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Particle Physics II

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Title: Particle Physics II


1
Particle Physics II CP violationLecture 1
  • N. Tuning

2
Outline
  • 1 May
  • Introduction matter and anti-matter
  • P, C and CP symmetries
  • K-system
  • CP violation
  • Oscillations
  • Cabibbo-GIM mechanism
  • 8 May
  • CP violation in the Lagrangian
  • CKM matrix
  • B-system
  • 15 May
  • B-factories
  • B?J/Psi Ks
  • Delta ms

3
Literature
  • Slides based on the course from Wouter Verkerke.
  • W.E. Burcham and M. Jobes, Nuclear and Particle
    Physics, chapters 11 and 14.
  • Z. Ligeti, hep-ph/0302031, Introduction to Heavy
    Meson Decays and CP Asymmetries
  • Y. Nir, hep-ph/0109090, CP Violation A New Era
  • H. Quinn, hep-ph/0111177, B Physics and CP
    Violation

4
Motivation What is so interesting about CP
violation?
  • Its about differences in matter and anti-matter
  • Why would they be different in the first place?
  • We see they are different our universe is matter
    dominated

5
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
  • You need a process that violates the baryon
    number B(Baryon number of matter1, of
    anti-matter -1)
  • Both C and CP symmetries should be violated
  • 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

6
What is evidence for the existence of anti-matter?
  • Energetic photons produced in matter/anti-matter
    annihilation
  • Look at spectrum of photons in universe and look
    for spikes
  • Main problem photons can not travel unlimited
    distances in the universe because of interactions
    with remaining cosmic background radiation and
    gases etc
  • Conclusion No anti-matter in 20Mpc radius.
  • How to look further into space?
  • Better Look for anti-Helium nuclei flying
    through space
  • Positrons, anti-protons can occasionally be
    produced in various processes, but producing
    anti-Helium is way too complicated by regular
    means Only viable source of anti-Helium are
    fusion processes in anti-stars
  • Presence/absence of anti-Helium says something
    about existence of anti-matter in distant regions
    of space
  • Large rest mass of Helium nuclei allows them to
    travel much further through space than photons ?
    Conclusions of anti-Helium searches cover much
    larger region of space

7
The AMS experiment Searching for He
  • In essence as small particle physics experiment
    in space
  • AMS-01 brought to space through flight of
    Discovery shuttle
  • Can detect and identify many types of cosmic rays

8
Results of the AMS experiment
  • Zero anti-helium found, plenty of Helium found
  • Rigidity of tracks is measure of particles
    momentum
  • Very high energy Helium nuclei have traveled from
    far ? Says something about spatial reach of
    experiment
  • Universe with pockets of anti-matter hypothesis
    increasingly unlikely
  • Future AMS-02 experiment will (launch 2007) will
    have much increased range

9
Introduction positron discovery by Anderson
  • Result discovery of a positively charged
    electron-like particle dubbed the positron
  • Experimental confirmation of existence of
    anti-matter!

Outgoing particle (low momentum / hi curvature)
Lead plate to slow down particlein chamber
Incoming particle (high momentum / low curvature)
10
Introduction positron discovery by Anderson
  • 4 years later Anderson confirmed this with g ?
    ee- in lead plate using g from Thorium carbide
    source

11
Introduction anti-neutrino Savannah river
  • Decisive experiment close to Savannah River
    nuclear reactor in South Carolina in 1956 (Nobel
    prize 1995)
  • Idea nuclear reactor provides enormous
    anti-neutrino flux from fission O(1013) /cm2/sec
  • Try to detect inverse beta decay n p ? n e

(Beta decay n ? p e- n)
n e ? p n p n ? n e
Cross over e-
Invert reaction
12
Introduction anti-neutrino Savannah river
  • How do you detect n p ? n e
  • Look for the positron through the reaction
    e e- ? g gand detect 2 photons produced
    simultaneously.
  • Savannah river Detector
  • Tank with 200 liters of water with 40 kg of CdCl2
    dissolved in it.
  • Surrounded by 110 photomultipliers for photon
    detection
  • Clean signal found ? direct proof of existence of
    neutrino
  • Nobel prize 1995
  • ?? n ? p e- not observed
  • ????? , Lepton number must be conserved

From inversebeta decay
From detectormaterial
13
Introduction - What about the other
anti-particles?
  • Dirac equation for every (spin ½) particle there
    is an anti-particle
  • It took a bit longer, but more were
    discoveredAnti-proton (1955) and anti-neutron
    (1955) using cyclotrons
  • Reactions with particles and anti-particles
  • Q How do you produce anti-particles anyway?
  • A In pairs with particles, e.g. g ? e e-
  • But this is not the whole story as we will see
    later
  • General rule crossing symmetry
  • In any existing reaction you can move a particle
    through the arrow while turning it into an
    anti-particle
  • Example e- g ? e- g (Compton scattering) g g
    ? e e- (Pair creation)

Move e- to right Move g to left(g g)
14
Definition and discovery of C,P,CP violation
15
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

16
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 15o and 40o 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.

17
Three Discrete Symmetries
  • Parity, P
  • Parity reflects a system through the origin.
    Convertsright-handed coordinate systems to
    left-handed 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
    anti-particle
  • e ? e- , K - ? K
  • Time Reversal, T
  • Changes, for example, the direction of motion of
    particles
  • t ? -t

18
P-parity experiments
  • Before 1956 physicists were convinced that the
    laws of nature were left-right symmetric.
    Strange?
  • A gedanken experiment Consider two perfectly
    mirror symmetric cars
  • What would happen if the ignition mechanism uses,
    say, 60Co b decay?

Gas pedal
Gas pedal
driver
driver
L and R are fully symmetric, Each nut, bolt,
molecule etc. However the engine is a black box
R
L
Person L gets in, starts, .. 60 km/h
Person R gets in, starts, .. What happens?
19
The situation in 1956
  • Nothing hints at the existence of any kind of
    Parity violating physics
  • Reminder Parity (x,y,z) ? (-x,-y,-z)
  • If universe is parity-symmetric, inverting all
    spatial coordinates would not changes laws of
    physics
  • 1956 Lee and Yang publish a paper Question of
    Parity Conservation in Weak Interactions/
  • Suggestion Weak interaction might violate Parity
    symmetry.
  • Originated from discussions at April HEP
    conference in Rochester, NY. Following Yang's
    presentation Richard Feynman brought up the
    question of non-conservation of parity.
  • Feynman himself later said, "I thought the idea
    (of parity violation) unlikely, but possible, and
    a very exciting possibility." Indeed Feynman
    later made a fifty dollar bet with a friend that
    parity would not be violated.

20
Parity symmetry The situation in 1956
  • When the paper appeared, physicists were not
    immediately prompted into action. The proposition
    of parity non-conservation was not unequivocally
    denied rather, the possibility appeared so
    unlikely that experimental proof did not warrant
    immediate attention.
  • The physicist Freeman Dyson wrote of his reaction
    to the paper "A copy of it was sent to me and I
    read it. I read it twice. I said, This is very
    interesting,' or words to that effect. But I had
    not the imagination to say, By golly, if this is
    true it opens up a whole new branch of physics.'
    And I think other physicists, with very few
    exceptions, at that time were as unimaginative as
    I."

21
Parity symmetry the experiment
  • Madame Wu
  • Another immigrant was now to play the next major
    role, Madame Chien-Shiung Wu.
  • Arriving at Berkely in 1936 from Shanghai, Wu was
    one of the most ardently pursued coeds on
    campus. But she was also a hard worker who
    abhorred the marked absence of women from the
    American scientific establishment. She says, "
    ... it is shameful that there are so few women
    in science... In China there are many, many
    women in physics. There is a misconception in
    America that women scientists are all dowdy
    spinsters. This is the fault of men. In Chinese
    society, a woman is valued for what she is, and
    men encourage her to accomplishments --- yet she
    retains eternally feminine."
  • Idea from experiment in collaboration with Lee
    and Yang Look at spin of decay products of
    polarized radioactive nucleus
  • Production mechanism involves exclusively weak
    interaction

22
Intermezzo Spin and Parity
  • How does the decay of a particle with spin tell
    you something about parity?
  • Gedanken-experiment decay of X ? a b
  • Spin 1,1gt ? ½, ½ gt ½, ½gt
  • It is important that X is maximally polarized
    only then there is a single solution for the spin
    of the decay products. If not, e.g.
  • 1,0gt ? ½, ½gt ½, -½gt
  • 1,0gt ? ½, -½gt ½, ½gt

?
23
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

H1 (right-handed)
H-1 (left-handed)
24
Intermezzo Spin and Parity and Helicity
  • Spin is quantized ? Helicity is quantized
  • Possible H values for S1/2 H-1 and H1
  • Most particles are linear combination of H1 and
    H-1 states
  • Angular distribution for particles observed in
    specific helicity eigenstate

I(q)RH 1 - (v/c) cos q
I(q)LH 1 (v/c) cos q

ConstantIf both helicitiesare producedequally
in decay.If not angulardistribution willnot
be flat
Superpositionof H1 and H-1states
25
Note on Helicity
  • Note that Helicity is not generally a Lorentz-
    invariant observable
  • Sign of particle momentum p is relative to
    observer.
  • A second observer overtaking the particle from
    the lab observer perspective will see the
    particle moving in the opposite direction (p
    -p) ? It see the opposite Helicity
  • Exception for massless particles
  • You cannot overtake massless particles moving at
    speed of light
  • Helicity for massless particles is
    Lorentz-invariant intrinsic property

26
A realistic experiment the Wu experiment (1956)
  • Observe radioactive decay of Cobalt-60 nuclei
  • The process involved 6027Co ? 6028Ni e- ne
  • 6027Co is spin-5 and 6028Ni is spin4, both e- and
    ne are spin-½
  • If you start with fully polarized Co (SZ5) the
    experiment is essentially the same (i.e. there is
    only one spin solution for the decay) 5,5gt ?
    4,4gt ½ ,½gt ½,½gt

S4
27
The Wu experiment 1956
  • Experimental challenge how do you obtain a
    sample of Co(60) where the spins are aligned in
    one direction
  • Wus solution adiabatic demagnitization of
    Co(60) in magnetic fields at very low
    temperatures (1/100 K!). Extremely challenging
    in 1956!

28
The Wu experiment 1956
  • The surprising result the counting rate is
    different
  • Electrons are preferentially emitted in direction
    opposite of 60Co spin!
  • Careful analysis of results shows that
    experimental data is consistent with emission of
    left-handed (H-1) electrons only at any angle!!

Backward Counting ratew.r.t unpolarized rate
60Co polarization decreasesas function of time
Forward Counting ratew.r.t unpolarized rate
29
The Wu experiment 1956
  • Physics conclusion
  • Angular distribution of electrons shows that only
    pairs of left-handed electrons / right-handed
    anti-neutrinos are emitted regardless of the
    emission angle
  • Since right-handed electrons are known to exist
    (for electrons H is not Lorentz-invariant
    anyway), this means no left-handed
    anti-neutrinos are produced in weak decay
  • Parity is violated in weak processes
  • Not just a little bit but 100
  • How can you see that 60Co violates parity
    symmetry?
  • If there is parity symmetry there should exist no
    measurement that can distinguish our universe
    from a parity-flipped universe, but we can!

30
Our universe vs a parity-flipped universe
  • What happens to helicity in parity-flipped
    universe?
  • Momentum flips sign
  • Spin stays the same
  • Helicity is product and flips sign
  • Conclusion
  • Any process that produces right-handed
    anti-neutrinos in our universe will produce
    left-handed anti-neutrinos in the mirrored
    universe.
  • If left and right-handed neutrinos are not
    produced at the same rate the physics in the
    mirrored universe is different

Orientation of spin
righthanded H1
Direction of motion
P
lefthanded H-1
Orientation of spin
Direction of motion
31
Parity violation in weak decays
  • Apply parity operation to 60Co decay

P-Flipped universe
Our universe
RH ne
RH ne
e-
e-
LH ne
LH ne
e-
e-
32
Parity violation in weak decays
  • Apply parity operation to 60Co decay

P-Flipped universe(LH anti-neutrinos only)
Our universe(RH anti-neutrinos only)
Allowed
Forbidden
Allowed
Forbidden
RH ne
RH ne
e-
e-
LH ne
LH ne
e-
e-
Preferential direction of electronsis forward
Preferential direction of electronsis backward
33
So P is violated, whats next?
  • Wus experiment was shortly followed by another
    clever experiment by L. Lederman Look at decay
    p ? m nm
  • Pion has spin 0, m,nm both have spin ½ ? spin of
    decay products must be oppositely aligned ?
    Helicity of muon is same as that of neutrino.
  • Nice feature can also measure polarization of
    both neutrino (p decay) and anti-neutrino (p-
    decay)
  • Ledermans result All neutrinos are left-handed
    and all anti-neutrinos are right-handed

p
m
nm
34
Charge conjugation symmetry
  • Introducing C-symmetry
  • The C(harge) conjugation is the operation which
    exchanges particles and anti-particles (not just
    electric charge)
  • It is a discrete symmetry, just like P, i.e. C2
    1
  • C symmetry is broken by the weak interaction,
  • just like P

OK
p
m
nm(LH)
C
nm(LH)
p-
m-
OK
35
The Weak force and C,P parity violation
  • What about CP ? CP symmetry?
  • CP symmetry is parity conjugation (x,y,z ?
    -x,-y,z)
  • followed by charge conjugation (X ? X)

?
??
??
P
C
CP appears to be preservedin weakinteraction!
?
?
??
??
?
??
CP
36
What do we know now?
  • C.S. Wu discovered from 60Co decays that the weak
    interaction is 100 asymmetric in P-conjugation
  • We can distinguish our universe from a parity
    flipped universe by examining 60Co decays
  • L. Lederman et al. discovered from p decays that
    the weak interaction is 100 asymmetric in
    C-conjugation as well, but that CP-symmetry
    appears to be preserved
  • First important ingredient towards understanding
    matter/anti-matter asymmetry of the universe
    weak force violates matter/anti-matter(C)
    symmetry!
  • C violation is a required ingredient, but not
    enough as we will learn later
  • Next a precision test of CP symmetry
    conservation in the weak interaction

37
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 hadronPygt pygt
  • 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 P1 then Pygt 1ygt (wave function
    symmetric in space)if P-1 then Pygt -1 ygt
    (wave function anti-symmetric in space)

38
Figuring out P eigenvalues for hadrons
  • QFT rules for particle vs. anti-particles
  • Parity of particle and anti-particle must be
    opposite for fermions (spin-N1/2)
  • Parity of bosons (spin N) is same for particle
    and anti-particle
  • Definition of convention (i.e. arbitrary choice
    in def. of q vs q)
  • Quarks have positive parity ? Anti-quarks 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 P1111, anti-baryons have
    P-1-1-1-1
  • (Anti-)mesons have P1-1 -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 JLS formalism, it has an
    intrinsic component and an orbital component
  • NB Photon is spin-1 particle has intrinsic P of
    -1

39
Parity eigenvalues for selected hadrons
  • The p meson
  • Quark and anti-quark 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
  • The K1(1270)
  • Quark anti-quark composite intrinsic P
    (1)(-1) -1
  • Orbital excitation with L1 ? extra term (-1)1
  • P(K1) 1

Meaning Ppgt -1pgt
40
Figuring out C eigenvalues for hadrons
  • Only particles that are their own anti-particles
    are C eigenstates because Cxgt ? xgt cxgt
  • E.g. p0,h,h,r0,f,w,y and photon
  • C eigenvalues of quark-anti-quark pairs is
    determined by L and S angular momenta C
    (-1)LS
  • 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 p0 ? g g C1(p0 has spin 0) ?
    (-1)(-1)
  • Process p0 ? g g g does not occur (and would
    violate C conservation)

41
Introduction to K0 physics
  • Now focusing on another little mystery in the
    domain of strange mesons what precisely is a
    K0 meson?
  • Quark contents K0 ?sd,?K0 ?ds
  • First what is the effect of C and P conjugation
    on the K0/K0-bar particles?
  • PK0gt -1K0gt (because ?qq pair)
  • PK0gt -1K0gt (because ?qq pair)
  • CK0gt K0gt (because K0 is anti-particle of K0
    ls0)
  • CK0gt K0gt (because K0 is anti-particle of K0
    ls0)
  • Knowing this we can evaluate the effect of CP on
    the K0
  • CPK0gt -1K0gt
  • CPK0gt -1 K0gt

42
What are the K0 CP Eigenstates
  • Thus K0 and K0 are not CP eigenstates,
  • Somewhat strange since they decay through weak
    interaction which appears to conserve CP!
  • Nevertheless it is possible to construct CP
    eigenstates as linear combinations
  • Remember QM You can always construct wave
    functions as linear combinations of the solutions
    of any operator (like the Hamiltonian)
  • K1gt 1/?2(K0gt - K0gt)
  • K2gt 1/?2(K0gt K0gt)
  • Proof is exercise for today
  • Does it make sense to look at linear combinations
    of K0gt and K0gt?
  • I.e does K1gt represent a real particle?

43
K0/K0 oscillations
  • Well it might, because it turns out that the weak
    interaction can turn a K0 particle into a K0
    particle!
  • Weird? Yes! Impossible? No!
  • In can be done using two consecutive weak
    interactions
  • Important implication for nature of K0 particle
  • Q If a K0 can turn into a K0 at any moment, how
    do you know what particle youre dealing with?
  • A You dont. Any particle in the lab is always a
    linear combination of the two ? It makes as much
    sense to talk about K1 and K2 eigenstates as it
    does to talk about K0 and K0 eigenstates

Weak force
Weak force
K0
(X)
K0
S1
S0
S-1
DS-1
DS-1
44
So what is the K0 really?
  • The K0 meson is something you can only describe
    with quantum mechanics
  • It is a linear combination of two particles!
  • You can either see it as a combination of K0gt
    and ?K0gt,eigenvalues of Strangeness (1 vs 1)
    and undefined CP
  • Or you can see it as a combination of K1gt and
    K2gt,eigenvalues of CP (1, -1), with undefined
    strangeness
  • Both representations are equivalent.
  • Kaons are typically produced in strong
    interactions in a strangeness eigenstate (K0 or
    ?K0)
  • Kaons decay through the weak interaction as
    eigenstates of CP (K1 or K2)
  • Since K1 and K2 dont have definite S, S is not
    conserved in weak decays as we already know
  • If you believe a particle must have a single well
    defined lifetime, then K1 and K2 are the real
    particles

45
So what is the K0 really?
  • Graphical analogy Any object with two
    components can be decomposed in more than one way

Anti-K0
K2
Kgt
K0
K1
46
Decays of neutral kaons
  • Neutral kaons is the lightest strange particle ?
    it must decay through the weak interaction
  • If weak force conserves CP then
  • decay products of K1 can only be a CP1 state,
    i.e.K1gt (CP1) ? p p (CP
    (-1)(-1)(-1)l0 1)
  • decay products of K2 can only be a CP-1 state,
    i.e.K2gt (CP-1) ? p p p (CP
    (-1)(-1)(-1)(-1)l0 -1)
  • You can use neutral kaons to precisely test that
    the weak force preserves CP (or not)
  • If you (somehow) have a pure CP-1 K2 state and
    you observe it decaying into 2 pions (with CP1)
    then you know that the weak decay violates CP

( S(K)0 ? L(pp)0 )
47
Designing a CP violation experiment
  • How do you obtain a pure beam of K2 particles?
  • It turns out that you can do that through clever
    use of kinematics
  • Exploit that decay of K into two pions is much
    faster than decay of K into three pions
  • Related to fact that energy of pions are large in
    2-body decay
  • t1 0.89 x 10-10 sec
  • t2 5.2 x 10-8 sec (600 times larger!)
  • Beam of neutral Kaons automatically becomes beam
    of K2gt as all K1gt decay very early on

K1 decay early (into pp)
Pure K2 beam after a while!(all decaying into
ppp) !
Initial K0 beam
48
The Cronin Fitch experiment
Essential idea Look for (CP violating) K2 ? pp
decays 20 meters away from K0 production point
Decay of K2 into 3 pions
Incoming K2 beam
If you detect two of the three pionsof a K2 ?
ppp decay they will generallynot point along the
beam line
49
The Cronin Fitch experiment
Essential idea Look for K2 ? pp decays20 meters
away from K0 production point
Decay pions
Incoming K2 beam
If K2 decays into two pions instead ofthree both
the reconstructed directionshould be exactly
along the beamline(conservation of momentum in
K2 ? pp decay)
50
The Cronin Fitch experiment
Essential idea Look for K2 ? pp decays20 meters
away from K0 production point
Decay pions
K2 ? pp decays(CP Violation!)
Incoming K2 beam
K2 ? ppp decays
Result an excess of events at Q0 degrees!
Note scale 99.99 of K ?ppp decaysare left of
plot boundary
51
Cronin Fitch Discovery of CP violation
  • Conclusion weak decay violates CP (as well as C
    and P)
  • But effect is tiny! (0.05)
  • Maximal (100) violation of P symmetry easily
    follows from absence of right-handed neutrino,
    but how would you construct a physics law that
    violates a symmetry just a tiny little bit?
  • Results also provides us withconvention-free
    definition ofmatter vs anti-matter.
  • If there is no CP violation, the K2 decaysin
    equal amounts to p e- ne (a) p- e ne (b)
  • Just like CPV introduces K2 ? pp decays, it also
    introduces a slight asymmetry in the above
    decays (b) happens more often than (a)
  • Positive charge is the charged carried by the
    lepton preferentially produced in the decay of
    the long-lived neutral K meson

52
Kaons K0,?K0, K1, K2, KS, KL,
  • The kaons are produced in mass eigenstates
  • K0gt ?sd
  • ?K0gt ?ds
  • The CP eigenstates are
  • CP1 K1gt 1/?2 (K0gt - ?K0gt)
  • CP -1 K2gt 1/?2 (K0gt ?K0gt)
  • The kaons decay to 2 (Short-lived) or 3 pions
    (Long-lived)
  • KSgt predominantly CP1
  • KLgt predominantly CP -1
  • ?- (2.286 0.014) x 10-3
  • e (2.284 0.014) x 10-3

53
What do we know now?
  • C and P are both violated by the weak interaction
    because neutrinos can only be produced in a
    single helicity state (LH neutrinos and RH
    anti-neutrinos)
  • Results from Wu and Lederman experiments
  • You can associate a P quantum number to all
    hadrons and a C quantum number to all hadrons
    that are their own anti-particle
  • These C and P quantum numbers are conserved in
    any reaction not involving the weak interaction
  • The K0 meson is a special particle that really
    exists as a combination of two particle the K0 /
    K0 combination or the K1 / K2 combination at your
    choice
  • The Cronin and Fitch experiment shows that in
    addition to C and P violation the product CP is
    also violated, but only a tiny little bit
  • Origin of CP violation sofar unknown ? Topic of
    future section

54
Schematic picture of selected weak decays
  • K0 ? K0 transition
  • Note 1 Two W bosons required (DS2 transition)
  • Note 2 many vertices, but still lowest order
    process

?s
?d
W
u
u
K0
K0
W
s
d
55
Strangeness violation in W mediated decays
  • In 1963 N. Cabibbo made the first step to
    formally incorporate strangeness violation in W
    mediated decays
  • For the leptons, transitions only occur within a
    generation
  • For quarks the amount of strangeness violation
    can be neatly described in terms of a rotation,
    where qc13.1o

Weakforcetransitions
u
Idea weak interaction couples to different
eigenstates than strong interactionweak
eigenstates can be writtenas rotation of
strongeigenstates
W
d d?cosqc s?sinqc
56
Cabibbos theory successfully correlated many
decay rates
  • Cabibbos theory successfully correlated many
    decay rates by counting the number of cosqc and
    sinqc terms in their decay diagram

57
Cabibbos theory successfully correlated many
decay rates
  • There was however one major exception which
    Cabibbo could not describe K0 ? m m-
  • Observed rate much lower than expected from
    Cabibbos ratecorrelations (expected rate ?
    g8sin2qccos2qc)

d
?s
cosqc
sinqc
u
W
W
nm
m
m-
58
The Cabibbo-GIM mechanism
  • Solution to K0 decay problem in 1970 by Glashow,
    Iliopoulos and Maiani ? postulate existence of
    4th quark
  • Two up-type quarks decay into rotated
    down-type states
  • Appealing symmetry between generations

u
c
W
W
dcos(qc)dsin(qc)s
s-sin(qc)dcos(qc)s
59
The Cabibbo-GIM mechanism
  • Cabibbo-GIM mechanism introduces clean formalism
    for quark flavour violations in the weak
    interactionThe weak interaction (W boson)
    couples to a rotated set of down-type
    states
  • Tiny problem at time of introduction there was
    no evidence for a 4th quark
  • Fourth charm quark discovered in 1974 ?
    Vindication of Cabbibo/GIM mechanism

Leptonsectorunmixed
Quark section mixed throughrotation of weak
w.r.t. strong eigenstates by qc
60
The Cabibbo-GIM mechanism
  • How does it solve the K0 ? mm- problem?
  • Second decay amplitude added that is almost
    identical to original one, but has relative minus
    sign ? Almost fully destructive interference
  • Cancellation not perfect because u, c mass
    different

d
?s
?s
d
-sinqc
cosqc
cosqc
sinqc
c
u
nm
nm
m
m-
m
m-
61
From 2 to 3 generations
  • 2 generations d0.97 d 0.22 s (?c13o)
  • 3 generations d0.97 d 0.22 s 0.003 b
  • NB probabilities have to add up to 1
    0.9720.2220.00321
  • ? Unitarity !

62
What do we know about the CKM matrix?
  • Magnitudes of elements have been measured over
    time
  • Result of a large number of measurements and
    calculations

Magnitude of elements shown only, no information
of phase
63
How do you measure those numbers?
  • Magnitudes are typically determined from ratio of
    decay rates
  • Example 1 Measurement of Vud
  • Compare decay rates of neutrondecay and muon
    decay
  • Ratio proportional to Vud2
  • Vud 0.9735 0.0008
  • Vud of order 1

64
  • End of Lecture 1
  • 1 May
  • Introduction matter and anti-matter
  • P, C and CP symmetries
  • K-system
  • CP violation
  • Oscillations
  • Cabibbo-GIM mechanism
  • 8 May
  • CP violation in the Lagrangian
  • CKM matrix
  • B-system
  • 15 May
  • B-factories
  • B?J/Psi Ks
  • Delta ms

65
Exercises Spin in decay helicity
  • Decay topology consider the process
    6027Co?6028Nie-??e where the e and the?? are
    emitted along the polarization (z) axis. (See
    illustration.) We are now interested in the
    orientation of the spin of the electron/anti-neutr
    ino w.r.t to the direction of flight.
  • Show that there are two possibilities for decays
    along the 60Co spin axis
  • one where the electron spin points to the same
    direction has the direction of motion and
  • one where the electron spin points to the
    opposite direction of the direction of motion
  • What are the helicities of the electron and
    anti-neutrino for the twoemission possibilites,
    respectively. (Helicity is defined as
    )

66
Exercise Pion decay p-? l-??l
  • Given a p- (spin 0) in rest that decays into a m-
    and a ??m (both spin ½)
  • Draw the decay for both spin orientation
    possibilities
  • What is the helicity of the anti-neutrino for
    both possibilities?
  • Which of the two processes does not occur in
    nature?
  • Draw the C-conjugated diagram of the p decay
    that occurs in nature. Does the C-conjugated
    process occur in nature? Explain why (not)?
  • Draw the C and P conjugated diagram of the p-
    decay that occurs in nature. Does this decay
    occur in nature?
  • Can the following decay occur p-? e-??e ?
  • The (V-A) theory predicts that the decay rate
    G(p-? l-??l ) is proportional to the two-body
    phase space factor multiplied by (1-v/c) , where
    v is the speed of the lepton in the pion rest
    frame. Derive the phase space factor (p2dp/dE),
    where p is the lepton momentum and E the total
    energy in the pion rest frame.
  • Estimate the ratio of branching ratios G(p-?
    e-??e ) /G(p-? µ-??µ)

67
Exercises CP Eigenstates of the K0
  • Consider K1 and K2
  • K1gt 1/?2(K0gt - ?K0gt)
  • K2gt 1/?2(K0gt ?K0gt)
  • Prove that K1 and K2 are eigenstates of the CP
    operation and determine the eigenvalues of K1 and
    K2.
  • Given CP conservation, how do K1 and K2 decay?
  • Why is the lifetime of K2 so much larger?
    (mpi140 MeV, mK490MeV)
  • In the experiment of Cronin and Fitch, a beam of
    almost only K2 particles is produced from a beam
    K0 particles by placing the experiment 20 meters
    away from the K0 production point so that most K1
    particles will have decayed.
  • The distribution of K1 decay distances is an
    exponential distribution so even after 20 meters
    there will be a few K1 left. It is important to
    know how many such decays there are as a K1 decay
    in the detector is indistinguishable from a K2
    decaying (with CP violation) into two pions.
  • Given that the decay time of the K2 is 5.2 x 10-8
    sec, what fraction of the K2 has not decayed yet
    after 20 meters (assume v ? c)
  • Given that the decay time of the K1 is t1 0.89
    x 10-10 sec, what fraction of the K1 has not
    decayed yet after 20 meters
  • What is the ratio of K1 to K2 decays after 20
    meters
  • How many K0 particles need to be produced to
    measure 22700 K2 decays between 20 and 21 meters
    of flight with a 1 detection efficiency for
    particles decaying in that one-meter stretch?

68
Exercise Weak decay diagrams
  • Feynman diagrams for weay decays
  • Draw the diagram for p decay.
  • Indicate the CKM matrix element labels at each
    weak vertex
  • Draw the diagram for L0 ? pnee decay
  • Indicate the CKM matrix element labels at each
    weak vertex
  • Draw two (topologically different) diagrams for
    the K0 ? K0 transition
  • Indicate the CKM matrix element labels at each
    weak vertex
  • Both diagram may have at most 4 vertices
  • Hint One was shown in the course material.

69
Solutions
70
Solution to exercises
  • Exercise 1
  • The two possible configurationsare shown on the
    right. The blackarrows show the orientation
    ofthe spin. The red dashed arrowsshow the
    direction of motion
  • In the left scenario H(e)1, H(n)-1In the
    right scenarioH(e)-1, H(n)1
  • See book

e-
ne
S1/2
S4
S4
ne
e-
S1/2
71
Solution to exercises
  • Exercise 2
  • See below
  • Top H(n) RH, Bottom H(n)LH
  • Only the top process occurs in nature (there
    exist only left-handed neutrinos and right-handed
    anti-neutrinos)

p-
m-
nm
72
Solution to exercises
  • Exercise 2 continued
  • The C-conjugated diagram of the p- decay that
    occurs in nature is
  • The C conjugated process does not occur in
    nature, as it features a right-handed neutrino.
  • The CP conjugated diagram of the p- decay that
    occurs in nature is
  • This process does occur in nature, just like in
    the original p- decay process, because it
    features a left-handed neutrino. CP therefore
    appears to be a conserved symmetry in the weak
    interaction

p
m
nm
p
m
nm
73
Solution to exercises
  • Exercise 2 continued
  • Yes, but is surpressed! e- wants to be left
    handed because it is almost massless.
  • See book

74
Solution to exercises
  • Exercise 3
  • Start with the known CP properties of the K0 and
    K0
  • PK0gt -K0gt, because quark-antiquark gives
    (1)(-1)(-1) and S,L0
  • CPK0gt C(-K0gt) -1K0gt
  • CPK0gt -1 K0gt
  • To prove that K1gt is an eigenvalue of CP we
    should show that the CP operation on K1gt yields
    a constant times K1gt.Calculate effect of CP on
    K1gt (omitting norm factor 1/?2)
  • CP(K0gt - K0gt) (-K0gt K0gt) 1(K0gt -
    K0gt) 1K1gt
  • Same thing for K2gt
  • CP(K0gt K0gt) (-K0gt - K0gt) -1(K0gt
    K0gt) -1K2gt
  • K1 ? pipi, K2?pipipi
  • 3 times pion mass is almost kaon mass hardly any
    phase space!

75
Solution to exercises
  • Exercise 3 continued
  • Distribution of decays follows f(t)exp(-t/t)
    with t5.2x10-8.To calculate the fraction that
    decays after 20 meters we need to calculate the
    fraction that decays after 20m/c 6.6x10-8 sec
  • The primitive of f(t) is F(t) -t exp(-t/t)
    F(0) -t -5.2x108, F(?)0,
    F(20/c)-texp(-(20/c)/t) -5.33x10-10Fraction
    (K2) exp(-20/ct) 27.7
  • For K1 fraction formula is the same but with
    different t, Fraction(K1) exp(-749)
    10(-749/ln(10))10-325.29 1.9x10-325The ratio
    is 1.9x10-325 / 27.7 6.9 x 10-325.
  • Fraction of decays between 20 and 21 meters is
    exp(-20/ct)-exp(-21/ct) 0.27746 0.2602
    0.017 1.7 The number of K2s to produce is
    therefore 22700 / 1.7 / 1 133 million

76
Solution to exercises
  • Exercise 4
  • Feynman diagram for p- decay (u d)

p-
d
u
Vud
W-
nm
m-
77
Solution to exercises
  • Exercise 4
  • Feynman diagram for L0 ? pnee decay (L0 uds)

L0
u
d
s
W-
Vus
e-
ne (RH)
u
d
u
p
78
Solution to exercises
  • Exercise 4
  • Two Feynman diagrams for K0 K0 mixing. You can
    make additional ones by replacing one or both of
    the c quarks with u or t quarks

Vcs
d
Vcd
s
c
c
K0
K0
s
d
Vcd
Vcs
Vcs
d
c
Vcd
s
K0
K0
s
d
c
Vcs
Vcd
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