Particle Physics II CP violation (also known as Physics of Antimatter ) Lecture 1. N. Tuning. Niels Tuning (1)

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1 Particle Physics II CP violation (also known as Physics of Antimatter ) Lecture 1 N. Tuning Niels Tuning (1)
2 Plan 1) Mon 2 Feb: Antimatter + SM 2) Wed 4 Feb: CKM matrix + Unitarity Triangle 3) Mon 9 Feb: Mixing + Master eqs. + B 0 J/ψK s 4) Wed 11 Feb: CP violation in B (s) decays (I) 5) Mon 16 Feb: CP violation in B (s) decays (II) 6) Wed 18 Feb: CP violation in K decays + Overview 7) Mon 23 Feb: Exam on part 1 (CP violation) Final Mark: if (mark > 5.5) mark = max(exam, 0.8*exam + 0.2*homework) else mark = exam In parallel: Lectures on Flavour Physics by prof.dr. R. Fleischer Tuesday + Thrusday Niels Tuning (2)
3 Plan 2 x 45 min 1) Keep track of room! 1) Monday + Wednesday: Start: 9:00 9:15 End: 11:00 Werkcollege: 11:00 ? Niels Tuning (3)
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5 Grand picture. These lectures Main motivation Universe Niels Tuning (5)
6 Introduction: it s all about the charged current CP violation is about the weak interactions, In particular, the charged current interactions: The interesting stuff happens in the interaction with quarks Therefore, people also refer to this field as flavour physics Niels Tuning (6)
7 Motivation 1: Understanding the Standard Model CP violation is about the weak interactions, In particular, the charged current interactions: Quarks can only change flavour through charged current interactions Niels Tuning (7)
8 Introduction: it s all about the charged current CP violation is about the weak interactions, In particular, the charged current interactions: In 1 st hour: Pparity, Cparity, CPparity the neutrino shows that Pparity is maximally violated Niels Tuning (8)
9 Introduction: it s all about the charged current CP violation is about the weak interactions, In particular, the charged current interactions: b In 1 st hour: W  gv ub Pparity, Cparity, CPparity Symmetry related to particle antiparticle u b gv* ub W + u Niels Tuning (9)
10 Motivation 2: Understanding the universe It s about differences in matter and antimatter Why would they be different in the first place? We see they are different: our universe is matter dominated Equal amounts of matter & anti matter (?) Matter Dominates! Niels Tuning (10)
11 Where and how do we generate the Baryon asymmetry? No definitive answer to this question yet! In 1967 A. Sacharov formulated a set of general conditions that any such mechanism has to meet 1) You need a process that violates the baryon number B: (Baryon number of matter=1, of antimatter = 1) 2) Both C and CP symmetries should be violated 3) Conditions 1) and 2) should occur during a phase in which there is no thermal equilibrium In these lectures we will focus on 2): CP violation Apart from cosmological considerations, I will convince you that there are more interesting aspects in CP violation Niels Tuning (11)
12 Introduction: it s all about the charged current CP violation is about the weak interactions, In particular, the charged current interactions: Same initial and final state Look at interference between B 0 f CP and B 0 B 0 f CP Niels Tuning (12)
13 Motivation 3: Sensitive to find new physics CP violation is about the weak interactions, In particular, the charged current interactions: Box diagram: ΔB=2 Penguin diagram: ΔB=1 b s b s b s μ μ B s b s b g s x x s g b s b B s B 0 b d b g x s s μ K * μ B s s b g b x s μ μ Are heavy particles running around in loops? Niels Tuning (13)
14 Recap: CPviolation (or flavour physics) is about charged current interactions Interesting because: 1) Standard Model: in the heart of quark interactions 2) Cosmology: related to matter antimatter asymetry 3) Beyond Standard Model: measurements are sensitive to new particles Matter Dominates! b s s b Niels Tuning (14)
15 Grand picture. These lectures Main motivation Universe Niels Tuning (15)
16 Personal impression: People think it is a complicated part of the Standard Model (me too:). Why? 1) Nonintuitive concepts? Imaginary phase in transition amplitude, T ~ e iφ Different bases to express quark states, d =0.97 d s b Oscillations (mixing) of mesons: K 0 > K 0 > 2) Complicated calculations? 3) Many decay modes? Beetopaipaigamma B f A 2 f g+ t g t 2 g+ t g t B f Af g+ t g 2  t 2 g+ t g t + + PDG reports 347 decay modes of the B 0 meson: Γ 1 l + ν l anything ( ± 0.28 ) 10 2 Γ 347 ν ν γ < CL=90% And for one decay there are often more than one decay amplitudes Niels Tuning (16)
17 Antimatter Dirac (1928): Prediction Anderson (1932): Discovery Presentday experiments Niels Tuning (17)
18 Schrödinger Classic relation between E and p: Quantum mechanical substitution: (operator acting on wave function ψ) Schrodinger equation: Solution: (show it is a solution) Niels Tuning (18)
19 KleinGordon Relativistic relation between E and p: Quantum mechanical substitution: (operator acting on wave function ψ) KleinGordon equation: or : Solution: with eigenvalues: But! Negative energy solution? Niels Tuning (19)
20 Dirac Paul Dirac tried to find an equation that was relativistically correct, but linear in d/dt to avoid negative energies (and linear in d/dx (or ) for Lorentz covariance) He found an equation that turned out to describe spin1/2 particles and predicted the existence of antiparticles Niels Tuning (20)
21 Dirac How to find that relativistic, linear equation?? Write Hamiltonian in general form, but when squared, it must satisfy: Let s find α i and β! So, α i and β must satisfy: α 2 1 = α 2 2 = α 2 3 = β 2 α 1,α 2,α 3, β anticommute with each other (not a unique choice!) Niels Tuning (21)
22 Dirac What are α and β?? The lowest dimensional matrix that has the desired behaviour is 4x4!? Often used PauliDirac representation: with: So, α i and β must satisfy: α 1 2 = α 2 2 = α 3 2 = β 2 α 1,α 2,α 3, β anticommute with each other (not a unique choice!) Niels Tuning (22)
23 Dirac Usual substitution: Leads to: Multiply by β: (β 2 =1) Gives the famous Dirac equation: Niels Tuning (23)
24 Dirac The famous Dirac equation: R.I.P. : Niels Tuning (24)
25 Dirac The famous Dirac equation: Remember! μ : Lorentz index 4x4 γ matrix: Dirac index Less compact notation: Even less compact : What are the solutions for ψ?? Niels Tuning (25)
26 Dirac The famous Dirac equation: Solutions to the Dirac equation? Try plane wave: Linear set of eq: 2 coupled equations: If p=0: Niels Tuning (26)
27 Dirac The famous Dirac equation: Solutions to the Dirac equation? Try plane wave: 2 coupled equations: If p 0: Two solutions for E>0: (and two for E<0) with: Niels Tuning (27)
28 Dirac Tuning (28) The famous Dirac equation: Solutions to the Dirac equation? Try plane wave: 2 coupled equations: If p 0: Two solutions for E>0: (and two for E<0) + 0 / 0 1 (1) m E p u + m E p u / (2)
29 Dirac Niels Tuning (29) The famous Dirac equation: ψ is 4component spinor 4 solutions correspond to fermions and antifermions with spin+1/2 and 1/2 Two solutions for E>0: (and two for E<0) + 0 / 0 1 (1) m E p u + m E p u / (2)
30 Discovery of antimatter Lead plate positron Nobelprize 1936 Niels Tuning (30)
31 Why antimatter must exist! FeynmanStueckelberg interpretation One observer s electron is the other observer s positron Niels Tuning (31)
32 CPT theorem CPT transformation: C: interchange particles and antiparticles P: reverse spacecoordinates T: Reverse timecoordinate CPT transformation closely related to Lorentzboost CPT invariance implies Particles and antiparticles have same mass and lifetime Lorentz invariance Niels Tuning (32)
33 CPT is conserved, but does antimatter fall down? Niels Tuning (33)
34 Experiments Need to have neutral antimatter Otherwise electrostatic forces spoil the weak gravitational force Make antiprotons Accelerator Antiproton factory Decelerator Storage Produce antihydrogen for study Trap Observe (spectroscopy, ) Thanks to Rolf Landua (CERN) Niels Tuning (34)
35 Antiproton beam CERN (1980): SppS: led to discovery of W, Z Niels Tuning (35)
36 Antiproton production Acceleration effciency ~ 103 Production efficiency ~ 104 Collection efficiency ~ 102 Niels Tuning (36)
37 Antiproton storage AC: Accumulator (3.57 GeV) PS: Decelarator (0.6 GeV) LEAR: Low Energy Antiproton ring (1982) Niels Tuning (37)
38 Antihydrogen 1995: First 9 antihydrogen atoms made: 1997: Replace LEAR by AD (antiproton decelerator) Niels Tuning (38)
39 Antihydrogen: challenge Beam energy: ~ GeV Atomic energy scale: ~ ev Trap charged particles: Niels Tuning (39)
40 Antihydrogen production ATHENA and ATRAP experiments Niels Tuning (40)
41 Antihydrogen production ATRAP, ALPHA, ASACUSA, AEGIS experiments: Niels Tuning (41)
42 Antihydrogen production Niels Tuning (42)
43 Antihydrogen detection ATRAP, ATHENA: pioneering the trapping technique ALPHA: trapped antihydrogen for 16 minutes Niels Tuning (43)
44 Antihydrogen detection ASACUSA: 2011: trapped antiproton in He (replacing an electron), measuring mass to Jan 2014: The ASACUSA experiment at CERN has succeeded for the first time in producing a beam of antihydrogen atoms. In a paper published today in Nature Communications, the ASACUSA collaboration reports the unambiguous detection of 80 antihydrogen atoms 2.7 metres downstream of their production, where the perturbing influence of the magnetic fields used initially to produce the antiatoms is small. This result is a significant step towards precise hyperfine spectroscopy of antihydrogen atoms. Niels Tuning (44)
45 Antihydrogen detection AEgIS Does antihydrogen fall with the same acceleration as hydrogen? Niels Tuning (45)
46 C, P, T C, P, T transformation: C: interchange particles and antiparticles P: reverse spacecoordinates T: Reverse timecoordinate CPT we discussed briefly After the break we deal with P and CP violation! Niels Tuning (46)
47 Break Niels Tuning (47)
48 P and C violation What is the link between antimatter and discrete symmetries? C operator changes matter into antimatter 2 more discrete symmetries: P and T Niels Tuning (48)
49 Continuous vs discrete symmetries Space, time translation & orientation symmetries are all continuous symmetries Each symmetry operation associated with one ore more continuous parameter There are also discrete symmetries Charge sign flip (Q Q) : C parity Spatial sign flip ( x,y,z x,y,z) : P parity Time sign flip (t t) : T parity Are these discrete symmetries exact symmetries that are observed by all physics in nature? Key issue of this course Niels Tuning (49)
50 Three Discrete Symmetries Parity, P Parity reflects a system through the origin. Converts righthanded coordinate systems to lefthanded ones. Vectors change sign but axial vectors remain unchanged x x, p p, but L = x p L Charge Conjugation, C Charge conjugation turns a particle into its antiparticle e + e , K  K Time Reversal, T Changes, for example, the direction of motion of particles t t Niels Tuning (50)
51 Example: People believe in symmetry Instruction for Abel Tasman, explorer of Australia (1642): Since many rich mines and other treasures have been found in countries north of the equator between 15 o and 40 o latitude, there is no doubt that countries alike exist south of the equator. The provinces in Peru and Chili rich of gold and silver, all positioned south of the equator, are revealing proofs hereof. Niels Tuning (51)
52 Example: People believe in symmetry Award Ceremony Speech Nobel Prize (1957): it was assumed almost tacitly, that elementary particle reactions are symmetric with respect to right and left. In fact, most of us were inclined to regard the symmetry of elementary particles with respect to right and left as a necessary consequence of the general principle of rightleft symmetry of Nature. only Lee and Yang asked themselves what kind of experimental support there was for the assumption that all elementary particle processes are symmetric with respect to right and left. Niels Tuning (52)
53 A realistic experiment: the Wu experiment (1956) Observe radioactive decay of Cobalt60 nuclei The process involved: 60 27Co 60 28Ni + e  + n e 60 27Co is spin5 and 60 28Ni is spin4, both e and n e are spin½ If you start with fully polarized Co (S Z =5) the experiment is essentially the same (i.e. there is only one spin solution for the decay) 5,+5> 4,+4> + ½,+½> + ½,+½> S=1/2 S=4 S=1/2 Niels Tuning (53)
54 Intermezzo: Spin and Parity and Helicity We introduce a new quantity: Helicity = the projection of the spin on the direction of flight of a particle H S S p p H=+1 ( righthanded ) H=1 ( lefthanded ) Niels Tuning (54)
55 The Wu experiment 1956 Experimental challenge: how do you obtain a sample of Co(60) where the spins are aligned in one direction Wu s solution: adiabatic demagnetization of Co(60) in magnetic fields at very low temperatures (~1/100 K!). Extremely challenging in Niels Tuning (55)
56 The Wu experiment 1956 The surprising result: the counting rate is different Electrons are preferentially emitted in direction opposite of 60 Co spin! Careful analysis of results shows that experimental data is consistent with emission of lefthanded (H=1) electrons only at any angle!! Backward Counting rate w.r.t unpolarized rate 60 Co polarization decreases as function of time Forward Counting rate w.r.t unpolarized rate Niels Tuning (56)
57 The Wu experiment 1956 Physics conclusion: Angular distribution of electrons shows that only pairs of lefthanded electrons / righthanded antineutrinos are emitted regardless of the emission angle Since righthanded electrons are known to exist (for electrons H is not Lorentzinvariant anyway), this means no lefthanded antineutrinos are produced in weak decay Parity is violated in weak processes Not just a little bit but 100% How can you see that 60 Co violates parity symmetry? If there is parity symmetry there should exist no measurement that can distinguish our universe from a parityflipped universe, but we can! Niels Tuning (57)
58 So P is violated, what s next? Wu s experiment was shortly followed by another clever experiment by L. Lederman: Look at decay p + m + n m Pion has spin 0, m,n m both have spin ½ spin of decay products must be oppositely aligned Helicity of muon is same as that of neutrino. m + p + n m OK OK Nice feature: can also measure polarization of both neutrino (p + decay) and antineutrino (p  decay) Ledermans result: All neutrinos are lefthanded and all antineutrinos are righthanded Niels Tuning (58)
59 Charge conjugation symmetry Introducing Csymmetry The C(harge) conjugation is the operation which exchanges particles and antiparticles (not just electric charge) It is a discrete symmetry, just like P, i.e. C 2 = 1 m + p + n m (LH) OK C m  p  n m (LH) OK C symmetry is broken by the weak interaction, just like P Niels Tuning (59)
60 The Weak force and C,P parity violation What about C+P CP symmetry? CP symmetry is parity conjugation (x,y,z x,y,z) followed by charge conjugation (X X) n m Intrinsic spin m + m  p + P C p  p + CP appears to be preserved in weak interaction! m + CP n m n m Niels Tuning (60)
61 What do we know now? C.S. Wu discovered from 60 Co decays that the weak interaction is 100% asymmetric in Pconjugation We can distinguish our universe from a parity flipped universe by examining 60 Co decays L. Lederman et al. discovered from π + decays that the weak interaction is 100% asymmetric in Cconjugation as well, but that CPsymmetry appears to be preserved First important ingredient towards understanding matter/antimatter asymmetry of the universe: weak force violates matter/antimatter(=c) symmetry! C violation is a required ingredient, but not enough as we will learn later Niels Tuning (61)
62 Conserved properties associated with C and P C and P are still good symmetries in any reaction not involving the weak interaction Can associate a conserved value with them (Noether Theorem) Each hadron has a conserved P and C quantum number What are the values of the quantum numbers Evaluate the eigenvalue of the P and C operators on each hadron P y> = p y> What values of C and P are possible for hadrons? Symmetry operation squared gives unity so eigenvalue squared must be 1 Possible C and P values are +1 and 1. Meaning of P quantum number If P=1 then P y> = +1 y> (wave function symmetric in space) if P=1 then P y> = 1 y> (wave function antisymmetric in space) Niels Tuning (62)
63 Figuring out P eigenvalues for hadrons QFT rules for particle vs. antiparticles Parity of particle and antiparticle must be opposite for fermions (spinn+1/2) Parity of bosons (spin N) is same for particle and antiparticle Definition of convention (i.e. arbitrary choice in def. of q vs q) Quarks have positive parity Antiquarks have negative parity e  has positive parity as well. (Can define other way around: Notation different, physics same) Parity is a multiplicative quantum number for composites For composite AB the parity is P(A)*P(B), Thus: Baryons have P=1*1*1=1, antibaryons have P=1*1*1=1 (Anti)mesons have P=1*1 = 1 Excited states (with orbital angular momentum) Get an extra factor (1) l where l is the orbital L quantum number Note that parity formalism is parallel to total angular momentum J=L+S formalism, it has an intrinsic component and an orbital component NB: Photon is spin1 particle has intrinsic P of 1 Niels Tuning (63)
64 Parity eigenvalues for selected hadrons The p + meson Quark and antiquark composite: intrinsic P = (1)*(1) = 1 Orbital ground state no extra term P(p + )=1 The neutron Three quark composite: intrinsic P = (1)*(1)*(1) = 1 Orbital ground state no extra term P(n) = +1 Meaning: P p + > = 1 p + > Experimental proof: J.Steinberger (1954) πd nn n are fermions, so (nn) antisymmetric S d =1, S π =0 L nn =1 1) final state:p nn> = (1) L nn> = 1 nn> 2) init state: P d> = P pn> = (+1) 2 pn> = +1 d> To conserve parity: P π> = 1 π> The K 1 (1270) Quark antiquark composite: intrinsic P = (1)*(1) = 1 Orbital excitation with L=1 extra term (1) 1 P(K 1 ) = +1 Niels Tuning (64)
65 Figuring out C eigenvalues for hadrons Only particles that are their own antiparticles are C eigenstates because C x> x> = c x> E.g. p 0,h,h,r 0,f,w,y and photon C eigenvalues of quarkantiquark pairs is determined by L and S angular momenta: C = (1) L+S Rule applies to all above mesons C eigenvalue of photon is 1 Since photon is carrier of EM force, which obviously changes sign under C conjugation Example of C conservation: Process p 0 g g C=+1(p 0 has spin 0) (1)*(1) Process p 0 g g g does not occur (and would violate C conservation) Experimental proof of Cinvariance: BR(π 0 γγγ)< Niels Tuning (65)
66 This was an introduction to P and C Let s change gear Niels Tuning (66)
67 CP violation in the SM Lagrangian Focus on charged current interaction (W ± ): let s trace it u L I d L I g W +m Niels Tuning (67)
68 The Standard Model Lagrangian L L + L + L SM Kinetic Higgs Yukawa L Kinetic : Introduce the massless fermion fields Require local gauge invariance gives rise to existence of gauge bosons L Higgs : Introduce Higgs potential with <f> 0 Spontaneous symmetry breaking G SU(3) SU(2) U(1) SU(3) U(1) SM C L Y C Q The W +, W ,Z 0 bosons acquire a mass L Yukawa : Ad hoc interactions between Higgs field & fermions Niels Tuning (68)
69 Fields: Notation Fermions: 1 g5 1+ g5 y L y ; y R y 2 2 Y = Q  T 3 with y = Q L, u R, d R, L L, l R, n R Quarks: Under SU2: Left handed doublets Right hander singlets Leptons: u d I I I n I (3,2,1 6) (3,2,1 6) Li I u Ri (3,1,2 3) d I Ri (3,1, 1 3) l (1,2, 1 2) (1,2, 1 2) Li I l (1,1, 1) Ri I Q Li Lefthanded Interaction rep. SU(3) C SU(2) Hypercharge Y L generation index I n Ri (3,2,1 6) I L Li (1,2, 1 2) (=avg el.charge in multiplet) Scalar field: f (1, 2,1 2) + 0 Note: Interaction representation: standard model interaction is independent of generation number Niels Tuning (69)
70 Fields: Notation Q Y = Q T TY 3 Explicitly: The left handed quark doublet : Q I Li I I I I I I I I I ur, ug, u b cr, cg, c b tr, tg, t b (3,2,1 6),, I I I I I I I I I dr, dg, d b sr, sg, s b br, bg, b b L L L T T ( Y 16) Similarly for the quark singlets: u I Ri I I I I I I I I I ur ur ur c R r cr cr t R r tr tr R Y 23 I I I I I I I I I dr dr r sr sr r br br r Y 13 (3,1, 2 3),,,,,,,, I d (3,1, 1 3),, d,,, s,,, b Ri R R R The left handed leptons: L I I I n n 3 12 I e m n T + Li (1,2, 1 2),, Y  I I I e m T312 L L L 12 And similarly the (charged) singlets: l I (1,1, 1) e I, m I, I Y 1 Ri R R R Niels Tuning (70)
71 LSM L Kinetic + L Higgs + LYukawa :The Kinetic Part L Kinetic : Fermions + gauge bosons + interactions Procedure: Introduce the Fermion fields and demand that the theory is local gauge invariant under SU(3) C xsu(2) L xu(1) Y transformations. m Start with the Dirac Lagrangian: L iy ( g ) y m m m m m m D + ig G L + igw T + igb Y Replace: s a a b b m Fields: G m a : 8 gluons W m b : weak bosons: W 1, W 2, W 3 B m : hypercharge boson Generators: L a : GellMann matrices: ½ a (3x3) SU(3) C T b : Pauli Matrices: ½ b (2x2) SU(2) L Y : Hypercharge: U(1) Y For the remainder we only consider Electroweak: SU(2) L x U(1) Y Niels Tuning (71)
72 LSM L Kinetic + L Higgs + LYukawa : The Kinetic Part L kinetic m m : iy ( g ) y iy ( D g ) y m with y Q, u, d, L, l m I I I I I Li Ri Ri Li Ri For example, the term with Q Li I becomes: L m ( Q ) iq g D Q I I I kinetic Li Li m Li I m i m i m i m iq g m ( + gsg + gw + gb ) Q I Li a a b b Li Writing out only the weak part for the quarks: 0 I 2 Weak I I m i m m m u i Lkinetic( u, d) L iu, d g L m + g W1 1 + W2 2 + W3 3 2 d L 3 I m I I m I g I m I g I m I iulg m ul + idlg m dl  ulg mw  dl  dlg mw + ul u L I i d L I g W +m L=J m W m W + = (1/ 2) (W 1 + i W 2 ) W  = (1/ 2) (W 1 i W 2 ) Niels Tuning (72)
73 L L + L + L SM Kinetic Higgs Yukawa L 1 Dmf D f  V V m f f + f f 2 : The Higgs Potential 2 m 2 Higgs Higgs Higgs Symmetry 2 m 0: 0 V(f) f Broken Symmetry 2 m 0: 0 v 2 Vf f 2 v m ~ 246 GeV Spontaneous Symmetry Breaking: The Higgs field adopts a nonzero vacuum expectation value Procedure: e + imf f e + imf And rewrite the Lagrangian (tedious): (The other 3 Higgs fields are eaten by the W, Z bosons) Substitute: 0 e v+ H 2 1. G : SU. (3) SU(2) U(1) SU(3) U(1) 2. The W +,W ,Z 0 bosons acquire mass 3. The Higgs boson H appears SM C L Y C EM 0 Niels Tuning (73)
74 LSM LKinetic + LHiggs + LYukawa : The Yukawa Part Since we have a Higgs field we can (should?) add (adhoc) interactions between f and the fermions in a gauge invariant way. The result is: doublets singlet Li.. L + Yukawa Yij y f y Rj hc I I I ~ I I I Q f d.. Li Rj ij Q f u L j L f lrj h c Y + Y + Y i + d u l ij i Rj Li i, j : indices for the 3 generations! 0 1 f 0 * * With: f i 2 f f f  (The CP conjugate of f To be manifestly invariant under SU(2) ) Y, Y, Y d u l ij ij ij are arbitrary complex matrices which operate in family space (3x3) Flavour physics! Niels Tuning (74)
75 LSM LKinetic + LHiggs + LYukawa : The Yukawa Part Writing the first term explicitly: + d I I Yij ( ul, dl) i d 0 I Rj d I I d I I d I I Y11 ul, dl Y 0 12 ul, dl Y 0 13 ul, dl 0 I d R d I I d I I d I I I Y21 cl, sl Y 0 22 cl, sl Y 0 13 cl, sl 0 sr I br d I I d I I d I I Y31 tl, bl Y 0 32 tl, bl Y 0 33 tl, b L 0 Niels Tuning (75)
76 LSM LKinetic + LHiggs + LYukawa : The Yukawa Part There are 3 Yukawa matrices (in the case of massless neutrino s): Y, Y, Y d u l ij ij ij Each matrix is 3x3 complex: 27 real parameters 27 imaginary parameters ( phases ) many of the parameters are equivalent, since the physics described by one set of couplings is the same as another It can be shown (see ref. [Nir]) that the independent parameters are: 12 real parameters 1 imaginary phase This single phase is the source of all CP violation in the Standard Model Revisit later Niels Tuning (76)
77 L Yukawa S.S.B L Mass : The Fermion Masses Start with the Yukawa Lagrangian + d I I I u l LYuk Yij ( ul, dl ) i d Rj + Yij + ij 0... : v+ H S S B e 2 After which the following mass term emerges: L  L d M d + u M u I l I + l M l + h.. c Y I d I I u I Yuk Mass Li ij Rj Li ij Rj Li ij Rj with M v Y, M v Y, M v Y d d u u l l ij ij ij ij ij ij L Mass is CP violating in a similar way as L Yuk Niels Tuning (77)
78 L Yukawa S.S.B L Mass : The Fermion Masses Writing in an explicit form: I I I d u e I I I I I I I I I I I I d, s, b d s u, c, t u M M c e, m, M l  L m h. c. Mass + + L L L + I I I b t V M V M f f f f L R diagonal R The matrices M can always be diagonalised by unitary matrices V L f and V R f Then the real fermion mass eigenstates are given by: d I d V L VR d d d d I Li ij Lj Ri ij Rj u I u V L VR u u u u I Li ij Lj Ri ij Rj l I l V i V l l l l I Li L ij Lj R R ij Rj d I L, u I L, l I L are the weak interaction eigenstates d L, u L, l L are the mass eigenstates ( physical particles ) R f,, VL V L M V R R such that: d d s b V s b I I I f f f f I R L I Niels Tuning (78) I R
79 L Yukawa S.S.B L Mass : The Fermion Masses In terms of the mass eigenstates: md d mu u LMass d, s, b ms s u, c, t m c L + t L c L m b b m R t me e + e, m, mm m h. c. L + m m uu + m cc + m tt Mass u c t + m dd + m ss + m bb d s b + m ee + m mm + m e m In flavour space one can choose: Weak basis: The gauge currents are diagonal in flavour space, but the flavour mass matrices are nondiagonal Mass basis: The fermion masses are diagonal, but some gauge currents (charged weak interactions) are not diagonal in flavour space In the weak basis: L Yukawa = CP violating In the mass basis: L Yukawa L Mass = CP conserving R R What happened to the charged current interactions (in L Kinetic )? Niels Tuning (79)
80 LW L CKM : The Charged Current The charged current interaction for quarks in the interaction basis is: L The charged current interaction for quarks in the mass basis is: L L W W W g 2 g 2 g 2 u V Li I Li g u m d L L Li The unitary matrix: V u d CKM VL VL d u c t V L CKM s b,, V d W is the Cabibbo Kobayashi Maskawa mixing matrix: n l Lepton sector: similarly VMNS VL VL u g m d I Li L W + m With: However, for massless neutrino s: V n L = arbitrary. Choose it such that V MNS = 1 There is no mixing in the lepton sector g m + m W + m V CKM V CKM 1 Niels Tuning (80)
81 L Charged Currents g I m I g I m I m m u g W d + d g W u J W + JCC W CC Li m Li Li m Li CC m m L The charged current term reads: g 1g 1g g 1g 1g u W d + d W u g m  5 g m + * 5 uig WmVij 1 g d j + d jg WmVi j 1 g ui m  m + i g mvij j j g mvji i Under the CP operator this gives: CP g m + 5 g m i * 5 d g WmVij 1 g u + u g WmVij 1 g d 2 2 CC j i i j A comparison shows that CP is conserved only if V ij = V ij * (Together with (x,t) > (x,t)) In general the charged current term is CP violating Niels Tuning (81)
82 The Standard Model Lagrangian (recap) LSM L Kinetic + L Higgs + LYukawa L Kinetic : Introduce the massless fermion fields Require local gauge invariance gives rise to existence of gauge bosons CP Conserving L Higgs : Introduce Higgs potential with <f> 0 Spontaneous symmetry breaking CP Conserving G SU(3) SU(2) U(1) SU(3) U(1) SM C L Y C Q The W +, W ,Z 0 bosons acquire a mass L Yukawa : Ad hoc interactions between Higgs field & fermions CP violating with a single phase L Yukawa L mass : fermion weak eigenstates:  mass matrix is (3x3) nondiagonal fermion mass eigenstates:  mass matrix is (3x3) diagonal CPviolating CPconserving! L Kinetic in mass eigenstates: CKM matrix CP violating with a single phase Niels Tuning (82)
83 LSM LKinetic + LHiggs + LYukawa Recap + d I I I LYuk Yi j ( ul, dl ) i d... 0 Rj + L g I m  I g I m + I u g Wmd + dlig WmuL i Kinetic Li Li Diagonalize Yukawa matrix Y ij Mass terms Quarks rotate Off diagonal terms in charged current couplings I d d I s VCKM s I b b md d mu u LMass d, s, b ms s u, c, t mc c... L + L + m b b m t t L g m  5 g m + * 5 u g WmVij 1 g d + d g WmVi 1  g u CKM i j j j i R L L + L + L SM CKM Higgs Mass R Niels Tuning (83)
84 Ok. We ve got the CKM matrix, now what? It s unitary probabilities add up to 1 : d =0.97 d s b ( =1) How many free parameters? How many real/complex? How do we normally visualize these parameters? Niels Tuning (84)
85 Personal impression: People think it is a complicated part of the Standard Model (me too:). Why? 1) Nonintuitive concepts? Imaginary phase in transition amplitude, T ~ e iφ Different bases to express quark states, d =0.97 d s b Oscillations (mixing) of mesons: K 0 > K 0 > 2) Complicated calculations? 3) Many decay modes? Beetopaipaigamma B f A 2 f g+ t g t 2 g+ t g t B f Af g+ t g 2  t 2 g+ t g t + + PDG reports 347 decay modes of the B 0 meson: Γ 1 l + ν l anything ( ± 0.28 ) 10 2 Γ 347 ν ν γ < CL=90% And for one decay there are often more than one decay amplitudes Niels Tuning (85)
86
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