Electroweak physics (II)
(The SM: structure and phenomenology) Andrea Romanino
SISSA/ISAS
Plan (II)
• Structure of the Standard Model
• The Higgs sector
• The gauge sector
• The flavour sector
• Tests
• The neutrino sector
• Beyond the Standard Model
The Standard Model (SM) of particle physics
(in compact notation) i=1,2,3: family index
masses neutrino
Λ
) )(
(
flavour Ψ
Ψ
breaking symmetry
) (
|
|
gauge 4
Ψ 1 Ψ ˆ
2
H L H η L
H H V H
D
F F D
i
L
j ij i
i j ij µ
µν a µνa i
i
SM
+ λ
− +
−
=
The SM as a renormalizable theory
A precise definition requires specifying:
• The fermion content: Ψ
• The gauge group G and its action on Ψ
• The symmetry breaking (scalar) sector: H
• The globally symmetric lagrangian L ( Ψ , H )
( ) ( ) ψ ψ ψ ( ) ψ ( ) ψ ψ ψ
ψ ψ
ψ , , , ,
½,0) (
0,½) (
+
→ +
→
+
The fermion content
spinors Dirac
) , , , , , , , ,
, , , (
Ψ = e µ τ ν
eν
µν
τd s b u c t
) , , ,
, ,
, ,
,
:
(notation ei ↔ e µ τ νi ↔νe νµ ντ ui ↔ u c t di ↔ d s b
A 4-component Dirac spinor ψ has two 2-
components with definite chirality ( ): γ
5ψ
L Rψ 2
1
,
∓ γ
5=
A gauge symmetry can mix fields with same Lorentz quantum numbers ⇒ can act independently on ,
(chiral symmetry)
Lψ ψ
RSO(3,1)=SU(2)xSU(2) →
(or)
=
=
∗, 0
0
cR
L
ψ ε
ψ ψ ψ
( ) ( )
L R R↔
c ∗ c∗L
ψ ψ ψ
ψ , ψ ψ , ψ ψ
½,0) 0,½) (
(
GeV 300
~ Λ Λ ,
1
2 / )
1 ( 2
/ ) 1
( 2
2 weak
=
+
=
− +
−
=
=
F
µ L L µ L
µ L µ
cµ
†µ µ c
F c
G
d u
e ν
d u
e ν
j
j G j
L
γ γ
γ γ
γ
γ
5 5The gauge group G
Works well at E « Λ
However, it must fail at E » Λ:
) (unitarity /
1
~ vs
~ G
2E
2σ E
2σ
(1 family only)
M E E
g
~ E σ
A~ g
M M E
g E
~ M σ
A~ g
» 1 @
«
@
2 4
2 2
4 4 2
2 2
νe νe
e e
At E > Λ it should be possible to account for the 4-fermion operator in terms of renormalizable operators
νe νe
e e
νe νe
e e
2 h.c.
weakren
= g j
cµW
µ++ L
symmetry gauge
of SSB vector
massive ⇒
µ+
W
2 2
2 8
WF
M G = g
ψ W
T ψ
W
j
cµ µ+→ γ
µ a µa) prediction (NC
2
, ]
,
[ 1 2 3 3 σ3
T iT
T
T = =
• , are mixed by the generators → define
• Denote also
• then
• : G ⊇ SU(2),
• Q (charge/e) must also be a generator; Q = diag(0,1) on L (independent of T’s)
• Define ; is also a generator and commutes with the T’s:
From the lepton charged current to G
=
L L
e L ν
νL eL
2
2
1 µ
µ µ
iW W ± =W ∓
L W
T W
T L
g
Lweakren = γµ ( 1 µ1 + 2 µ2)
, 2 2
2 2
1 1 σ
σ T
T = =
singlet
~
doublet
~ eR
L
T3
Q Y = −
Action of G on the quarks
• L doublet, singlets of SU(2)
• On Q: ok
•
• triplets of SU(3)
=
L L
d
Q u uR ,dR
=
− −
= −
−
= 0 1
0 1
6 1 2
/ 1 0
0 2
/ 1 3
/ 1 0
0 3
/ 2 T3
Q Y
; 3 on
; 1 3 on
2 uR Y dR
Y = = −
L R
L
R u d d u , , ,
Left-handed fermions quantum numbers (summary)
3 / 2 1
3
3 / 1 1
3
6 / 1 2
3
1 1
1
2 / 1 2
1
U(1) SU(2)
SU(3)
−
−
R i R i i R i
i
u d
Q e
L
U(1) x
SU(2) x
SU(3)
G =
0 )
3 3
6 2
( 3 anomaly
Grav.
0 )
3 3
6 2
( 6 U(1)
0 )
Tr(
SU(2)) SU(2)x(not
) 3
( 2 / 3
xU(1) SU(2)
0 )
Tr(
xSU(3) SU(2)
2 ,
) 2 ( SU
0 )
Tr(
SU(3)) SU(3)x(not
0 )
2 ( 2 / 3
xU(1) SU(3)
0 )
Tr(
xSU(2) SU(3)
vectorlike )
3 ( SU
) ) (
) ( (
3) 3 (
) 3 (
) 3 (
3
3 2 a
2 C
2 a b
3 2 a
) ) (
2 a (
2 3
= +
+ +
+
= +
+ +
+
=
+
=
=
=
= +
+
=
R R R
R R R
R R
d e Q u
L
d e Q u
L
Q ab L
ab
u d Q
AB
Y Y
Y Y
Y
Y Y
Y Y
Y σ
Y Y
δ λ
δ }
σ σ
{
λ
Y Y
Y δ
σ
1
Anomaly cancellation
Y T
t τ
} τ τ { τ Tr
T
ijk ≡ ( i j , k ) =? 0, i = A, a ,(nice, but why?)
• G must be broken, or else
– All vector bosons would be massless – All fermions would be massless:
• A G-symmetric mass term combines left-handed fermions with conjugated quantum numbers under G:
• The representation of G on the SM fermions is chiral (= no such term is allowed)
• Note: the electroweak symmetry protects the fermion protects masses
(is that the reason why the SM fermions are chiral?)( )
h.c.) () h.c.
( + = +
=
m ψ
Rψ
Lm ψ
Lψ
Lψ
ψ m
Spontaneous symmetry breaking
Fermion masses and Higgs quantum numbers
• Electron mass term:
• = a doublet with Y=½ under SU(2)xU(1)
• The only possible renormalizable gauge invariant coupling of is (Yukawa interaction), where H is a scalar doublet with Y=½ under SU(2)xU(1) (Higgs doublet)
• One Higgs doublet is sufficient to embed all mass terms in gauge-invariant interactions
• The most general gauge invariant Yukawa lagrangian is then , where SU(2) and
SU(3) contractions have been understood ( ) )
h.c.
(
e
Re
L +m
L e e
e
R L ⊆ RR
LH
†e
λL e
RLi Ri Li
Ri Li
Ri
e d d u u
e
, ,H Q u
H Q d
H L
e
Ri j † Dij Ri j † Uij Ri jEij λ λ
λ + +
pq q p
ε H Q
QH
=The Higgs sector
Most general gauge invariant ren. lagrangian for H :
2
2 ( )
) 2 (
) (
) (
H H
H H
µ H
H V
H H
V H
D H
D L
H †
†
†
† µ
µ † H
+ λ
=
−
=
breaking symmetry
k Electrowea 0
2 < 0 ⇒
H
≠ ⇒µ
)
~ scale a
at but breaking,
symmetry k
Electrowea 0
0
(
µ
2 > ⇒H
≠ ⇒m
π> 0 λH
breaking symmetry
) (
|
|
flavour Ψ
Ψ
gauge 4
Ψ 1 Ψ ˆ
2
V H H
D
H F F
D i L
µ
j i ij
µν a µνa
i i
SM
− +
+
−
= λ
The renormalizable part of the SM
is now fully specified
The Higgs sector (II)
• Unbroken generators
• 3 broken generators ↔ 3 massive vectors ↔ 3
unphysical Goldstone bosons ↔ 1 real physical Higgs
2 2
2 | | (174GeV) ,
0 0 ,
=
=
>
=
H
v µ v v
H
λQ b T
a
ib v b
H
T
⇒ ∝
−
= −
=
3 2 1
0 2
, 2 real, 2
,
, = = 1
+
=
σ Y
T b
a T
b aY
T
a a a a aGoldstone bosons and Higgs
• To identify the Goldstone bosons:
– Write down the 4x4 Higgs mass matrix and find the massless eigenstates or
– Perform infinitesimal SU(2) x U(1) rotations of the vacuum
– CP: ; H has CP = +1, has CP = -1
⇒
−
= +
=
3 2 1
2
iG
G v iG
ε H
T G ε i H
δ
a a
+ +
=
+
2
iG
0v h H G
0 3 2
1 ,
2
G G G
G
+ =iG
+ = −G
0H
†H
→Higgs mass and self-coupling
• Higgs potential in unitary gauge:
• The Higgs self-coupling is proportional to its mass (non decoupling effects)
2 2
2
2 | µ | 2 v
m
h= = λ
Hconst.
8 2
) 2 (
)
(
2 3 42
0
= + + +
=
=m h v h h
H V
h
V
G hλ
Hλ
HTheoretical constraints on the Higgs mass
• Assume that the SM holds up to the scale Λ:
finite (perturbative) ⇒ upper limit on
> 0 ⇒ lower limit on
(if < 0, the absolute
minimum of the effective potential resides at or above Λ)
) Λ
H ( λ
) Λ
H ( λ
) Λ
H ( λ
m
hm
h) Λ
H ( λ
[Gino’s courtesy]
h V(h)
Λ 2 2 4
8 ) ( 2
) ) (
( h h
h h h µ
V ≈ + λH
• The lower limit can be relaxed if we live in a metastable vacuum
[Hambye, Riesselmann]
Experimental constraints on the Higgs mass
• Direct experimental limit:
> 114 GeV
• Indirect upper limit from EW precision tests (see below):
< 280 GeV @ 95% CL
(assumes no new physics contributions to the EW precision tests)
m
hm
h[LEP EW WG]
W, Z, and γ
• The vector boson masses arise from
•
• depend on the multiplet on which they act
• can be different because the corresponding generators cannot be linked by a gauge transformation
Y B ig T
igW t
G ig
Dµ = ∂µ + s µA A + µa a + ' µ
' , , g g gs
Y T
t A, a ,
H D
H
D
µ )† µ (' 2
2 )
(
2 3 2 2
2 1
+
=
− ′
−
=
+
µ µ µ
µ
µ µ
µ
Z g
g iv gW
B g gW
iW W
iv g H
D
µ µ
µ µ
µ Wµ iW Z c W s B
W − ≡ −
+ ≡ 1 2 3
,
2
2 '
/
cosθ g g g
cW ≡ W = +
• Therefore,
• A is indeed the photon field
• Z couples to the neutral current (vector and axial couplings)
•
– Not guaranteed by gauge invariance nor by the breaking pattern – Peculiar of EW breaking by a doublet (triplets ruled out)
where 2 ,
) (
2 2 µ
Z µ µ µ
µ W
µ † M Z Z
W W
M H
D H
D = + − +
2 1 iT T
T ± = ±
2
2 '
' '
g g
c gg g gs
e W W
= +
=
=
W µ µ W
µ µ
µ
µ T s Q Z
c i g ieQA
T g W
i T
g W i
D ( )
2 2
2 3 − +
+ +
+
∂
= + + − − +igsGµAt A
level) (tree
cos2 1
2
2 =
≡
W Z
W
θ M
ρ M
W µ W µ
µ s W c B
A = 3 +
2 2 2 2
2 2 2
2 , '
2 g g v
M g v
MW = Z = +
2 = 0 MA
Also,
4 2
1
2 v
GF
=
(Custodial symmetry)
• In general, ρ = 1 can be traced back to a symmetry of the Higgs potential (custodial symmetry)
• ⇒ V(H) is symmetric under O(4) ~ , broken to the diagonal (custodial) SU(2)
• The whole lagrangian is symmetric for vanishing g’ and L-R
symmetric Yukawas. In particular, the W-H couplings are invariant under SU(2) ~ O(3), hence ρ = 1
• ρ = 1 can be reproduced if the symmetry breaking mechanism has a custodial SU(2) symmetry under which both the W’s and the G’s
22 22
12 12
|2
|H = h r +h i +h r +h r xSU(2)R
SU(2)L
2 / ) Φ Φ ( ,
Φ Φ
, Φ
2 1 2
1 † † †
L UR H H Tr h U
h h
ε h → =
=
∗
Gauge interactions
• Fermion gauge interactions:
• Gauge boson self-interactions: from
in terms of mass eigenstates:
µA A sµ s µ µ
em µ µ
W n µ µ
c
j Z ej A g j G
c W g
g j Ψ
i Ψ Ψ
D i
Ψ
− − −
+
−
∂
= + h.c.
ˆ 2 ˆ
W χ µ
R L
χ e u d ν
f χ
nµ µ iL
iL µ iL
µ iL
c
ν e u d j f T s Q f
j
i i i i
) (
, 3 2
, , , ,
−
= +
=
∑
= = γ
γ γ
µ ν ν
µ µν
νc µb a abc
µ a ν
ν a µ
µν
B B
B
W W
ε g W
W W
∂
−
∂
=
−
∂
−
∂
=
µ+
W
ν−
W
Z , γ
µ+
W
ν−
W
µ µ µ
µ Z Z
W +, , ,γ
ν ν ν ν Z
W −, ,γ , γ a
µν µνa
W
4W
− 1
W +
W −
e+
e−
γ
W −
e+
W +
W −
e+
e−
νe
(a)
e− (b)
(a) (a+b)
(a+b+c)
• Higgs gauge interactions
gauge unitarity
2 1
2 2 22 2 2
+
+
M
WW
µ+W
µ −M
ZZ
µZ
µv
h v
h
The flavour sector
•
• The Higgs coupling to fermions is proportional to their masses
– The coupling to light (« 174 GeV) fermions is small
– The coupling to the top leads to non-decoupling effects – The Higgs is mainly produced by gauge interactions
• Despite the rich flavour structure:
– No flavour or CP violation with leptons (neglecting neutrino masses)
v m
ijE ,D,U = λEij,D,UH Q u
H Q d
H L e
L
f = λEij Ri j † + λDij Ri j † + λUij Ri j−
2 h.c.
2
2 + + +
+
+ +
=
h u
v u h m
d v d
h m e
v e m
u u m
d d m
e e m
Lj Ri ijU
Lj Ri
ijD Lj
Ri ijE
Lj U Ri
Lj ij D Ri
Lj ij E Ri
ij
unitarity gauge
The lepton flavour sector (neglecting ν masses)
• Mass eigestates:
Then
• Extend to gauge multiplets (commutes with G):
• Then
No LFV nor CPV,
R E EL
† diag
E
U
Em U
m
= , unitary, = diag( i ) ≥ 0L
R E e
E diag
E
U m m
U
i e i
Li e Ri
Lj E Ri
ij
e e m e e m e e
m
+ h.c. = i ′ ′ + h.c. = i ′ ′
′ =
′ =
Lj E ij
Li
ij Rj Ri E
e U
e
e U
e
L R ) (
) (
Ri i Ri
Ri i i Ri
i
i D L e i D e L i D L e i D e L
ˆ + ˆ = ′ ˆ ′ + ′ ˆ ′
′ =
′ =
j E ij
i
Rj E ij
Ri
L U
L
e U
e
L R ) (
) (
i † e Ri
j † E Ri
ij
e L H
= λ ie
′L
′H
λ10 11
2 . 1 )
(
µ
→e γ
< × −BR
,
• Mass eigestates:
Then
• Cannot extend both to gauge multiplets
H Q d V H
Q u
H Q d H
Q d
Q U
Q
d U
d
u U
u
i j u ij
Ri j Uij
i † d i
j † D Ri
ij ij j
i D
Rj ij
D Ri
Rj ij
U Ri
i i
L R R
′
= ′
′
= ′
→
′ =
′ =
′ =
λ λ
λ
λ but
) (
) (
) (
e.g.
′ =
′ =
′ =
′ =
ij Lj U
Li
ij Rj U
Ri ij Lj
D Li
Rj D ij
Ri
u U
u
u U
u d
U d
d U
d
L R L
R ( )
) , (
) (
)
( d i i d i i
Li d Ri
Li d Ri
Lj U Ri
ij Lj
D Ri ij
u u m d
d m
u u m d
d m u
u m
d d
m
i i
i i
′ + ′
′
= ′
′ + + ′
′
= ′ +
+ h.c. h.c.
R L
R L U U
† diag U U
D D
† diag
D
U
Dm U m U m U
m
= , =The quark flavour sector
) ,
(both
u
Ljd
Lj ∈Q
• In terms of mass eigenstates:
• All flavour and CP violation effects originate from the quark charged current → calculable FCNC and CPV processes
(CP: g → g* in an arbitrary phase convention for the mass
eigenstate fields ⇒ CP is conserved iff all the couplings are real for at least one phase choice)
µ jL ij iL
µ iL µ iL
had
c u d V u d
j , = γ = ′ γ ′ )
( ,
, = nµhad ′
µhad
n
j
j
) ( ,
, = emµ had ′
µ had
em
j
j
Parameters: summary (no ν masses)
) CC (
18 : Tot 3
(l) sector Flavour
10 ,
, ,
(q) sector
Flavour
2 ,
sector Higgs
3 sector
Gauge
3 , 2 , 1
+ +
QCDe u d
h s
θ
m
δ θ
m m
m v
g,g',g
i i i
Tests of the electroweak sector
• The electroweak sector (fermions + gauge interactions + masses from the Higgs sector) is the best tested
part of the SM
– Wide range of predictions:
g, g’, v ↔ ↔ QED, W&Z masses, their
self-interactions and all fermion gauge interactions (tree level)
– Measurements at the ‰ level
• Excellent agreement with the experiment (even too good)
v s
W, ),
(α
Low energy tests
• β, lepton and pion decays (CC): GF, universality
• Atomic parity violation:
• Parity violation in Møller scattering
• (Parity violation in ep scattering)
• Neutrino-nucleous DIS:
θ
Wsin
2θ
Wsin
2θ
Wsin
2θ
Wsin
2(NC)
An example: Atomic Parity Violation
e e
Z
(Z,A) (Z,A)
A Z
s Q
r δ σ
m Q
H G
W W We
PV = F ⋅∇ ( ), = (2 − 4 ) −
∆ 2 2
55133
Ce in crossing -
level p
- s
) 3 ( 19 . 73
|
| ), 48 ( 69 . 72
|
|
Q
W exp=Q
W th=[E158]
(The 3σ NuTeV anomaly has probably more to do with QCD (parton distributions) than
High energy tests
• At LEP II, LEP I, SLC, Tevatron
• M
Z,Γ
ZZ resonance in e
+e
-→ff
N
v=2.9841±0.0083: 3 light neutrinos + anomaly cancellation = 3 families
• M
W,Γ
We
+e
-→W
+W
-at LEP II
•
•
•
• A
FB...
l
σ
h,gc
We WWZ
WW γ , couplings ∝ ,
) (
Γ )
( Γ
) (
Γ )
( Γ
L R R
L
L R R
f L
LR
Z f f Z f f
f f Z
f f A Z
→ +
→
→
−
= →
• Accuracy in most cases is at the ‰ level → sensitivity to 1-loop
corrections, which involve
– g, g’, v
– mt, αs(MZ), ∆αhad(MZ) – mh
and bring together
– the gauge sector:
– the flavour sector:
– the EW-breaking sector:
) 4
2 /( π λt
) 4 /(
), 4
/( 2
2 π g π
g ′
) /
log(
) 4
2 /(
h MW
m π
g
Bounds on NP
⋅
>
⇒
<
=
+ +
=
<
∑
1
~ loop, one
ve, perturbati is
NP if TeV 0.5
1
~ level, tree
ve, perturbati is
NP if TeV 5
g interactin strongly
is NP if TeV 50
~ TeV 5
Λ
TeV) 5
(
1 : Λ
EWPT
16
) Λ Λ
(
2 2
2 2 2
2
λ λ c
c π λ λ
c
c O L
E L
i SM
SM i
n i
i i
SM SM i
eff SM …
Accidental symmetries
• Global symmetries of :
– Must commute with the gauge symmetry
– Must be U(1) symmetry (non degenerate fermion spectrum)
• 5 (independent) global U(1) symmetries of :
• Symmetries of could be violated by (accidental symmetries)
GeV j
i L H L
L H
L
GeV L B
Q Q Q
k L j
i
B B k l j i
15 15
10
~ Λ masses
neutrino )
( and
violates )
)(
(
10 4
Λ decay
proton violates
Λ
≠ ⇒
⋅
>
⇒ ) 2 / 1 1
2 / 1 3
/ 1 3
/ 2 6
/ 1 (
0 0
0 0
0 0
0 3
/ 1 3
/ 1 3
/ 1
−
−
−
−
− Y
δ δ
L B
H e
L u
d Q
ik ik
k
R i i i
i R i R
SMren
L
SMren
L
SMren
L L
SMeffSmallness of neutrino masses
Natural scale of fermion masses:
v = 174 GeV
Why
(must have a different origin than
? 10
/v < −12 mν
) 10 3 . 0
/v ≈ −5 me
GeV) 10
2 (
eV 05
. GeV 0
10 5
. 0
~ Λ
Λ
) )(
Λ (
GUT 16 15 SMren SMeff
⋅
≈
⋅
⋅
=
+ +
=
M
h m hv v
m
L H L
h H L
L
ν ν
…
1 familyThe SM as an effective theory
Majorana
In neutrino physics we are still (and we will remain…) at the level of the Fermi theory
c c
c c
e e
d d
ν ν
u u
Right-handed neutrinos
Y c xSU(2)LxU(1) SU(3)
c c
c c
e e
d d
ν ν
u u
Right-handed neutrinos
B-L R
c xSU(2)LxSU(2) xU(1) SU(3)
c c
c c
e e
d d
ν ν
u u
Right-handed neutrinos
SO(10)
c c
c c
e e
d d
ν ν
u u
Right-handed neutrinos
Y c xSU(2)LxU(1) SU(3)
heavy be
therefore can
and singlet
SM a
c
is v
v λ m
LH v
λ
c→
ν=
(as for the other fermions)(unlike the other fermions) c
c
v M v
L
HE⊃ − 2
T D ν D
T
M m m
m
M λ h λ
L H L
h H
1 1 Λ
) )(
Λ (
−
=
−
→
X
H
L
H
L νc νc
M
See-saw
: out
Integrate ν
cMajorana
Beyond the Standard Model
• Experimental “problems” of the SM:
– Gravity
– Dark matter
– Baryon asymmetry
• Experimental hints of physics beyond the SM
– Neutrino masses
– Quantum number unification
• Theoretical problems of the SM:
– Naturalness problem
– Cosmological constant problem – Strong CP problem
• Theoretical puzzles of the SM:
– Hierarchy
– Family replication
– Small Yukawa couplings, pattern of masses and mixings
– Gauge group, anomaly cancellation, charge quantization, quantum numbers
E
ΛSM
− MPl
−
SM NP
The SM is an effective theory valid below ΛSM
• Where is ?
• What type of physics above ? ΛSM
ΛSM
The naturalness problem as a guideline for NP
GeV H =174
−
2 2
2 2
2 2
2
2 (4 2 ) Λ
2 4 ) 3 Λ
( SM F t W Z h SM
h
h m M M m
π m G
m = + − − −
Where is ? Q
SMThe main upper limit follows from solving the hierarchy problem
=
+
=
+
=
GeV 250
if TeV
2 ) Λ
Λ (
GeV 115
TeV if 5
. 0 ) Λ
Λ (
2 2 2
2 2 2
SM h SM h
h
SM h SM h
h
m m
m
m m
m
• is the scale of the degrees of freedom cutting off the Higgs mass quadratic divergence
• barring accidental cancellations ΛSM
TeV ΛSM <~
Unification
3 / 2 1
3
3 / 1 1
3
6 / 1 2
3
1 1
1
2 / 1 2
1
U(1) SU(2)
SU(3)
−
−
R i R i i R i
i
u d
Q e
L
10 ,
,
5 ,
SU(5)
R i i i
R
R i i
u Q e
d L
16 ,
, , ,
,
SO(10)
R i R i
i i i R
R
i ν e Q u d
L
(SU(5))
heavy
5V τ = ig G t +igW T +ig'B Y + ig µα α s µA A µa a µ
s g g g MU
g ' @
3
5 = 5
=
=