The Standard Theory of Elementary Particle Physics and Beyond

Similar documents
Quantum Field Theory. Ling-Fong Li. (Institute) Quark Model 1 / 14

January 31, PHY357 Lecture 8. Quark composition of hadrons. Hadron magnetic moments. Hadron masses

Lecture 9 Valence Quark Model of Hadrons

The SU(3) Group SU(3) and Mesons Contents Quarks and Anti-quarks SU(3) and Baryons Masses and Symmetry Breaking Gell-Mann Okubo Mass Formulae Quark-Mo

Gian Gopal Particle Attributes Quantum Numbers 1

This means that n or p form a doublet under isospin transformation. Isospin invariance simply means that. [T i, H s ] = 0

Lecture 8. CPT theorem and CP violation

Notes on SU(3) and the Quark Model

Quark Model. Ling-Fong Li. (Institute) Note 8 1 / 26

The Quark Parton Model

Dr Victoria Martin, Prof Steve Playfer Spring Semester 2013

Lecture 9. Isospin The quark model

The Development of Particle Physics. Dr. Vitaly Kudryavtsev E45, Tel.:

Quark Model History and current status

wave functions PhD seminar- FZ Juelich, Feb 2013

Flavour physics Lecture 1

Clebsch-Gordan Coefficients

Quark model of hadrons and the SU(3) symmetry

SU(3) symmetry and Baryon wave functions

arxiv:hep-ph/ v3 15 Mar 2006

Lie Theory in Particle Physics

Particle Physics. Lecture 11: Mesons and Baryons

Quark Model. Mass and Charge Patterns in Hadrons. Spin-1/2 baryons: Nucleons: n: MeV; p: MeV

Problem Set # 1 SOLUTIONS

Kern- und Teilchenphysik I Lecture 13:Quarks and QCD

Symmetry Groups conservation law quantum numbers Gauge symmetries local bosons mediate the interaction Group Abelian Product of Groups simple

Particle Physics. Michaelmas Term 2009 Prof Mark Thomson. Handout 7 : Symmetries and the Quark Model. Introduction/Aims

Lecture notes Particle Physics II. Quantum Chromo Dynamics. 2. SU(2) and SU(3) Symmetry. Michiel Botje Nikhef, Science Park, Amsterdam

Discrete Transformations: Parity

Another view of the Gell-Mann-Okubo mass formula

Partners of the SU(3) hadrons

Standard Model & Beyond

Lecture 6 Isospin. What is Isospin? Rota4ons in Isospin space Reac4on rates Quarks and Isospin Heavier quarks FK

Part 7: Hadrons: quarks and color

Lecture 6 Isospin. What is Isospin? Rota4ons in Isospin space Reac4on rates Quarks and Isospin Gell- Mann- Nishijima formula FK

The Gauge Principle Contents Quantum Electrodynamics SU(N) Gauge Theory Global Gauge Transformations Local Gauge Transformations Dynamics of Field Ten

Weak interactions and vector bosons

CHAPTER II: The QCD Lagrangian

SU(3) systematization of baryons. Vadim Guzey. Theory Center, Jefferson Lab

Introduction to Quantum Chromodynamics (QCD)

Isospin. K.K. Gan L5: Isospin and Parity 1

Introduction to group theory and its representations and some applications to particle physics

Introduction to Gauge Theories

The Strong Interaction and LHC phenomenology

Quarks and hadrons. Chapter Quark flavor and color

QCD and Models : introduction

Quarks and hadrons. Chapter 7

Introduction to particle physics Lecture 4

Back to Gauge Symmetry. The Standard Model of Par0cle Physics

Quark Model of Hadrons

Introduction to particle physics Lecture 6

SU(N) representations

Mass Spectrum of a Baryon Octet is Linear

The Eightfold Way model, the SU(3)-flavour model and the medium-strong interaction

.! " # e " + $ e. have the same spin as electron neutrinos, and is ½ integer (fermions).

Electroweak interactions of quarks. Benoit Clément, Université Joseph Fourier/LPSC Grenoble

How nucleon gets its mass

arxiv:hep-ph/ v2 15 Oct 2001

PHYS 3446 Lecture #17

Particle Physics. Lecture 12: Hadron Decays.!Resonances!Heavy Meson and Baryons!Decays and Quantum numbers!ckm matrix

Discovery of Pions and Kaons in Cosmic Rays in 1947

Properties of the proton and neutron in the quark model

Hadron Physics & Quantum Chromodynamics Adnan Bashir, IFM, UMSNH, Mexico August 2013 Hermosillo Sonora

Gell-Mann Okubo Mass Formula for SU(4) Meson Hexadecuplet

THE STANDARD MODEL AND THE GENERALIZED COVARIANT DERIVATIVE

The hadronization into the octet of pseudoscalar mesons in terms of SU(N) gauge invariant Lagrangian

Λ QCD and Light Quarks Contents Symmetries of the QCD Lagrangian Chiral Symmetry and Its Breaking Parity and Handedness Parity Doubling Explicit Chira

Origin and Status of INSTANTONS

Kaons - A Micro-physics Laboratory Will you still need me when I m 64? (The Beatles)

Quark model. Jan 30, 2006 Lecture 8 1

PHYS 420: Astrophysics & Cosmology

July 10, Particle Physics I Physics G8069 Fall 2006

Le Modèle Standard et ses extensions

Astronomy, Astrophysics, and Cosmology

Homework 3: Group Theory and the Quark Model Due February 16

Adding families: GIM mechanism and CKM matrix

Lecture 3: Quarks and Symmetry in Quarks

Chapter 5 Theories and Lagrangians III: The Standard Model

Exotic Diquark Spectroscopy

The Heavy Quark Spin Symmetry and SU(3)-Flavour Partners of the X(3872)

Symmetries, Fields and Particles 2013 Solutions

Outline. Charged Leptonic Weak Interaction. Charged Weak Interactions of Quarks. Neutral Weak Interaction. Electroweak Unification

Evidence for the Strong Interaction

Part 6: Hadrons: quantum numbers and excited states

A.A. Godizov. Institute for High Energy Physics, Protvino, Russia

Kern- und Teilchenphysik II Lecture 1: QCD

The Quantum Chromodynamics Theory Of Quadruply Strange Pentaquarks

ON SOME MODELS OF THE EXOTIC HADRON STATES. Siniša R. Ignjatović and Vesna Borka Jovanović

Isospin: An Approximate Symmetry on the Quark Level

Physics 125 Course Notes Identical Particles Solutions to Problems F. Porter

η π 0 γγ decay in the three-flavor Nambu Jona-Lasinio model

OUTLINE. CHARGED LEPTONIC WEAK INTERACTION - Decay of the Muon - Decay of the Neutron - Decay of the Pion

Symmetries, Groups, and Conservation Laws

Particle Physics - Chapter 1 The static quark model

Examination paper for FY3403 Particle physics

DEEP INELASTIC SCATTERING

Electric Dipole Moments and the strong CP problem

Critical lines and points. in the. QCD phase diagram

Fundamental Particles and Forces

Symmetries, Fields and Particles 2013 Solutions

Transcription:

The Standard Theory of Elementary Particle Physics and Beyond An Introduction in (about) 20 lectures CINVESTAV, Mexico City, Mexico 10 February-2April, 2005 Luciano Maiani, Universita di Roma La Sapienza and INFN, Roma, Italy Lecture 8, March 3, 2005 1

5. QUARKS Quarks 1 Precursors The Eightfold way Fundamental triplets, mesons and baryons The naive (constituent) quark model Quarks 2 symmetries and currents symmetry breaking weak and electromagnetic currents Cabibbo theory The breaking of the chiral symmetry Quarks 3 GIM mechanism and the charmed quark Guessing the c-quark mass Charmed Mesons and baryons SU(2)xU(1) with two quark doublets Quarks 4 Quark masses A useful theorem The KM matrix Mixing and CP violation in B mesons 2

J. Letessier and J. Rafelski, Hadrons and Quark Gluon Plasma, Cambridge Monogr. Part. Phys. Nucl. Phys. Cosmol. 18 (2002). ρ( m ) = δ( m m ) i i NOTE: ρ tot = ρ( m ) + 3δ( m m π )

1. Precursors E. Fermi, C. N. Yang Are Mesons Elementary Particles? Phys. Rev. 76 (1949)1739. M. Gell-Mann: Symmetries of Baryons and Mesons, Phys. Rev. 125 (1962) 1067. The Fermi-Yang model: Baryons are fundamental, mesons are not N N interaction = repulsive, N-Nbar attractive, may form deeply bound states Lightest states: L=0 (S-wave) spin N-Nbar = 0 J PC = 0 -+ Isospin : 1/2 1/2 = 1 0 The 3 pions + a neutral particle - η(547)? Further states: L=0 (S-wave) Spin N-Nbar = 1 J PC = 1 -- Vector mesons : ρ(770), ω (782); in fact there is another one: φ(1020)?? A photon-like, fundamental vector field coupled to baryon number would make an attractive force for N-Nbar and a repulsive one for N-N. Gell-Mann calls it B. Tentative name: gluon (from glue) B cannot be massless like the photon. 4

Precursors (cont d) The Sakata Model p T = n Λ S. Sakata: On a composite model for the new particles, Progr. Theor. Phys. 16, 686, 1956. M. Gell-Mann: Symmetries of Baryons and Mesons, Phys. Rev. 125 (1962) 1067. Fundamental fields: T, Bµ Lagrangian: L = T[ i( µ g strong B µ )γ µ + M]T 1 4 B µν B µν + 1 2 µ2 B µ B µ B µν = µ B ν ν B µ Natural Symmetry: SU(3): T UT; U + U =1,det(U) =1 As in F&Y, an overall phase in U would be associated to baryon number conservation SU(3) symmetry is violated (at least!) by the unequal masses of the elements of T: (m p + m n -2m Λ ) 0: SU(3) SU(2) I U(1) S U(1) Q (~ 30%) (m p - m n ) 0: SU(2) I U(1) S U(1) I3 U(1) S (~ 0.1%) M = m p m n m Λ 5

Spectroscopy of the Sakata model: mesons T-Tbar states: SU(3) rep.= 8 1 L=0 (S-wave) Spin (T-Tbar) = 0 JPC= 0 -+ Pseudoscalar Mesons fit well (today!), including η (960) Spin(T-Tbar) = 1 J PC = 1 -- Vector Mesons fit well: ρ(770), ω (782), φ(1020), K* (892) The real problem are baryons. Simplest possibility for spin 1/2, B=1, is: (T-Tbar)T This formula entails the existence of baryons with S=+1 (K+N) but the K+N channel is flat, unlike K-N which presents several resonances. The baryon spectrum is a fatal blow for the model. Note: a K + N resonance may have been observed recently, Θ + (1540), but its relevance is anyway not comparable to that of the states Σ, Ξ, Y* 6

K - -p cross-section 7

K + -N cross-sections 8

The Eightfold Way M. Gell-Mann: Symmetries of Baryons and Mesons, Phys. Rev. 125 (1962) 1067. A strategic conversion: The symmetry SU(3) is suggested by the Sakata model as a (broken) symmetry of the strong interactions, which extends Isospin to include the strangeness degrees of freedom Can we find anyway a viable classification on baryons and mesons in SU(3)multiplets? can we describe the SU(3) breaking quantitatively? 9

Strangeness and the formula of Gell-Mann & Nishijima Hadrons make isospin multiplets, characterised by (I, I 3 ) and S; Q goes in steps of 1, like I 3, so we can put Q= I 3 + Y/2 Y is called hypercharge and is = 2<Q> (since <I 3 >=0) Y commutes with I, I 3, so it is a functions of the other conserved numbers, S and B Gell-Mann and Nishijima note that: Y = B + S so that: Q = I 3 + 1 (B + S) 2 Y is symmetrically distributed also for the stable baryons unlike S (recall S baryons 0) Y is a good candidate to be the second commuting generator in a symmetry group of rank two (I 3 e Y). 10

SU(3) generators Le 8 Gell-Mann matrices 0 ;λ 4 = 0 1 0 ;λ 5 = 0 i 0 ; 0 0 0 1 0 0 i 0 0 λ 1,2,3 = σ1,2,3 0 λ 6 = 0 0 1 ;λ = 0 0 7 i ;λ = 1 1 0 0 8 3 0 1 0 0 1 0 0 i 0 0 0 2 U = e i! a" a # a ; # a = 3 3, complex, hermitian; Tr(# a ) = 0 SU(3) SU(2) I U(1) Y λ 1,2,3 = I 1,2,3 ;λ 8 = Y [λ i,λ j ] = 2if ijk λ k (i, j,k =1,2...8) λ 0 = 2 3 1 {λ i,λ j } = 2d ijk λ k (i, j,k = 0,1,...8) f ijk = structure constants of the Lie algebra; completly antisymmetric; d ijk = completly symmetric; the numerical vlues are given in Gell-Mann s article. Tr(λ i λ j ) = 2δ ij Two fundamental reps (1) : 3, 3-bar: 3 and 3-bar are not equivalent (unlike SU(2) why?) dim of the Regular Rep. (2) = 8 (λ (3) ) α,β = [(λ (3) ) α,β ]* = (λ α,β ) * (1) we can construct all reps with their tensor products (2) the rep. which transforms like the generators themselves 11

Symmetry breaking We write the strong interaction Lagrangian (e=0, G=0): L strong = L sym + L sb in the Fermi-Yang-Sakata model, L sb is just due to the unequal masses: M = m p m n m Λ = m m 1 p n 2 M = m 0 λ 0 + m 8 λ 8 + m 3 λ 3 ; m T = (m p + m n + m Λ ) /3 1GeV L sb = T M p 0 0 0 M n 0 T 0 0 M! 1 + m + m 2m 1 p n Λ 6 0 Under SU(3), M transforms like a superposition of the diagonal components of an octet. Thus, neglecting isospin violation we are led to the octet hypothesis: L sb! 8 1 + m + m + m 1 p n Λ 3 2 1 1 12

Invariant Operations in SU(3) Vector of rep. 3 Vector of rep. 3-bar: Note: x i (Ux) i = U k i x k y i (U k i ) * y k = y k (U + ) i k = (yu + ) i y i x i (yu + Ux) = (yx) = in var iante That is : δ i j = invariant The second invariant operation: completly antisymmetric tensor: ε ijk U i i' U j j' U k k' ε i' j'k' = detuε ijk = ε ijk That is : ε ijk ( or ε ijk ) = invariant 13

The irreducible tensors (IT) 1) {i T(n,m) = T 1,i 2,...i n } {i,i { j1, j 2,..., j m };T 2,...i } n j { j, j2,..., j m } δ i = 0 2 quantum numbers: corrisponds to rank = 2 of SU(3) 2) T(n,0) T(0,m) = T(n,m) [T(n 1,0) T(0,m 1) dim(n,0) dim(0,m) = dim(n,m) + dim(n 1,0) dim(0,m 1) dim(n,m) = (n +1)(m +1)(n + m + 2) 2 Fundamental Reps. : (1,0)= 3 (0,1) = 3-bar Regular Rep.: (1,1)= 8 Decuplet: (3,0) = 10 Antidecuplet: (0,3)= 10-bar n=m : self conjugate rep. 14

Decomposition of 3, 8, 10 Isospin of u and d= +/- 1/2 Hypercharge of s=y Hypercharge of u and d = y+1 Trace(Y)=0 Y=-2/3 These quantum numbers fix the decomposition in isopin and hypercharge of the Irr. Tensors. 8 = x a x b - 1/3δ b a = (I=1, Y=0); (I=0, Y=0), (I=1/2,+1), (I=1/2, -1) 10 =Symm(x a x b x c )=(I=3/2, Y=1);(I=1, Y=0);(I=1/2, Y=-1); (I=0, Y=-2) Note: TrY=0 u(+1/2 1/ 3 ) x = d( 1/2 1/ 3 ) ; s(0 2 / 3 ) 15

S=Y +1 (497.7) Mesons: J PC =0 -+ Masses in MeV (493.7) (135.0) 0-1 (139.6) η' (547.3) (957.8) (139.6) (493.7) (497.7) -1-1/2 0 +1/2 +1 I 3 16

S=Y +1 K *0 K *+ (892) Mesons: J PC =1 -- Masses in MeV 0 ρ ω 0 φ (782.6) (1020) ρ + (770) -1 ρ 0 K *- K *0-1 -1/2 0 +1/2 +1 I 3 17

Baryons with J P =1/2 + Masses in MeV S N (939.6) P (938.3) +0 Λ 0 (1115.7) -1-2 Σ - (1197.4) Σ - (1192.6) Σ + (1189.4) Ξ - (1321.3) Ξ 0 (1314.8) -1-1/2 0 +1/2 +1 I 3 18

S 0 Δ (1232) -1-2 -3 (1530) (1385) (1672) Predicted: 1679-3/2-1 -1/2 0 +1/2 +1 +3/2 I 3 19

Mass relations for the stable Baryons Choose a basis of tensors (B (a) ) i j corresponding to definite isospin and hypercharge. Form the matrix: B i j = ψa (T (a) ) i j, where ψa are the fields of the eight baryons: B j i Σ 0 2 + Λ Σ + p 6 = Σ Σ0 2 + Λ n 6 Ξ Ξ 0 2 Λ 6 Form invariant tensors with B, B-bar and λ 8 Develop in the field bilinears: you get the general expression of M (8). i B j Σ 0 2 + Λ 6 = Σ Ξ Σ + Σ0 2 + Λ Ξ 0 6 p n 2 Λ 6 20

M (8) = 3{aTr(Bλ 8 B) + btr(bbλ 8 )} = at 1 + bt 2 T 1 = [NN + ΣΣ ΛΛ 2ΞΞ] T 2 = [ 2NN + ΣΣ ΛΛ + ΞΞ] Note: coeff. of (a-b) is proportional to Y coeff. of (a+b) + const. is proportional to C 2 =-Y 2 /2+2I(I+1): N Σ Λ Ξ (a-b) 3 0 0-3 (a+b) -1 2-2 -1 C 2 +1 +4 0 +1 Add a costant mass, eliminate the 3 parameters: Gell-Mann Okubo relation 1 3Λ + Σ (N + Ξ) = 2 4 1 0 side = 1128 MeV 2 0 side = 1135 MeV!!! 21

Decuplet M = M 0 + ay Masses are equispaced, 2 parameters and 4 masses. Δ (1232) (1385) (1530) (1672) Δ=153 Δ=145 Δ=142 22

Pseudoscalar Mesons Gell-Mann Okubo η = 4K π 3 1 st side = 547 MeV 2 nd side = 615 MeV??? squared masses? There is octet- singlet mixing! η 2 = 4K 2 π 2 The G-M O relation gives the mass of 8>, but there are other 2 unlnowns: the mass of 0> and a non-diagonal mass. Trovo sin 2 θ = M 8 η η' η linear mass formula: sinθ= 0.41, θ = 27 0 quadratic mass formula: sinθ= 0.19, θ = 12 0 3 η(547) >= cosθ 8 > +sinθ 0 > η'(958) >= sinθ 8 > +cosθ 0 > 1 st side = 0.299 GeV 2 2 nd side = 0.322 GeV 2? better? 23

Gell-Mann Okubo Vector Mesons octet-singlet mixing: ω(783) >= cosθ V 8 > +sinθ V 0 > ω 8 = 4K * ρ = 933MeV ω 2 8 = 4K *2 ρ 2 3 3 φ(1020) >= sinθ V 8 > +cosθ V 0 > sin 2 θ V = M 8 ω φ ω linear: sinθ= 0.80, tanθ=1.3, θ = 53 0 quadratic: sinθ= 0.77, tanθ=1.2, θ = 50 0 = 0.863GeV 2 A simple result: the angle is close to the ideal mixing angle, for which: ω = cosθ 1 1 1 6 + sinθ 1 1 1 3 = 1 1 2 1 2 1 φ = sinθ 1 1 1 6 + cosθ 1 1 1 3 = 1 0 2 0 2 1 1 tanθ = 2;θ = 54 0.7 24

Quarks! Basic fermions of spin 1/2: an SU(3) tripletto: u d ; s Nota: I 3 Y Q S +1/2 +1/3 +2/3 0 1/2 +1/3 1/3 0 0 2/3 1/3 1 Y such that q-qbar has integer hypercharges Q=I 3 +1/2Y the s quark carries the negative unit of strangeness Mesons = q-qbar = 8 + 1.as before. Baryons: Sakata used basic fields with B=1(p,n, Λ). Now, we can choose the baryon numer of the triplet as appropriate: B( q)= 1/3 Baryons= (qqq) (qqq) has only negative strangeness, and contains only the observed reps: 1, 8, 10 Three quarks for Master Mark! 25

Qaurk Composition of the Baryons Octet: I Y (S) partic. [ud]u, [ud]d 1/2 1 0 p, n [su]u, [su]d, [sd]u, [ud]s 0,1 0-1 Σ, Λ [su]s, [sd]s 1/2-1 -2 Ξ Decuplet: {uuu}, {uud}, {udd}, {ddd} 3/2 1 0 Δ {uus}, {uds}, {dds} 1 0-1 Y* {uss}, {dss} 1/2-1 -2 Ξ* {sss} 0-2 -3 Ω 26

Quarks! (continua) Octet Baryons: [3 3 ]A 3=3-bar 3=8 1= B [ab ]c and we have to subtract the Trace (= singlet). In formulae, we get a tensor with mixed symmetry : B {[ab]c} = N(B [ab]c 1 6 ε abcε def B [de ] f ) = = N( 2 3 B [ab ]c 1 3 B [bc]a 1 3 B [ca ]b ) = N 3 [(B [ab ]c + B [cb ]a ) + (B [ab ]c + B [ac ]b )] the same symmetry applies to the spin wave function: 1/2 1/2 1/2 1/2 the overall wave-function (spin * SU(3)) is symmetric the same holds (trivially) for the decuplet: Δ ++ =u u u What happened to Fermi statistics!!!??!! 27