The Standard Theory of Elementary Particle Physics and Beyond

Size: px
Start display at page:

Download "The Standard Theory of Elementary Particle Physics and Beyond"

Transcription

1 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,

2 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

3 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 )

4 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) 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

5 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, M. Gell-Mann: Symmetries of Baryons and Mesons, Phys. Rev. 125 (1962) Fundamental fields: T, Bµ Lagrangian: L = T[ i( µ g strong B µ )γ µ + M]T 1 4 B µν B µν 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

6 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

7 K - -p cross-section 7

8 K + -N cross-sections 8

9 The Eightfold Way M. Gell-Mann: Symmetries of Baryons and Mesons, Phys. Rev. 125 (1962) 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

10 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 (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

11 SU(3) generators Le 8 Gell-Mann matrices 0 ;λ 4 = ;λ 5 = 0 i 0 ; i 0 0 λ 1,2,3 = σ1,2,3 0 λ 6 = ;λ = i ;λ = i 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 = {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

12 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 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! m + m + m 1 p n Λ

13 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

14 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

15 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

16 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

17 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

18 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

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

20 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 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 Λ 6 = Σ Ξ Σ + Σ0 2 + Λ Ξ 0 6 p n 2 Λ 6 20

21 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) (a+b) C Add a costant mass, eliminate the 3 parameters: Gell-Mann Okubo relation 1 3Λ + Σ (N + Ξ) = side = 1128 MeV 2 0 side = 1135 MeV!!! 21

22 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

23 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 = η(547) >= cosθ 8 > +sinθ 0 > η'(958) >= sinθ 8 > +cosθ 0 > 1 st side = GeV 2 2 nd side = GeV 2? better? 23

24 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 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 sinθ = φ = sinθ cosθ = tanθ = 2;θ =

25 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 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 = 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

26 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/ Ξ Decuplet: {uuu}, {uud}, {udd}, {ddd} 3/2 1 0 Δ {uus}, {uds}, {dds} Y* {uss}, {dss} 1/ Ξ* {sss} Ω 26

27 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

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

Quantum Field Theory. Ling-Fong Li. (Institute) Quark Model 1 / 14 Quantum Field Theory Ling-Fong Li (Institute) Quark Model 1 / 14 QCD Quark Model Isospin symmetry To a good approximation, nuclear force is independent of the electromagnetic charge carried by the nucleons

More information

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

January 31, PHY357 Lecture 8. Quark composition of hadrons. Hadron magnetic moments. Hadron masses January 3, 08 PHY357 Lecture 8 Quark composition of hadrons Hadron magnetic moments Hadron masses January 3, 08 Quark rules for building Hadrons! Three types of stable quark configurations established!

More information

Lecture 9 Valence Quark Model of Hadrons

Lecture 9 Valence Quark Model of Hadrons Lecture 9 Valence Quark Model of Hadrons Isospin symmetry SU(3) flavour symmetry Meson & Baryon states Hadronic wavefunctions Masses and magnetic moments Heavy quark states 1 Isospin Symmetry Strong interactions

More information

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

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 Lecture 2 Quark Model The Eight Fold Way Adnan Bashir, IFM, UMSNH, Mexico August 2014 Culiacán Sinaloa The SU(3) Group SU(3) and Mesons Contents Quarks and Anti-quarks SU(3) and Baryons Masses and Symmetry

More information

Gian Gopal Particle Attributes Quantum Numbers 1

Gian Gopal Particle Attributes Quantum Numbers 1 Particle Attributes Quantum Numbers Intro Lecture Quantum numbers (Quantised Attributes subject to conservation laws and hence related to Symmetries) listed NOT explained. Now we cover Electric Charge

More information

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

This means that n or p form a doublet under isospin transformation. Isospin invariance simply means that. [T i, H s ] = 0 1 QCD 1.1 Quark Model 1. Isospin symmetry In early studies of nuclear reactions, it was found that, to a good approximation, nuclear force is independent of the electromagnetic charge carried by the nucleons

More information

Lecture 8. CPT theorem and CP violation

Lecture 8. CPT theorem and CP violation Lecture 8 CPT theorem and CP violation We have seen that although both charge conjugation and parity are violated in weak interactions, the combination of the two CP turns left-handed antimuon onto right-handed

More information

Notes on SU(3) and the Quark Model

Notes on SU(3) and the Quark Model Notes on SU() and the Quark Model Contents. SU() and the Quark Model. Raising and Lowering Operators: The Weight Diagram 4.. Triangular Weight Diagrams (I) 6.. Triangular Weight Diagrams (II) 8.. Hexagonal

More information

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

Quark Model. Ling-Fong Li. (Institute) Note 8 1 / 26 Quark Model Ling-Fong Li (Institute) Note 8 1 / 6 QCD Quark Model Isospin symmetry To a good approximation, nuclear force is independent of the electric charge carried by the nucleons charge independence.

More information

The Quark Parton Model

The Quark Parton Model The Quark Parton Model Quark Model Pseudoscalar J P = 0 Mesons Vector J P = 1 Mesons Meson Masses J P = 3 /2 + Baryons J P = ½ + Baryons Resonances Resonance Detection Discovery of the ω meson Dalitz Plots

More information

Dr Victoria Martin, Prof Steve Playfer Spring Semester 2013

Dr Victoria Martin, Prof Steve Playfer Spring Semester 2013 Particle Physics Dr Victoria Martin, Prof Steve Playfer Spring Semester 2013 Lecture 12: Mesons and Baryons Mesons and baryons Strong isospin and strong hypercharge SU(3) flavour symmetry Heavy quark states

More information

Lecture 9. Isospin The quark model

Lecture 9. Isospin The quark model Lecture 9 Isospin The quark model There is one more symmetry that applies to strong interactions. isospin or isotopic spin It was useful in formulation of the quark picture of known particles. We can consider

More information

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

The Development of Particle Physics. Dr. Vitaly Kudryavtsev E45, Tel.: The Development of Particle Physics Dr. Vitaly Kudryavtsev E45, Tel.: 0114 2224531 v.kudryavtsev@sheffield.ac.uk Previous lecture New unstable particles discovered in 40s-50s. First hyperons (particles

More information

Quark Model History and current status

Quark Model History and current status Quark Model History and current status Manon Bischoff Heavy-Ion Seminar 2013 October 31, 2013 Manon Bischoff Quark Model 1 Outline Introduction Motivation and historical development Group theory and the

More information

wave functions PhD seminar- FZ Juelich, Feb 2013

wave functions PhD seminar- FZ Juelich, Feb 2013 SU(3) symmetry and Baryon wave functions Sedigheh Jowzaee PhD seminar- FZ Juelich, Feb 2013 Introduction Fundamental symmetries of our universe Symmetry to the quark model: Hadron wave functions q q Existence

More information

Flavour physics Lecture 1

Flavour physics Lecture 1 Flavour physics Lecture 1 Jim Libby (IITM) XI th SERC school on EHEP NISER Bhubaneswar November 2017 Lecture 1 1 Outline What is flavour physics? Some theory and history CKM matrix Lecture 1 2 What is

More information

Clebsch-Gordan Coefficients

Clebsch-Gordan Coefficients Phy489 Lecture 7 Clebsch-Gordan Coefficients 2 j j j2 m m m 2 j= j j2 j + j j m > j m > = C jm > m = m + m 2 2 2 Two systems with spin j and j 2 and z components m and m 2 can combine to give a system

More information

Quark model of hadrons and the SU(3) symmetry

Quark model of hadrons and the SU(3) symmetry Quark moel of harons an the SU) symmetry Davi Nagy - particle physics 5) January 4, 0 Young man, if I coul remember the names of these particles, I woul have been a botanist. Enrico Fermi to his stuent

More information

SU(3) symmetry and Baryon wave functions

SU(3) symmetry and Baryon wave functions INTERNATIONAL PHD PROJECTS IN APPLIED NUCLEAR PHYSICS AND INNOVATIVE TECHNOLOGIES This project is supported by the Foundation for Polish Science MPD program, co-financed by the European Union within the

More information

arxiv:hep-ph/ v3 15 Mar 2006

arxiv:hep-ph/ v3 15 Mar 2006 The [56,4 + ] baryons in the 1/N c expansion N. Matagne and Fl. Stancu University of Liège, Institute of Physics B5, Sart Tilman, B-4000 Liège 1, Belgium (Dated: February, 008) arxiv:hep-ph/040961v 15

More information

Lie Theory in Particle Physics

Lie Theory in Particle Physics Lie Theory in Particle Physics Tim Roethlisberger May 5, 8 Abstract In this report we look at the representation theory of the Lie algebra of SU(). We construct the general finite dimensional irreducible

More information

Particle Physics. Lecture 11: Mesons and Baryons

Particle Physics. Lecture 11: Mesons and Baryons Particle Physics Lecture 11: Mesons and Baryons Measuring Jets Fragmentation Mesons and Baryons Isospin and hypercharge SU(3) flavour symmetry Heavy Quark states 1 From Tuesday: Summary In QCD, the coupling

More information

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

Quark Model. Mass and Charge Patterns in Hadrons. Spin-1/2 baryons: Nucleons: n: MeV; p: MeV Mass and Charge Patterns in Hadrons To tame the particle zoo, patterns in the masses and charges can be found that will help lead to an explanation of the large number of particles in terms of just a few

More information

Problem Set # 1 SOLUTIONS

Problem Set # 1 SOLUTIONS Wissink P640 Subatomic Physics I Fall 2007 Problem Set # 1 S 1. Iso-Confused! In lecture we discussed the family of π-mesons, which have spin J = 0 and isospin I = 1, i.e., they form the isospin triplet

More information

Kern- und Teilchenphysik I Lecture 13:Quarks and QCD

Kern- und Teilchenphysik I Lecture 13:Quarks and QCD Kern- und Teilchenphysik I Lecture 13:Quarks and QCD (adapted from the Handout of Prof. Mark Thomson) Prof. Nico Serra Dr. Patrick Owen, Dr. Silva Coutinho http://www.physik.uzh.ch/de/lehre/phy211/hs2016.html

More information

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

Symmetry Groups conservation law quantum numbers Gauge symmetries local bosons mediate the interaction Group Abelian Product of Groups simple Symmetry Groups Symmetry plays an essential role in particle theory. If a theory is invariant under transformations by a symmetry group one obtains a conservation law and quantum numbers. For example,

More information

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

Particle Physics. Michaelmas Term 2009 Prof Mark Thomson. Handout 7 : Symmetries and the Quark Model. Introduction/Aims Particle Physics Michaelmas Term 2009 Prof Mark Thomson Handout 7 : Symmetries and the Quark Model Prof. M.A. Thomson Michaelmas 2009 205 Introduction/Aims Symmetries play a central role in particle physics;

More information

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

Lecture notes Particle Physics II. Quantum Chromo Dynamics. 2. SU(2) and SU(3) Symmetry. Michiel Botje Nikhef, Science Park, Amsterdam Lecture notes Particle Physics II Quantum Chromo Dynamics 2. SU(2) and SU(3) Symmetry Michiel Botje Nikhef, Science Park, Amsterdam November 2, 23 Symmetry in (particle) physics If the Lagrangian of the

More information

Discrete Transformations: Parity

Discrete Transformations: Parity Phy489 Lecture 8 0 Discrete Transformations: Parity Parity operation inverts the sign of all spatial coordinates: Position vector (x, y, z) goes to (-x, -y, -z) (eg P(r) = -r ) Clearly P 2 = I (so eigenvalues

More information

Another view of the Gell-Mann-Okubo mass formula

Another view of the Gell-Mann-Okubo mass formula 3 February 017 Another view of the Gell-Mann-Okubo mass formula Jean Pestieau 1 The Gell-Mann-Okubo mass formula for light hadrons assumes that mass effective operator is in the 8 representation of flavour

More information

Partners of the SU(3) hadrons

Partners of the SU(3) hadrons Partners of the SU(3) hadrons Bernard Riley 1 The hadrons of the SU(3) J P = 0 -, ½ + and 1 - multiplets are shown to have partners of the same spin or of spin difference ½. Partnerships occur between

More information

Standard Model & Beyond

Standard Model & Beyond XI SERC School on Experimental High-Energy Physics National Institute of Science Education and Research 13 th November 2017 Standard Model & Beyond Lecture III Sreerup Raychaudhuri TIFR, Mumbai 2 Fermions

More information

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

Lecture 6 Isospin. What is Isospin? Rota4ons in Isospin space Reac4on rates Quarks and Isospin Heavier quarks FK Lecture 6 Isospin What is Isospin? Rota4ons in Isospin space Reac4on rates Quarks and Isospin Heavier quarks FK7003 33 SU() Isospin Isospin introduced based on the observa4on that: m p = 0.9383 GeV and

More information

Part 7: Hadrons: quarks and color

Part 7: Hadrons: quarks and color FYSH3, fall Tuomas Lappi tuomas.v.v.lappi@jyu.fi Office: FL49. No fixed reception hours. kl Part 7: Hadrons: quarks and color Introductory remarks In the previous section we looked at the properties of

More information

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

Lecture 6 Isospin. What is Isospin? Rota4ons in Isospin space Reac4on rates Quarks and Isospin Gell- Mann- Nishijima formula FK Lecture 6 Isospin What is Isospin? Rota4ons in Isospin space Reac4on rates Quarks and Isospin Gell- Mann- Nishijima formula FK7003 08 SU() Isospin Isospin introduced based on the observa4on that: m p =

More information

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

The Gauge Principle Contents Quantum Electrodynamics SU(N) Gauge Theory Global Gauge Transformations Local Gauge Transformations Dynamics of Field Ten Lecture 4 QCD as a Gauge Theory Adnan Bashir, IFM, UMSNH, Mexico August 2013 Hermosillo Sonora The Gauge Principle Contents Quantum Electrodynamics SU(N) Gauge Theory Global Gauge Transformations Local

More information

Weak interactions and vector bosons

Weak interactions and vector bosons Weak interactions and vector bosons What do we know now about weak interactions? Theory of weak interactions Fermi's theory of weak interactions V-A theory Current - current theory, current algebra W and

More information

CHAPTER II: The QCD Lagrangian

CHAPTER II: The QCD Lagrangian CHAPTER II: The QCD Lagrangian.. Preparation: Gauge invariance for QED - 8 - Ã µ UA µ U i µ U U e U A µ i.5 e U µ U U Consider electrons represented by Dirac field ψx. Gauge transformation: Gauge field

More information

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

SU(3) systematization of baryons. Vadim Guzey. Theory Center, Jefferson Lab SU(3) systematization of baryons Vadim Guzey Theory Center, Jefferson Lab In collaboration with M.V. Polyakov: V. Guzey, hep-ph/05176 V. Guzey and M.V. Polyakov, hep-ph/051355 Cake seminar, Theory Group,

More information

Introduction to Quantum Chromodynamics (QCD)

Introduction to Quantum Chromodynamics (QCD) Introduction to Quantum Chromodynamics (QCD) Jianwei Qiu Theory Center, Jefferson Lab May 29 June 15, 2018 Lecture One The plan for my four lectures q The Goal: To understand the strong interaction dynamics

More information

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

Isospin. K.K. Gan L5: Isospin and Parity 1 Isospin Isospin is a continuous symmetry invented by Heisenberg: Explain the observation that the strong interaction does not distinguish between neutron and proton. Example: the mass difference between

More information

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

Introduction to group theory and its representations and some applications to particle physics Introduction to group theory and its representations and some applications to particle physics Valery Zamiralov D.V.Skobeltsyn Institute of Nuclear Physics, Moscow, RUSSIA February 14, 7 Contents 1 Introduction

More information

Introduction to Gauge Theories

Introduction to Gauge Theories Introduction to Gauge Theories Basics of SU(n) Classical Fields U() Gauge Invariance SU(n) Gauge Invariance The Standard Model Michel Lefebvre University of Victoria Physics and Astronomy PHYS506B, spring

More information

The Strong Interaction and LHC phenomenology

The Strong Interaction and LHC phenomenology The Strong Interaction and LHC phenomenology Juan Rojo STFC Rutherford Fellow University of Oxford Theoretical Physics Graduate School course Lecture 2: The QCD Lagrangian, Symmetries and Feynman Rules

More information

Quarks and hadrons. Chapter Quark flavor and color

Quarks and hadrons. Chapter Quark flavor and color Chapter 5 Quarks and hadrons Every atom has its ground state the lowest energy state of its electrons in the presence of the atomic nucleus as well as many excited states which can decay to the ground

More information

QCD and Models : introduction

QCD and Models : introduction [169/105] HUGS Summer School Jun, 2010 QCD and Models : introduction Eric Swanson Theodore Wulf (1910) Too Many Hadrons! Quarks and the Eightfold Way Quarks and the Eightfold Way Three quarks for

More information

Quarks and hadrons. Chapter 7

Quarks and hadrons. Chapter 7 Chapter 7 Quarks and hadrons Every atom has its ground state the lowest energy state of its electrons in the presence of the atomic nucleus as well as many excited states, which can decay to the ground

More information

Introduction to particle physics Lecture 4

Introduction to particle physics Lecture 4 Introduction to particle physics Lecture 4 Frank Krauss IPPP Durham U Durham, Epiphany term 2009 Outline 1 Mesons and Isospin 2 Strange particles 3 Resonances 4 The quark model Nuclei, nucleons, and mesons

More information

Back to Gauge Symmetry. The Standard Model of Par0cle Physics

Back to Gauge Symmetry. The Standard Model of Par0cle Physics Back to Gauge Symmetry The Standard Model of Par0cle Physics Laws of physics are phase invariant. Probability: P = ψ ( r,t) 2 = ψ * ( r,t)ψ ( r,t) Unitary scalar transformation: U( r,t) = e iaf ( r,t)

More information

Quark Model of Hadrons

Quark Model of Hadrons Quark Model of Hadrons mesons baryons symmetric antisymmetric mixed symmetry Quark Model of Hadrons 2 Why do quarks have color? ground state baryons orbital wave function = symmetic with L=0 SU(3) f x

More information

Introduction to particle physics Lecture 6

Introduction to particle physics Lecture 6 Introduction to particle physics Lecture 6 Frank Krauss IPPP Durham U Durham, Epiphany term 2009 Outline 1 Fermi s theory, once more 2 From effective to full theory: Weak gauge bosons 3 Massive gauge bosons:

More information

SU(N) representations

SU(N) representations Appendix C SU(N) representations The group SU(N) has N 2 1 generators t a which form the asis of a Lie algera defined y the commutator relations in (A.2). The group has rank N 1 so there are N 1 Casimir

More information

Mass Spectrum of a Baryon Octet is Linear

Mass Spectrum of a Baryon Octet is Linear Mass Spectrum of a Baryon Octet is Linear arxiv:hep-ph/9608289v1 9 Aug 1996 L. Burakovsky Theoretical Division, T-8 Los Alamos National Laboratory Los Alamos NM 87545, USA and L.P. Horwitz School of Natural

More information

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 The Eightfold Way model, the SU()-flavour model and the medium-strong interaction Syed Afsar Abbas Jafar Sadiq Research Institute AzimGreenHome, NewSirSyed Nagar, Aligarh - 000, India (e-mail : drafsarabbas@gmail.com)

More information

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

.!  # e  + $ e. have the same spin as electron neutrinos, and is ½ integer (fermions). Conservation Laws For every conservation of some quantity, this is equivalent to an invariance under some transformation. Invariance under space displacement leads to (and from) conservation of linear

More information

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

Electroweak interactions of quarks. Benoit Clément, Université Joseph Fourier/LPSC Grenoble Electroweak interactions of quarks Benoit Clément, Université Joseph Fourier/LPSC Grenoble HASCO School, Göttingen, July 15-27 2012 1 PART 1 : Hadron decay, history of flavour mixing PART 2 : Oscillations

More information

How nucleon gets its mass

How nucleon gets its mass Fiz-Tech, Dec 05, 2006 How nucleon gets its mass Dmitri Diakonov Petersburg Nuclear Physics Institute 1. Quantum Chromodynamics: the theory of strong interactions 2. Chiral symmetry of strong interactions

More information

arxiv:hep-ph/ v2 15 Oct 2001

arxiv:hep-ph/ v2 15 Oct 2001 THE EIGHTFOLD WAY 1 Jonathan L. Rosner arxiv:hep-ph/0109241v2 15 Oct 2001 The Eightfold Way is the name coined by Murray Gell-Mann (1961) to describe a classification scheme of the elementary particles

More information

PHYS 3446 Lecture #17

PHYS 3446 Lecture #17 PHY 3446 Lecture #7 Monday, Nov. 6, 26 Dr.. Elementary Particle Properties Quantum Numbers trangeness Isospin Gell-Mann-Nishijima Relations Production and Decay of Resonances Monday, Nov. 6, 26 PHY 3446,

More information

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

Particle Physics. Lecture 12: Hadron Decays.!Resonances!Heavy Meson and Baryons!Decays and Quantum numbers!ckm matrix Particle Physics Lecture 12: Hadron Decays!Resonances!Heavy Meson and Baryons!Decays and Quantum numbers!ckm matrix 1 From Friday: Mesons and Baryons Summary Quarks are confined to colourless bound states,

More information

Discovery of Pions and Kaons in Cosmic Rays in 1947

Discovery of Pions and Kaons in Cosmic Rays in 1947 Discovery of Pions and Kaons in Cosmic Rays in 947 π + µ + e + (cosmic rays) Points to note: de/dx Bragg Peak Low de/dx for fast e + Constant range (~600µm) (i.e. -body decay) small angle scattering Strange

More information

Properties of the proton and neutron in the quark model

Properties of the proton and neutron in the quark model Properties of the proton and neutron in the quark model A good way to introduce the ideas encoded in the quark model is to understand how it simply explains properties of the ground-state baryons and mesons

More information

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

Hadron Physics & Quantum Chromodynamics Adnan Bashir, IFM, UMSNH, Mexico August 2013 Hermosillo Sonora Hadron Physics & Quantum Chromodynamics Adnan Bashir, IFM, UMSNH, Mexico August 2013 Hermosillo Sonora Hadron Physics & QCD Part 1: First Encounter With Hadrons: Introduction to Mesons & Baryons, The Quark

More information

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

Gell-Mann Okubo Mass Formula for SU(4) Meson Hexadecuplet LA-UR-96-415 IASSNS-HEP-96/81 Gell-Mann Okubo Mass Formula for SU(4) Meson Hexadecuplet L. Burakovsky Theoretical Division, T-8 Los Alamos National Laboratory Los Alamos NM 87545, USA and L.P. Horwitz

More information

THE STANDARD MODEL AND THE GENERALIZED COVARIANT DERIVATIVE

THE STANDARD MODEL AND THE GENERALIZED COVARIANT DERIVATIVE THE STANDAD MODEL AND THE GENEALIZED COVAIANT DEIVATIVE arxiv:hep-ph/9907480v Jul 999 M. Chaves and H. Morales Escuela de Física, Universidad de Costa ica San José, Costa ica E-mails: mchaves@cariari.ucr.ac.cr,

More information

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

The hadronization into the octet of pseudoscalar mesons in terms of SU(N) gauge invariant Lagrangian The hadronization into the octet of pseudoscalar mesons in terms of SU(N gauge invariant Lagrangian National Research Nuclear University Moscow 115409, Moscow, Russia E-mail: a kosh@internets.ru By breaking

More information

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

Λ QCD and Light Quarks Contents Symmetries of the QCD Lagrangian Chiral Symmetry and Its Breaking Parity and Handedness Parity Doubling Explicit Chira Lecture 5 QCD Symmetries & Their Breaking From Quarks to Hadrons Adnan Bashir, IFM, UMSNH, Mexico August 2013 Hermosillo Sonora Λ QCD and Light Quarks Contents Symmetries of the QCD Lagrangian Chiral Symmetry

More information

Origin and Status of INSTANTONS

Origin and Status of INSTANTONS Utrecht University Origin and Status of INSTANTONS Gerard t Hooft, Spinoza Institute. Erice 2013 The pre-qcd age (before 1971) d s u J PC = 0 + K o K + K* o K* + π η π o η π + ρ ω ρ o ϕ ρ + K K o K* J

More information

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

Kaons - A Micro-physics Laboratory Will you still need me when I m 64? (The Beatles) Kaons - A Micro-physics Laboratory Will you still need me when I m 64? (The Beatles) William A. Bardeen Guest Scientist Retired Fermilab William A. Bardeen, Sakata100 Symposium, October 27-28, 2011 p.1

More information

Quark model. Jan 30, 2006 Lecture 8 1

Quark model. Jan 30, 2006 Lecture 8 1 Quark model Jan 30, 2006 Lecture 8 1 Quark model of hadrons!!!! Developed long before QCD was recognized as the appropriate quantum field theory of the strong interactions Postulate that 1.! All baryons

More information

PHYS 420: Astrophysics & Cosmology

PHYS 420: Astrophysics & Cosmology PHYS 420: Astrophysics & Cosmology Dr Richard H. Cyburt Assistant Professor of Physics My office: 402c in the Science Building My phone: (304) 384-6006 My email: rcyburt@concord.edu My webpage: www.concord.edu/rcyburt

More information

July 10, Particle Physics I Physics G8069 Fall 2006

July 10, Particle Physics I Physics G8069 Fall 2006 July 10, 2007 Particle Physics I Physics G8069 Fall 2006 Contents List of exercises Conventions Useful formulas Selected particle properties Course outline Preface page v vii viii x xiii xvii 1 The particle

More information

Le Modèle Standard et ses extensions

Le Modèle Standard et ses extensions Particules Élémentaires, Gravitation et Cosmologie Année 2007-08 08 Le Modèle Standard et ses extensions Cours III: 15 février f 2008 Weak Interactions: from Fermi s s model to a gauge theory 15 fevrier

More information

Astronomy, Astrophysics, and Cosmology

Astronomy, Astrophysics, and Cosmology Astronomy, Astrophysics, and Cosmology Luis A. Anchordoqui Department of Physics and Astronomy Lehman College, City University of New York Lesson IX April 12, 2016 arxiv:0706.1988 L. A. Anchordoqui (CUNY)

More information

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

Homework 3: Group Theory and the Quark Model Due February 16 Homework 3: Group Theory and the Quark Model Due February 16 1. Lorentz Group. From the defining requirement that a Lorentz transformation implemented by a matrix Λ leave the metric invariant: Λ µ ρη ρσ

More information

Adding families: GIM mechanism and CKM matrix

Adding families: GIM mechanism and CKM matrix Particules Élémentaires, Gravitation et Cosmologie Année 2007-08 08 Le Modèle Standard et ses extensions Cours VII: 29 février f 2008 Adding families: GIM mechanism and CKM matrix 29 fevrier 2008 G. Veneziano,

More information

Lecture 3: Quarks and Symmetry in Quarks

Lecture 3: Quarks and Symmetry in Quarks Lecture 3: Quarks and Symmetry in Quarks Quarks Cross Section, Fermions & Bosons, Wave Eqs. Symmetry: Rotation, Isospin (I), Parity (P), Charge Conjugate (C), SU(3), Gauge symmetry Conservation Laws: http://faculty.physics.tamu.edu/kamon/teaching/phys627/

More information

Chapter 5 Theories and Lagrangians III: The Standard Model

Chapter 5 Theories and Lagrangians III: The Standard Model Chapter 5 Theories and Lagrangians III: The Standard Model The previous two chapters were devoted to introducing the basic ingredients necessary in building up a physical description of elementary particles:

More information

Exotic Diquark Spectroscopy

Exotic Diquark Spectroscopy Exotic Diquark Spectroscopy JLab November 2003 R.L. Jaffe F. Wilczek hep-ph/0307341 The discovery of the Θ + (1540) this year marks the beginning of a new and rich spectroscopy in QCD.... What are the

More information

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

The Heavy Quark Spin Symmetry and SU(3)-Flavour Partners of the X(3872) The Heavy Quark Spin Symmetry and SU(3)-Flavour Partners of the X(3872) Carlos Hidalgo, J. Nieves and M. Pavón-Valderrama Hypernuclear and Strange Particle Physics 2012 IFIC (CSIC - Universitat de València)

More information

Symmetries, Fields and Particles 2013 Solutions

Symmetries, Fields and Particles 2013 Solutions Symmetries, Fields and Particles 03 Solutions Yichen Shi July 9, 04. a Define the groups SU and SO3, and find their Lie algebras. Show that these Lie algebras, including their bracket structure, are isomorphic.

More information

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

Outline. Charged Leptonic Weak Interaction. Charged Weak Interactions of Quarks. Neutral Weak Interaction. Electroweak Unification Weak Interactions Outline Charged Leptonic Weak Interaction Decay of the Muon Decay of the Neutron Decay of the Pion Charged Weak Interactions of Quarks Cabibbo-GIM Mechanism Cabibbo-Kobayashi-Maskawa

More information

Evidence for the Strong Interaction

Evidence for the Strong Interaction Evidence for the Strong Interaction Scott Wilbur Scott Wilbur Evidence for the Strong Interaction 1 Overview Continuing search inside fundamental particles Scott Wilbur Evidence for the Strong Interaction

More information

Part 6: Hadrons: quantum numbers and excited states

Part 6: Hadrons: quantum numbers and excited states FYSH3, fall 3 Tuomas Lappi tuomas.v.v.lappi@jyu.fi Office: FL49. No fixed reception hours. fall 3 Part 6: Hadrons: quantum numbers and excited states Introductory remarks Properties of hadrons can be understood

More information

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

A.A. Godizov. Institute for High Energy Physics, Protvino, Russia arxiv:1410.886v1 [hep-ph] 0 Oct 2014 QCD and nuclear physics. How to explain the coincidence between the radius of the strong interaction of nucleons and the characteristic scale of neutron-neutron electrostatic

More information

Kern- und Teilchenphysik II Lecture 1: QCD

Kern- und Teilchenphysik II Lecture 1: QCD Kern- und Teilchenphysik II Lecture 1: QCD (adapted from the Handout of Prof. Mark Thomson) Prof. Nico Serra Dr. Marcin Chrzaszcz Dr. Annapaola De Cosa (guest lecturer) www.physik.uzh.ch/de/lehre/phy213/fs2017.html

More information

The Quantum Chromodynamics Theory Of Quadruply Strange Pentaquarks

The Quantum Chromodynamics Theory Of Quadruply Strange Pentaquarks The Quantum Chromodynamics Theory Of Quadruply Strange Pentaquarks Based on a generalized particle diagram of baryons and antibaryons which, in turn, is based on symmetry principles, this theory predicts

More information

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

ON SOME MODELS OF THE EXOTIC HADRON STATES. Siniša R. Ignjatović and Vesna Borka Jovanović FACTA UNIVERSITATIS (NIŠ) Physics, Chemistry and Technology Vol. 12, N o 2, Special Issue, 2014, pp. 151 158 DOI: 10.2298/FUPCT1402151I ON SOME MODELS OF THE EXOTIC HADRON STATES Siniša R. Ignjatović and

More information

Isospin: An Approximate Symmetry on the Quark Level

Isospin: An Approximate Symmetry on the Quark Level Isospin: An Approximate Symmetry on the Quark Level Molly S. Peeples molly@mit.edu Cambridge, MA 0139 April 7, 004 Abstract Isospin is an approximate symmetry which treats the up and down quarks as different

More information

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

Physics 125 Course Notes Identical Particles Solutions to Problems F. Porter Physics 5 Course Notes Identical Particles Solutions to Problems 00 F. Porter Exercises. Let us use the Pauli exclusion principle, and the combination of angular momenta, to find the possible states which

More information

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

η π 0 γγ decay in the three-flavor Nambu Jona-Lasinio model TIT/HEP-38/NP INS-Rep.-3 η π 0 γγ decay in the three-flavor Nambu Jona-Lasinio model arxiv:hep-ph/96053v 8 Feb 996 Y.Nemoto, M.Oka Department of Physics, Tokyo Institute of Technology, Meguro, Tokyo 5,

More information

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

OUTLINE. CHARGED LEPTONIC WEAK INTERACTION - Decay of the Muon - Decay of the Neutron - Decay of the Pion Weak Interactions OUTLINE CHARGED LEPTONIC WEAK INTERACTION - Decay of the Muon - Decay of the Neutron - Decay of the Pion CHARGED WEAK INTERACTIONS OF QUARKS - Cabibbo-GIM Mechanism - Cabibbo-Kobayashi-Maskawa

More information

Symmetries, Groups, and Conservation Laws

Symmetries, Groups, and Conservation Laws Chapter Symmetries, Groups, and Conservation Laws The dynamical properties and interactions of a system of particles and fields are derived from the principle of least action, where the action is a 4-dimensional

More information

Particle Physics - Chapter 1 The static quark model

Particle Physics - Chapter 1 The static quark model Particle Physics - Chapter The static quark model Paolo Bagnaia last mod. 7-Mar-8 The static quark model. Quantum numbers 2. Hadrons : elementary or composite? 3. The eightfold way 4. Baryon Resonances

More information

Examination paper for FY3403 Particle physics

Examination paper for FY3403 Particle physics Department of physics Examination paper for FY3403 Particle physics Academic contact during examination: Jan Myrheim Phone: 900 75 7 Examination date: December 6, 07 Examination time: 9 3 Permitted support

More information

DEEP INELASTIC SCATTERING

DEEP INELASTIC SCATTERING DEEP INELASTIC SCATTERING Electron scattering off nucleons (Fig 7.1): 1) Elastic scattering: E = E (θ) 2) Inelastic scattering: No 1-to-1 relationship between E and θ Inelastic scattering: nucleon gets

More information

Electric Dipole Moments and the strong CP problem

Electric Dipole Moments and the strong CP problem Electric Dipole Moments and the strong CP problem We finally understand CP viola3on.. QCD theta term Jordy de Vries, Nikhef, Amsterdam Topical Lectures on electric dipole moments, Dec. 14-16 Introductory

More information

Critical lines and points. in the. QCD phase diagram

Critical lines and points. in the. QCD phase diagram Critical lines and points in the QCD phase diagram Understanding the phase diagram Phase diagram for m s > m u,d quark-gluon plasma deconfinement quark matter : superfluid B spontaneously broken nuclear

More information

Fundamental Particles and Forces

Fundamental Particles and Forces Fundamental Particles and Forces A Look at the Standard Model and Interesting Theories André Gras PHYS 3305 SMU 1 Overview Introduction to Fundamental Particles and Forces Brief History of Discovery The

More information

Symmetries, Fields and Particles 2013 Solutions

Symmetries, Fields and Particles 2013 Solutions Symmetries, Fields and Particles 013 Solutions Yichen Shi Easter 014 1. (a) Define the groups SU() and SO(3), and find their Lie algebras. Show that these Lie algebras, including their bracket structure,

More information