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 (CKM) Matrix
• NEUTRAL WEAK INTERACTION - Elastic Neutrino-Electron Scattering - Electron-Positron Scattering Near the Z0 Pole
• ELECTROWEAK UNIFICATION - Chiral Fermion States - Weak Isospin and Hypercharge - Electro-Weak Mixing THE WEAK FORCE Characteristics of the WEAK FORCE
The time scale of the decay is long. Radioactive decays must proceed by the weak force since the timescale ranges from 10-8 s to years E.g. neutron β decay
Weak decays often involve neutrinos • do not interact by the EM force or the strong force • cannot detect in conventional detectors • can infer existence from conservation of E, p (Pauli, 1930)
Neutrinos would not be directly detected for 25 years: Reines & Cowan, using Savannah River nuclear reactor DECAY OF THE NEUTRON HELICITY Helicity is the component of the (spin) angular momentum along momentum vector. For fermions, the value is –1/2 or +1/2, depending on whether spin S is antiparallel or parallel to direction of motion p
Solutions of the Dirac equation:
where
are helicity eigenstates:
For antiparticles the relation is reversed (because v(p) ~ u(-p)): HELICITY
with
In the limit m=0 (E>>m):
obeys
Thus the following “chirality” projection operators are also helicity projection operators for m=0:
For m=0, PL projects onto helicity –1/2 fermions but helicity +1/2 anti-fermions. HELICITY and EM INTERACTION
We can use the projection operators to split the electromagnetic current into 2 pieces:
where
Since
we have
and HELICITY and EM INTERACTION Helicity is conserved in the electromagnetic interaction in high energy (m=0) limit
Allowed QED vertices in high energy limit
mirror reflection
Helicity is reversed under parity:
Equalities are due to parity CHARGED LEPTONIC WEAK INTERACTION
The mediators of weak interactions are “intermediate vector bosons”, which are extremely heavy:
The propagator for massive spin-1 particles is:
, where M is MW or MZ
In practice very often:
The propagator for W or Z in this case: WEAK INTERACTION
Lorentz condition ε µ p = 0 µ FEYNMAN RULES
also 3 and 4 boson vertices exist CHARGED LEPTONIC WEAK INTERACTION The theory of “charged” interactions is simpler than that for “neutral” ones. We start by considering coupling of W’s to leptons. The fundamental leptonic vertex is :
The Feynman rules are the same as for QED, except for the vertex factor :
( the weak vertex factor )
“Weak coupling constant” (analogous to ge in QED and gs in QCD) : CHARGED WEAK INTERACTION
The charged weak interaction violates parity maximally
By analogy to EM we associate the charged weak interactions with a current, which is purely left-handed:
also
The charged weak interaction only couples to left-handed leptons (e,µ,τ,νi). (Also, only couples to left-handed quarks.) It couples only to right-handed anti-fermions. Example: Inverse Muon Decay
( lowest order diagram )
When the amplitude is :
Simplifies because MW = 80 GeV much larger than q< (100 MeV). Example: Inverse Muon Decay Applying Casimir’s trick we find :
trace theorems trace theorems
using : Example: Inverse Muon Decay
In CM frame, and neglect the mass of the electron :
where E is the incident electron (or neutrino) energy. The differential scattering cross section is :
The total cross section : DECAY OF THE MUON
The amplitude :
As before : DECAY OF THE MUON In the muon rest frame :
Let :
Plug in : DECAY OF THE MUON
The decay rate given by Golden Rule* :
where :
* a lot of work, since this is a three body decay DECAY OF THE MUON
Perform integral :
where :
Next we will do the integral. Setting the polar axis along (which is fixed, for the purposes of the integration), we have : DECAY OF THE MUON
Also :
The integral is trivial. For the integration, let :
and : DECAY OF THE MUON
integration :
where :
The limits of E2 and E4 integrals : DECAY OF THE MUON
Using: DECAY OF THE MUON DECAY OF THE MUON DECAY OF THE MUON DECAY OF THE MUON
The total decay rate :
Lifetime : DECAY OF THE MUON
gW and MW do not appear separately, only in the ratio.
Let’s introduce “Fermi coupling constant” :
The muon lifetime : = 2.2×10-6 s DECAY OF THE MUON In Fermi’s original theory of the beta decay there was no W; the interaction was a direct four-particle coupling.
Using the observed muon lifetime and mass :
and :
“Weak fine structure constant” :
Larger than electromagnetic fine structure constant! WEAK INTERACTIONS
Weak force is weak because boson propagator is massive, not because coupling strength is weak. DECAY OF THE NEUTRON
( the same as in previous case ) DECAY OF THE NEUTRON In the rest frame of the neutron :
We can’t ignore the mass of the electron. As before :
where : DECAY OF THE NEUTRON The integral yields :
and :
Setting the z-axis along (which is fixed, for the purposes of the integral), we have :
and : DECAY OF THE NEUTRON
where :
and : DECAY OF THE NEUTRON
The range of E2 integral :
E is the electron energy
( exact equation) DECAY OF THE NEUTRON
Approximations :
Expanding to lowest order : DECAY OF THE NEUTRON DECAY OF THE NEUTRON
(picture from Griffiths) DECAY OF THE NEUTRON
where : Putting in the numbers : DECAY OF THE NEUTRON
But the proton and neutron are not point particles.
Replacement in the vertex factor:
cV is the correction to the vector “weak charge” cA is the correction to the axial vector “weak charge” DECAY OF THE NEUTRON
Another correction, the quark vertex carries a factor of is the Cabibbo angle.
cosθC = 0.97 Lifetime : CHOICE OF WEAK EIGENSTATES 4-Fermion INTERACTION
DECAY OF THE PION
The decay of the pion is really a scattering event in which the incident quarks happen to be bound together.
We do not know how the W couples to the pion. Use the “form factor”.
“form factor” DECAY OF THE PION DECAY OF THE PION DECAY OF THE PION DECAY OF THE PION
The decay rate :
The following ratio could be computed without knowing the decay constant :
Experimental value : DECAY OF THE PION CHARGED WEAK INTERACTIONS OF QUARKS For leptons, the coupling to W+ and W- takes place strictly within a particular generation :
For example :
There is no cross-generational coupling as :
There are 3 generations of quarks :
Coupling within a generation :
There exist cross-generational coupling as : CHARGED WEAK INTERACTIONS OF QUARKS
(Cabibbo, 1963) (extra cos or sin in the vertex factor) Example : Leptonic Decays
l is an electron or muon.
The quark vertex :
Using a previous result :
The branching ratio :
Corresponding to a Cabibbo angle : Example : Semileptonic Decays
(semileptonic decay)
(non-leptonic weak decay) Example: Semileptonic Decays Neutron decay : Quark process : There are two d quarks in n, and either one could couple to the W. The net amplitude for the process is the sum. Using the quark wave functions
The overall coefficient is simply cos, as claimed before.
In the decay: the quark process is But : the same
we get an extra factor Example : Semileptonic Decays
The decay rate : GIM MECHANISM Cabibbo-GIM Mechanism The decay is allowed by Cabibbo theory.
Amplitude : , far greater.
GIM introduced the fourth quark c (1970). The couplings with s and d :
GIM = GLASHOW, ILIOPOULOS, MAIANI Cabibbo-GIM mechanism
Now the diagrams cancel. Cabibbo-GIM mechanism The Cabibbo-GIM mechanism : Instead of the physical quarks d and s, the “correct” states to use in the weak interactions are d’ and s’ :
In matrix form :
The W’s couple to the “Cabibbo-rotated” states : Cabibbo-Kobayashi-Maskawa (CKM) Matrix
CKM is a generalization of Cabibbo-GIM for three generations of quarks.
The weak interaction quark generations are related to the physical quarks states by Kobayashi-Maskawa (KM) matrix
For example :
Canonical form of KM matrix depend only on three generalized Cabibbo angles and one phase factor. Kobayashi-Maskawa (KM) matrix
The full matrix :
Using the experimental values : THE CKM MATRIX NEUTRAL WEAK INTERACTIONS
Neutral weak interaction mediated by the Z0 boson
f stands for any lepton or quark
Not allowed : NEUTRAL WEAK INTERACTIONS It doesn’t matter if we use physical states or Cabibbo rotated states. NEUTRAL WEAK INTERACTIONS
First process mediated by Z0
(Bubble chamber photograph at CERN, 1973) NEUTRAL WEAK INTERACTIONS In the same series of experiments : Neutrino-quark process in the form of inclusive scattering
The cross sections were three times smaller than the correspondent charged events :
Indication of a new kind of interaction, and not simply a high order process. (which correspond to a far smaller cross section) NEUTRAL WEAK INTERACTIONS
The coupling to Z0 :
where :
(“Weak mixing angle” or “Weinberg angle”) NEUTRAL WEAK INTERACTIONS Neutral vector and axial vector coupling in GWS model : NEUTRAL WEAK INTERACTIONS
( Z0 propagator )
When :
the propagator is simply :
The masses of the bosons are related by the formula : Example : Elastic Neutrino-Electron Scattering Example : Elastic Neutrino-Electron Scattering
Now compute in CM frame and let : (mass of the electron) Example : Elastic Neutrino-Electron Scattering
( E is the electron or neutrino energy )
Using : Example : Elastic Neutrino-Electron Scattering
The total cross section :
Compare to :
(computed in the earlier)
(0.08 , experimental) Example : Elastic Neutrino-Electron Scattering
Most neutral processes are “masked” by electromagnetic ones. 0 Example : Electron-Positron Scattering Near the Z Pole
f is any quark or lepton (except electron – we must include one more diagram)
We are interested in the regime :
The amplitude :
where : 0 Example : Electron-Positron Scattering Near the Z Pole
( since we are working in the vicinity of 90 GeV ) Ignore the mass of quark or lepton
Finally : 0 Example : Electron-Positron Scattering Near the Z Pole
problems at Z0 pole 0 Example : Electron-Positron Scattering Near the Z Pole Z0 is not a stable particle. Its lifetime has the effect of “smearing out” the mass. Replacement in the propagator :
= decay rate
The cross section :
Because : the above correction is negligible outside Z0 pole. 0 Example : Electron-Positron Scattering Near the Z Pole Cross section for the same process, mediated by a photon :
( Qf is the charge of f in units of e )
The ratio : 0 Example : Electron-Positron Scattering Near the Z Pole 0 Example : Electron-Positron Scattering Near the Z Pole
Well below the Z0 pole :
Right on the Z0 pole : 0 Example : Electron-Positron Scattering Near the Z Pole CHIRAL FERMION STATES
To unify the weak and electromagnetic interaction, let’s move the matrix into the particle spinor.
( L stands for “left-handed” )
(But uL is not, in general, a helicity eigenstate) CHIRAL FERMION STATES
If the particle is massless :
helicity
where :
“projection operator”
Using : we can compute the following table è CHIRAL FERMION STATES CHIRAL FERMION STATES
(inverse beta decay)
The contribution to the amplitude from this vertex :
Negatively charged weak current and e stand for the particle spinors.
Rewrite as : (coupling between left-handed particles only)
Note that :
Electromagnetic current : WEAK ISOSPIN AND HYPERCHARGE
Negatively charged weak current
Positively charged weak current WEAK ISOSPIN AND HYPERCHARGE
We can express both by introducing the left handed doublet :
and the matrices : WEAK ISOSPIN AND HYPERCHARGE
We could have a full “weak isospin” symmetry if only there is a third weak current, “neutral weak current”.
Weak analog of hypercharge (Y) in the Gell-Mann – Nishijima formula :
Weak hypercharge : WEAK ISOSPIN AND HYPERCHARGE Everything could be extended to the other leptons and quarks :
Weak isospin currents :
Weak hypercharge current :
where : ELECTRO-WEAK MIXING GWS model asserts that the three weak isospin currents couple to a weak Isotriplet of intermediate vector bosons, whereas the weak hypercharge current couples to an isosinglet intermediate vector boson.
wave functions representing the particles.