Weak Interactions of
Leptons and Quarks
Enrico Fermi
GSW Electroweak theory (1968)
Sheldon Glashow Abdus Salam Steve Weinberg
ν
−
−
W
or
ν
W+
Leptonic Electroweak Theory
+
( )
1 52
2 γ γ
µ −
−
= igW
ν
µ
MW = 80.398 ± 0.0259 GeV MZ = 91.1876 ± 0.0021 GeV
ΓW = 2.141± 0.041 GeV
ΓZ = 2.9452 ± 0.0023 GeV
=
−
i g
µν−
q
µq
νM
W2⎛
⎝⎜
⎞
⎠⎟
q
2−
M
W2+
iM
WΓ
WThe vertex rule for leptons
ν − − W
( )
1 52
2 γ γ
µ −
−
= igW
Features of the Leptonic Weak Interactions
• Changes a lepton into its
neutrino partner and vice-versa
• W-polarization perpendicular
to its momentum
• Purely left-handed αW = gW
2
4πc
does not appear in GSW theory
−
i gµν − qµqν MW2 ⎛
⎝⎜
⎞ ⎠⎟ q2 − MW2 + iMWΓW
ig
µνM
W2q2 MW2
Low-energy W-propagator W-propagator
(internal line)
γ5 =iγ0γ1γ2γ 3= 0 I
I 0
⎛ ⎝⎜
⎞ ⎠⎟
1−γ5 = I −I
−I I
⎛ ⎝⎜
e ν − e − W − µ µ ν 1 p 2
p p'2 p'1
Muon Decay
−iM= ( )−i 2 gW
2 2 ⎛
⎝⎜ ⎞⎠⎟
2
u(p1′)γ µ
( )
1−γ 5 u(p1) ⎡⎣ ⎤⎦
gµν − qµqν /MW2 q2 − MW2
⎡ ⎣ ⎢ ⎢ ⎤ ⎦ ⎥
⎥ u(p2)γ
ν
( )
1−γ 5v(p2′ ) ⎡
⎣ ⎤⎦
propagator left-handed e−νe current
left-handed µ−νµ current
2gW
4MW
⎛ ⎝⎜
⎞ ⎠⎟
2
u(p1′)γ µ
( )
1−γ 5 u(p1)⎡
⎣ ⎦⎤⎡⎣u(p2)γ µ
( )
1−γ 5 v(p2′ )⎤⎦µ
−→
e
−+
ν
e+
ν
µu(p1′)γµ
( )
1−γ5 u(p1)⎡
⎣ ⎤⎦
†
spins∑
u(p1′)γν
( )
1−γ 5 u(p1)⎡
⎣ ⎤⎦
= Tr γ µ
( )
1−γ5 ( p1+m)γν( )
1−γ5 p1′+mν µ(
)
⎡
⎣⎢ ⎦⎥⎤=Tr⎡⎣γ µ
( )
1−γ 5 ( p1+m)γν( )
1−γ 5( )
p1′ ⎤⎦ (neglect mνµ)= Tr⎣⎡γ µ
( )
1−γ5 ( p1+m)( )
1+γ 5 γν( )
p1′ ⎤⎦=Tr⎡γ µ( )
1−γ5 2( )p1 γν( )
p1′ ⎣⎢⎤
⎦⎥ (trace of the mass term = 0)
=2Tr⎣⎡γµ
( )
1−γ5 ( )p1 γν( )
p1′ ⎤⎦=2Tr⎡⎣γ µ( )p1 γν( )
p1′ ⎤⎦ −2Tr⎡⎣γ µγ5( )p1 γν( )
p1′ ⎤⎦=8⎡p1′µp1ν + p1µp1′ν −gµν
( )
p1⋅p1′ +iεµανβp1αp1′β⎣ ⎤⎦ e ν − e − W − µ µ ν 1 p 2
p p'2 p'1 Casimir Trick: −iM 2gW
4MW
⎛ ⎝⎜
⎞ ⎠⎟
2
u(p1′)γµ( )1−γ5 u(p1)
⎡
⎣ ⎦⎤⎡⎣u(p2)γµ( )1−γ5 v(p′2)⎤⎦
The other term is similar, so:
M2 = 64
2
gW
2 2MW
⎛ ⎝⎜
⎞ ⎠⎟
4
p1′µp1ν + p1µp1′ν −gµν
( )
p1⋅p1′ +iεµανβ(
p1α p1′β)
⎡⎣ ⎤⎦
×⎣⎢⎡p2′µp2ν + p2µp′2ν − gµν
(
p2⋅ p2′)
+iεµρνσ(
p2′ρpσ2)
⎤⎦⎥= 1 2 gW MW ⎛ ⎝⎜ ⎞ ⎠⎟ 4
2
(
p1′ ⋅p2′)
(p1⋅ p2)+2(
p1⋅ p2′)
(
p1′ ⋅p2)
⎡⎣ +i2εµανβεµρνσ
(
p1α p1′βp′2ρp2σ)
⎤⎦⎥ = 1 2 gW MW ⎛ ⎝⎜ ⎞ ⎠⎟ 42
(
p1′ ⋅p2′)
(p1⋅ p2)+2(
p1⋅ p2′)
(
p1′ ⋅p2)
⎡⎣ − −
(
2(
δραδσβ −δρβδσα)
)
p1α p1′βp′2ρp2σ ⎤⎦⎥ = 2 gWMW ⎛ ⎝⎜ ⎞ ⎠⎟ 4
p1′ ⋅p2
(
)
(p1⋅ ′p2)e ν
−
e
− W
− µ
µ
ν
1
p
2
p p'2 p'1
Muon rest frame
neglect electron mass
Now we need to integrate over 3-body phase space
Neutrino masses are small, so set
′
p2
( )
2 = mνe
2 0 p′ 1
( )
2 = mνµ
e ν −
e
− W
− µ
µ ν
1
p
2
p p'2 p'1
lots of work to compute this 3-body integral
Total Decay Rate:
e ν
−
e
−
W
−
µ µ
ν
1
p
2
p p'2 p'1
Muon lifetime:
Fermi’s constant!
e
ν
−
e
−
W
−
µ
µ
ν
e
ν
−
e
−
µ
µ
ν
⎯
⎯
⎯ →
⎯
q2<<MW2Electroweak Theory
(renormalizable) (not renormalizable) Fermi’s Theory
The Strength of the Weak
Large compared to QED!
• Weak interactions are weak because the W is so heavy
Quark & Lepton Vertices
we never see this we always
see this
ν
−
−
W
or
ν
+
W +
So Leptonic charged weak vertex must be:
we always see this Conservation of Lepton Number
Left-handed SU(2) Doublets
Right-handed SU(2) Singlets E
−
W
E
Electron doublet
−
W
M
M Muon doublet
−
W
T
T
Tau doublet
Write
E
−
W
E
Electron doublet Compare to QCD
QCD
carries off colour charge carries off weak charge
u-quark in blue state emits a BR-gluon and changes into a u-quark in a red state
E-particle in electron state emits a W −
and changes into an E-particle in a neutrino state
suggests
WHY NOT?
Must allow cross-generational quark flavours to change into each other
d
−
e
e ν
d
u
u
d u
neutron proton
−
W
u
d
−
W c
s
−
W t
b
We observe that neutrons decay into protons (provided the
(
)
c Wig
θ γ
γ µ 1 sin
2 2 5 − − = u s − W
(
)
cW
ig
θ γ
γ µ 1 cos
2 2 5 − − = − W u d
1963: Cabbibo proposes quark-model weak vertices
Nicola Cabbibo
Kaon Decay Expts
We don’t know why this angle has the value that it does.
We regard it as another constant of nature, like the speed of light, or the mass of the electron. s − K p −
ν p'1
2 '
p
u
µ
ν
d
+
µ
s
−
µ
GIM Mechanism
ΔS =1 for both Why so different?
Problems with the Cabbibo theory:
Kaon decay rates were sometimes too small
an integral you compute from the diagrams
BR
(
K+ →π+ +νe +νe)
=(
1.7 ±1.1)
×10−10BR
(
K+ →π0 +νe + e+)
=(
5.07 ± 0.04)
×10−2Also:
K0
ΓCabbibo
(
K0 → µ+µ−)
ΓCabbibo
(
K0 → all)
I piµ;m
u2
(
)
×sinθccosθc>> Γ
expt
(
K0 → µ+µ−)
Γexpt
(
K0 → all)
= 7.3×10(
)
c Wig
θ γ
γ µ 1 cos
2 2 5 − − =
= + igW
2 2 γ
µ
1− γ 5
(
)
sinθcc s − W − W c d
1971: Glashow, Iliopolis, & Maini propose that maybe a new quark exists (call it c)
(
)
cW ig
θ γ
γ µ 1 sin
2 2 5 − − = u s − W
(
)
cW
ig
θ γ
γ µ 1 cos
2 2 5 − − = − W u d
u
µ
ν
d
+µ
s
−
µ
c
µν
d
+
µ
s
−
µ
+
u s − W − W u d
− igW
2 2 γ
µ
(
1− γ 5)
cosθc + igW
2 2 γ
µ
(
1− γ 5)
sinθc
c
s
−
W c W−
d
+
′
s = −d sinθc + scosθc
− igW
2 2 γ
µ
(
1− γ 5)
+
′
d = d cosθc + ssinθc
− igW
2 2 γ
µ
(
1− γ 5)
cosθc − igW
2 2 γ
µ
(
1− γ 5)
sinθc
− igW
2 2 γ
µ
(
1− γ 5)
The CKM Matrix
Left-handed SU(2) quark Doublets
weak eigenstates mass eigenstates
Cabbibo matrix
From the viewpoint of QED and QCD, d and s are the elementary particles From the viewpoint of Electroweak, d’ and s’ are the elementary particles
1973 : Kobayashi & Maskawa propose a 6-quark model
to explain
P
violation
Note: we also must have u,c, t quarks as the partners of
d, s,b
CKM matrix
(not obvious, but can prove using matrix algebra)
− W
S
S
−
W
B B
− W
D
− W
S
S
−
W
B B
− W
D
D
Regard each down-type quark and its up-type partner as 2 states of one particle!
Similar to what happens for leptons:
E
−
W
E
Electron doublet
−
W
M
M
Muon doublet
−
W
T
T
Tau doublet Down
doublet Strange doublet
Expt:
Jarlskog Invariant
These numbers are all
constants of nature. We do not have any explanation of their values at this point in history. This is one way to parametrize the CKM matrix
The Unitarity Triangle
Does α+β+γ =180o ? → Must check by experiment!
Electroweak Unification
+
=
Magnetism
Electricity Electromagnetism (QED)
Electromagnetism (QED)
Radioactivity (Weak)
=
Electroweak (QFD?)
W + W −
f
Z
f
Neutral Currents
Bludman (1958) electrically neutral
Fermion identity preserved
Problem: This interaction will be overwhelmed by electromagnetism!
How can we observe it? Answer: Gargamelle (1973)
The effects of the W’s are easy to find: they change both the charge and the type (or flavour) of particle
π− µ−
νµ νµ
iron slab
CF3Br freon Gargamelle
νµ
X
Hadron without a charged lepton
Results What
=
−
ig
Z2 2
γ
µ
c
Vf−
c
Afγ
5(
)
f
Z
f
Exp’t
ν
µ
=
−
i g
µν−
q
µq
νM
Z2⎛
⎝⎜
⎞
⎠⎟
q
2−
M
Z2+
iM
ZΓ
Z
−
i
g
µνM
Z2q2 MZ2
Z
Z-exchange
=
−
e
1 '
p
2
p
2
'
p
1
p
Z
−
e
1
' p
2
p
1
p
γ
+
2
'
p
f f
+
e e+
f f
f f
−
e e+
e
+e
-‐‑Neutral Current ScaOering
(neglecting fermion masses)
Casimir
Z
CMS − e 1 ' p 2 p 1 p γ 2 ' p f + e f − e 1 ' p 2 p 2 ' p 1 p Z f + e f Total Cross Section from Z exchange Total Cross Section from photon exchange
−
e 1
'
p
2 p
2 '
p
1 p
Z
f
+
e
f
−
e
1 '
p
2
p
1
p
γ
2
' p
f
+ e
f
2 2
Compare
E MZc2
E = MZc2
Photons dominate