay is very constrained. -
(Max Planck Institute Für Physik) 1St Lecture
QCD Giulia Zanderighi (Max Planck Institute für Physik) 1st Lecture ESHEP School September 2019 Today’s high energy colliders Today’s high energy physics program relies mainly on results from Today’s high energy colliders Collider Process Today’s high statusenergy colliders + T-oday’s high energy colliders Collider LEP/LEP2Process setaetus Today’s high1989-2000energy colliders Today’s chighurrenenergyt and ucpolliderscoming ex- Hera e±p Today’s high1992-2007energy colliders HERCAoll(idAe&r B) Preo±cpess rsutanntuinsg periments collide protons Collider TevatronProcess statupps curre1983-2011nt and upcoming ex- Collider Process status current and upcoming ex- THeERvCaotrlAloidn(eAr(I&&B)II) Proceep±sp¯sp startuunsning cpuerrrimenetntsancdolluidpecopmroitongnsex- HERA (A & B)LHC-e ±Runp I runninppg cpuerrrimenetntsa2010-2012ncadolllluidipnecvopomrolvitonegnQseCDx- Collider Process status THeERvatrALoHn(AC(I&&B)II) ep±p¯p starurtsnn2in0g07 pe⇒riments collide protons THeERvatrAon(A(I&&B)II) ep±p¯p running perimcuernretsnctolalinded puroptoconms ing ex- LHC- Run II pp astartedll inavlloilnv 2015evoQlvCDe QCD THeERvatrALoHn(AC(I&&B)II) ep±p¯p starurtsnn2in0g07 pe⇒riments collide protons TevatrLoHnC(I & II) pp¯ starurtsnn2in0g07 ⇒ all involve QCD LEPHER highA: m precisionainly mea measurementssurements of pa ofrto masses,n denaslilti couplings,iensvaonlvdedQiffr CDEWacti oparametersn ... TevaLtrHLoHCnC(I & II) pppp¯ stasrtstarur2tsn0n02i7n0g07 ⇒ ⇒ Hera: mainly measurements of proton structureal l/ inpartonvolve densitiesQCD HTHEReERLvA:HatrA:Cmonma:inamliynalmyinemlyaesdpuaipsrsecumoreveemnrtseysntaotsffrptsthoafer2top0toan0rp7todaennsddietirene⇒sslaiatitenedds -
Chapter 16 Constituent Quark Model
Chapter 16 Constituent Quark Model 1 Quarks are fundamental spin- 2 particles from which all hadrons are made up. Baryons consist of three quarks, whereas mesons consist of a quark and an anti-quark. There are six 2 types of quarks called “flavours”. The electric charges of the quarks take the value + 3 or 1 (in units of the magnitude of the electron charge). − 3 2 Symbol Flavour Electric charge (e) Isospin I3 Mass Gev /c 2 1 1 u up + 3 2 + 2 0.33 1 1 1 ≈ d down 3 2 2 0.33 − 2 − ≈ c charm + 3 0 0 1.5 1 ≈ s strange 3 0 0 0.5 − 2 ≈ t top + 3 0 0 172 1 ≈ b bottom 0 0 4.5 − 3 ≈ These quarks all have antiparticles which have the same mass but opposite I3, electric charge and flavour (e.g. anti-strange, anti-charm, etc.) 16.1 Hadrons from u,d quarks and anti-quarks Baryons: 2 Baryon Quark content Spin Isospin I3 Mass Mev /c 1 1 1 p uud 2 2 + 2 938 n udd 1 1 1 940 2 2 − 2 ++ 3 3 3 ∆ uuu 2 2 + 2 1230 + 3 3 1 ∆ uud 2 2 + 2 1230 0 3 3 1 ∆ udd 2 2 2 1230 3 3 − 3 ∆− ddd 1230 2 2 − 2 113 1 1 3 Three spin- 2 quarks can give a total spin of either 2 or 2 and these are the spins of the • baryons (for these ‘low-mass’ particles the orbital angular momentum of the quarks is zero - excited states of quarks with non-zero orbital angular momenta are also possible and in these cases the determination of the spins of the baryons is more complicated). -
The Quark Model
The Quark Model • Isospin Symmetry • Quark model and eightfold way • Baryon decuplet • Baryon octet • Quark spin and color • Baryon magnetic moments • Pseudoscalar mesons • Vector mesons • Other tests of the quark model • Mass relations and hyperfine splitting • EM mass differences and isospin symmetry • Heavy quark mesons • The top quarks • EXTRA – Group Theory of Multiplets J. Brau Physics 661, The Quark Model 1 Isospin Symmetry • The nuclear force of the neutron is nearly the same as the nuclear force of the proton • 1932 - Heisenberg - think of the proton and the neutron as two charge states of the nucleon • In analogy to spin, the nucleon has isospin 1/2 I3 = 1/2 proton I3 = -1/2 neutron Q = (I3 + 1/2) e • Isospin turns out to be a conserved quantity of the strong interaction J. Brau Physics 661, Space-Time Symmetries 2 Isospin Symmetry • The notion that the neutron and the proton might be two different states of the same particle (the nucleon) came from the near equality of the n-p, n-n, and p-p nuclear forces (once Coulomb effects were subtracted) • Within the quark model, we can think of this symmetry as being a symmetry between the u and d quarks: p = d u u I3 (u) = ½ n = d d u I3 (d) = -1/2 J. Brau Physics 661, Space-Time Symmetries 3 Isospin Symmetry • Example from the meson sector: – the pion (an isospin triplet, I=1) + π = ud (I3 = +1) - π = du (I3 = -1) 0 π = (dd - uu)/√2 (I3 = 0) The masses of the pions are similar, M (π±) = 140 MeV M (π0) = 135 MeV, reflecting the similar masses of the u and d quark J. -
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. -
1 Historical Introduction to the Elementary Particles
13 1 Historical Introduction to the Elementary Particles This chapter is a kind of ‘folk history’ of elementary particle physics. Its purpose is to provide a sense of how the various particles were first discovered, and how they fit into the overall scheme of things. Along the way some of the fundamental ideas that dominate elementary particle theory are explained. This material should be read quickly, as background to the rest of the book. (As history, the picture presented here is certainly misleading, for it sticks closely to the main track, ignoring the false starts and blind alleys that accompany the development of any science. That’s why I call it ‘folk’ history – it’s the way particle physicists like to remember the subject – a succession of brilliant insights and heroic triumphs unmarred by foolish mistakes, confusion, and frustration. It wasn’t really quite so easy.) 1.1 The Classical Era (1897–1932) It is a little artificial to pinpoint such things, but I’d say that elementary particle physics was born in 1897, with J. J. Thomson’s discovery of the electron [1]. (It is fashionable to carry the story all the way back to Democritus and the Greek atomists, but apart from a few suggestive words their metaphysical speculations have nothing in common with modern science, and although they may be of modest antiquarian interest, their genuine relevance is negligible.) Thomson knew that cathode rays emitted by a hot filament could be deflected by a magnet. This suggested that they carried electric charge; in fact, the direction of the curvature required that the charge be negative. -
Yucal Ne'eman and Murray Gell-Mann Physicists Welcomed The
Yucal Ne'eman and Murray Gell-Mann Physicists welcomed the news last month of and symmetric arrangement of many of the nearly the discovery of a subatomic particle which may 100 fundamental particles known today. It also bring some order out of the apparent chaos among provides a logical base for a naming system for nuclear particles. The omega-minus, discovered particles to replace the current colloquial names. by scientists working with the particle accelerator Though the names are still primarily Greek letters, at Brookhaven National Laboratory in New York, they now have more meaning. confirms a theory proposed independently, three As proposed, the eightfold way had a gap - an years ago, by Murray Gell-Mann, professor of unknown particle, conspicuous by its absence. To theoretical physics at Caltech; and Yuval Ne'eman fill this gap, a new particle, the omega-minus, was of Israel, now research fellow in theoretical phys- hypothesized. If the particle were to be discov- ics at Caltech. The theory relates nuclear particles ered, the gap would be filled and the Gell-Mann- to each other in a manner reminiscent of Mende- Ne'eman theory would be verified in one im- lyeev's periodic table of the elements. It sets up portant respect. "family relationships" between many of the strong- It was felt, moreover, that this verification ly interacting particles now known. (Strongly in- would make the eightfold way a certainty, since teracting particles are those subject to the force the properties prophesied for the omega-minus known, appropriately enough, as strong interac- were so unusual that they could not be predicted tion. -
NEUTRINOS and SAKATA Field Via Annihilation of V and V in Muon Decay Interaction If Ve 'Ij =V
-1- NAKAGAWA was to clsrify phenomenological consequences of the assumption ve 'iJ. They pointed out the occur.!nce of 1.1 - e conversion in Coulomb NEUTRINOS AND SAKATA field via annihilation of v and v in muon decay interaction if ve 'iJ =v. and calculated the probability for one electron decay of mu -A Personal View- mesic atom in K-orbit and the probability for muon scattering under Coulomb field of nucleus associated by 1.1 ~ e conversion. Masami Nakagawa DeparCllent of Physics. Keijo University, Nagoya 468, Japan A CRITIQUE (1955) This conference. a workshop for the neutrino mass. is to require In 1955 Sakata wrote a paper3 in Japanese with a shocking title real contributions to Today's and Future's problems on the neutrinos, 'Superstition around Majorana Neutrino'. He says it sbould not be so it ai&ht DDt be the place to mention past history. But it may, adequate to question whether a neutrino is a Dirac or Majorana part I beli_e. be worth presenting some historical review of researches icle in an alternative judgment. and it is nothing but a supersti on neutrinos in Japan. especially of those guided by the late Prof tion to believe that the answer to the question be obtained by expe- essor Sboichi Sakata, since be had continuously been taking great riment of double beta decay and so on. His point is that such a leadership at least twenty years from the proposal of two meson-two question making the Majorana theory in sharp conflict with the Dirac n_Uino t~ry (1942) to the proposal of mixture theory of massive theory arises from choosing the interaction within unnecessarily a_trinos <1962/)*). -
Nuclear and Particle Physics
PHY401: Nuclear and Particle Physics Lecture 4, Monday, August 31, 2020 Dr. Anosh Joseph IISER Mohali Particles and Nuclei A Historical Introduction II PHY401: Nuclear and Particle Physics Dr. Anosh Joseph, IISER Mohali Neutrinos (1930 - 1962) Let’s go back to year 1930. Only 3 elementary particles were known to us at that time. Protons, neutrons, and electrons. Study of nuclear beta decay - gave an unusual puzzle. PHY401: Nuclear and Particle Physics Dr. Anosh Joseph, IISER Mohali Neutrinos (1930 - 1962) Beta decay: a radioactive nucleus A is transformed into a lighter nucleus B, with the emission of electron: A ! B + e-. (1) Charge conservation requires that B carry one more unit of positive charge than A. We now know that the underlying process here is the conversion of a neutron, in A, into a proton, in B. In 1930, the neutron had not yet been discovered. PHY401: Nuclear and Particle Physics Dr. Anosh Joseph, IISER Mohali Neutrinos (1930 - 1962) Neutron was discovered in 1932. Examples of beta decay: 40 40 19K −! 20Ca 64 64 29Cu −! 30Zn 3 3 1H −! 2He PHY401: Nuclear and Particle Physics Dr. Anosh Joseph, IISER Mohali Neutrinos (1930 - 1962) Upper number is atomic weight (number of neutrons + protons) Lower number is atomic number (number of protons) of the nucleus. In two-body decays (A ! B + C) outgoing energies are kinematically determined, in the center-of-mass frame. PHY401: Nuclear and Particle Physics Dr. Anosh Joseph, IISER Mohali Neutrinos (1930 - 1962) If ‘parent’ nucleus (A) is at rest, so that B and e come out back to back with equal and opposite momenta, ...then energy conservation dictates that electron energy is 2 2 2 mA - mB + me 2 Ee = c .