H
Quarks
Quarks – – “ “ the building the building blocks of the Universe blocks of the Universe ” ”
The number of quarks increased with discoveries of new particles and have reached 6
For unknown reasons Nature created 3 copies (generations) of quarks and leptons Charm came as
surprise but
completed the
picture
Discovery History Discovery History
u d
t c
s b
six quarks 1947
1974 1995
1977
e µ
ν µ
τ ν τ ν e
six leptons 1956
1895
1963
1936 1975
Now we have a beautiful pattern of three pairs of quarks and three pairs of leptons. They are shown here with their year of discovery.
2000
Matter and Antimatter Matter and Antimatter
The first
generation is what we are made of
Antimatter was created together with matter
during the “Big bang”
Antiparticles are created at accelerators in ensemble with
particles but the visible Universe does not contain antimatter
Quark
Quark ’ ’ s s Colour Colour
( )
( )
( )
d d d s s s
u u u
!
! ++
" # # #
$ # # #
" # # #
Baryons are “made” of quarks
To avoid Pauli principle veto one can antisymmetrize the wave function introducing a new quantum number - “colour”, so that
( )
ijk
i j k
d d d
"
!
# = $ $ $
?
The Number of Colours The Number of Colours
The x-section of The x-section of electron-positron electron-positron
annihilation into annihilation into
hadrons is proportional hadrons is proportional to the number of quark to the number of quark
colours. The fit to colours. The fit to
experimental data at experimental data at
various colliders at various colliders at
different energies gives different energies gives
N
c= 3.06 ± 0.10
The Number of Generations The Number of Generations
Z-line shape Z-line shape
obtained at LEP obtained at LEP depends on the depends on the
number of number of
flavours and flavours and
gives the gives the
number of (light) number of (light)
neutrinos or neutrinos or
(generations) of (generations) of
the Standard the Standard
Model Model
N
g= 2.982 ± 0.013
Quantum Numbers of Matter Quantum Numbers of Matter
Quarks Quarks
Leptons Leptons
L
L
R R
R R
Q up
down U up
D down
! "
= # $
% &
=
=
SU(3)c SU(2)L UY(1)
3 3 3
2 1 1
1/ 3 4 / 3
2 / 3
!
?
L
L
R R
R R
L e
N
E e
!
!
" #
= $ %
& '
=
=
1 1 1
2 1 1
1 0 2
!
triplets doublets
singlets
3
/ 2
Q T = + Y
Electric charge
T
3T
3 121
- 2
0 0
V-A currents in
weak interactions
The group structure of the SM The group structure of the SM
Casimir Operators For SU(N)
QCD analysis
definitely singles out
the SU(3) group as
the symmetry group of
strong interactions
Electro-weak sector of the SM Electro-weak sector of the SM
SU(2) x U(1) versus O(3)
The heavy photon gives the
The heavy photon gives the neutral current without flavourneutral current without flavour
violationviolation
Discovery of neutral currents was a crucial test of the gauge gauge model of weak interactions at CERN in 1973
3 gauge bosons 1 gauge boson 3 gauge bosonsAfter spontaneous symmetry breaking one has 3 massive gauge bosons
(W+ , W- , Z0) and 1 massless (γ)
2 massive gauge bosons
(W+ , W- ) and 1 massless (γ)
Gauge Invariance Gauge Invariance
( )
ij( ) exp[
a( )
a]
i
x U x
ji x T
ij j! # ! = " !
a =1, 2,...,N( )
( ) ( ) ( ) ( ) ( ) ( )
( ) ( ) ( ) ( ) ( ) ( )
i x x i x U x U x x
i x x x U x U x x
µ µ
µ µ
µ µ
µ µ
! " ! ! " !
! " ! ! " !
+
+
# $ #
= # + #
Gauge transformation
parameter matrix Fermion Kinetic term
Covariant derivative
! "
µD
µ= !
µI gA T #
µa a= !
µI g A $ #
µ Gauge field( ) ( ) ( )
D
µ! x " U x D
µ! x ( ) ( ) ( ) ( )
1g( ) ( )
A x
µU x A x U x
µ µU x U x
+ +
! + "
matrix
U U
+= 1
Gauge invariant kinetic term
i ! ( ) x "
µD
µ! ( ) x
[ D D
µ,
!] = G
µ!= "
µA
!# "
!A
µ+ g A A [
µ,
!] G
µ!( ) x " U x G ( )
µ!( ) x U x
+( )
Gauge field kinetic term 1
4
Tr G G
µ! µ!"
Field strength tensor( )
ji( )
i
x
jU x
! " !
+Lagrangian of the SM Lagrangian of the SM
gauge Yukawa Higgs
L L = + L + L
1 1 1
4 4 4
( ) (
†)
a a i i
gauge
L G G W W B B
iL D L iQ D Q iE D E
iU D U iD D D D H D H
µ! µ! µ! µ! µ! µ!
µ µ µ
" µ " " µ " " µ "
µ µ
"
" µ " µ " µ µ
# # #
# #
= $ $ $
+ + +
+ + +
L D U
Yukawa
L = y L E H y Q D H y Q U H
!" ! "+
!" ! "+
!" ! "2 † † 2
2
( )
Higgs
L = " V m H H = "
!H H H = i H !
2 †(3) (2) (1)
c L Y
SU ! SU ! U
α,β=1,2,3 - generation index
Fermion
Fermion Masses in the SM Masses in the SM
L L R R
0
! ! = ! ! =
L R R L
! ! + ! !
c c
L L L L
! ! + ! !
Direct mass terms are forbidden due to SU(2)
Linvariance !
SU(2) doublet SU(2) singlet Dirac Spinors
5 5
0 0 2 *
1 1
, , , ,
2 2
c
L
!
R! C i
" " = # " " = + " " = " !
+" = ! " = ! "
left right Dirac conjugated Charge conjugated
Lorenz invariant Mass terms SUL(2)
c c
R R R R
! ! + ! !
SUL(2) & UY(1) UY(1)
Unless Q=0, Y=0
c
! !
R RMajorana mass term
( )
0 exp( )
2 v
2
H H i !# H
!=$"H S
% &
' (
) )
* = +++* =
' + (
' (
, -
r r
r r
Spontaneous Symmetry Breaking Spontaneous Symmetry Breaking
(3) (2) (1) (3) (1)
c L Y c EM
SU ! SU ! U " SU ! U
0
H H
H
!
+"
= # $
% &
2 † † 2
2
( )
V = " m H H +
!H H
Introduce a scalar field with quantum numbers: (1,2,1) With potential
Unstable maximum Stable minimum At the minimum
0
0 exp( )
2 v
v 2 2
H H
H S iP i S
H
!"
+
+
# $ # $
# $ % & % &
= % ' & ( = % % + + & & = % % + & &
' (
' (
r r
scalar
pseudoscalar v.e.v.
Gauge transformation Higgs boson
h
0 H ! " v
= # $
% &
3 - 3 -
1
4 + 3 + 3
gW ' 2gW gW ' 2gW 0
(0 v)
2gW -gW ' 2gW -gW ' v
g B g B
g B g B
µ µ µ µ µ µ
µ µ µ µ µ µ
! + " ! + " ! "
# $ # $
% # & + $ # ' & + $ ' # $ & '
The Higgs Mechanism The Higgs Mechanism
( )
e
i a ae
i a a 1ge
i a ae
i a aW
µ ! "W
µ ! " µ ! " ! "# #
$ + %
a a
! = # "
Q: What happens with missing d.o.f. (massless goldstone bosons P,H
+or ξ ) ? A: They become longitudinal
d.o.f.of the gauge bosons W
µi, i=1,2,3
Gauge transformation
Longitudinal components Higgs field kinetic term
2 ' 2
2 2
g g
D H
µ= !
µH " W H
µ" B H
µ2 2
1
2 3 2v v ( ' )
2 4
g W W
µ+ µ!gW
µg B
µ" + ! +
1 23 3
2
Z sin cos
cos sin
W W
W W
W W W
B W
B W
µ µ
µ
µ µ µ
µ µ µ
! !
" ! !
±
=
= # +
= +
m
2 1 2 2
2
2 1 2 2 2
2
v
( +g' )v
W Z
M g
M g
=
=
tan /
0
W
g g M
!" = #
=
The Higgs Boson and
The Higgs Boson and Fermion Fermion Masses
Masses
2 † † 2
2
( )
V = " m H H +
!H H
0
v 2
H h
! "
# $
= # # + $ $
% & v
4v
2 2v
3 42 2 8
V ! h ! h ! h
!
= " + + +
( )v, ( )v, ( )v
u u d d l l
i i i
M = Diag y
!"M = Diag y
!"M = Diag y
!"2 2 v
m
h= m = !
2 2
v = m / !
E D U
Yukawa
L = y L E H y Q D H y Q U H
!" ! "+
!" ! "+
!" ! "α, β =1,2,3 - generation index Dirac fermion mass
( )v
N N
y L N H
"# " #$ M
i!= Diag y
"# Dirac neutrino massThe Running Couplings The Running Couplings
( ) ( / ) ( )
Bare
Z
R! " = " µ ! µ
2 2
( / ) 1 ( / ) ...
Z " µ = # b Log ! " µ +
2 2 2 2 2 2
( / ) ( / ) ( / )
Log p Log Log p
! " # ! " µ = ! µ
Radiative Corrections
~α (log Λ
2/p
2+fin.part)
UV divergenceRenormalization operation
UV cutoff Renormalization scale Renormalization constant
Subtraction of UV div
Finite
R
( )
! µ
2d
2( ), ( )
2d
2( / )
Log Z
d d
µ ! " ! " ! µ µ
µ = = # µ $
Running coupling
Renormalization Group Renormalization Group
2 2 2 2 2
( , ( )) (1 ( ) ( ))
R
PTQ µ ! µ = ! + b Log Q ! µ + O !
2 2 2
2
(
2 2) 0
d d
R R
d d
µ µ µ !
µ µ µ !
" "
= + =
" "
2 2 2 2
2
2
( , ( )) (1, ( , ))
( )
RG PT
R Q R Q
Q d
dQ
µ ! µ ! µ !
! " !
=
=
Observable
RG Eq.
Solution to RG eq.
Effective coupling
! " ( )
Solution to RG eq. sums up an infinite series of the leading Logs coming from Feynman diagrams
2 2
2 2
(1, ) , (1 ( ) ...)
1 ( )
R
PTb Log Q
b Log Q
! ! ! ! ! ! µ
! µ
= = " + +
#
Asymptotic Freedom and Asymptotic Freedom and
Infrared Slavery Infrared Slavery
( ) b
2! " = "
One-loop order 4/3 nf QED
-11+2/3 nf QCD
2 2
1 b Log Q ( )
! !
! µ
= "
QED QCD
α_ α_
UV Pole IR Pole
Comparison with Experiment Comparison with Experiment
Global Fit to Data Higgs Mass Constraint
Remarkable agreement of ALL the data with the SM predictions - precision tests of radiative corrections and the SM
Though the values of sin ϑw extracted from different experiments are in good agreement, two most precise
measurements from hadron and lepton asymmetries disagree by 3σ
••
Inconsistency at high energies due to Landau poles Inconsistency at high energies due to Landau poles
• Large number of free parameters • Large number of free parameters
• Still unclear mechanism of EW symmetry breaking • Still unclear mechanism of EW symmetry breaking
• • CP-violation is not understood CP-violation is not understood
• • The origin of the mass spectrum in unclear The origin of the mass spectrum in unclear
• • Flavour Flavour mixing and the number of generations is arbitrary mixing and the number of generations is arbitrary
• Formal unification of strong and electroweak interactions • Formal unification of strong and electroweak interactions
Where is the Dark matter?
The SM and Beyond The SM and Beyond
The problems of the SM:
The problems of the SM:
The way beyond the SM:
The way beyond the SM:
••
The SAME fields with NEW The SAME fields with NEW interactions and NEW fields
interactions and NEW fields GUT, SUSY, String, ED GUT, SUSY, String, ED
••