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Transcript
Standard Model and beyond:
particles & interactions
Gabriel González Sprinberg
Instituto de Física, Facultad de Ciencias
Montevideo - Uruguay
[email protected]
ECOS-SUD
Gabriel González Sprinberg, July 2003
1
Mar 8, 14 h – Ven 11, 14 h – Mar 15, 10 h – Ven 18, 10 h
OUTLINE

Particles: matter and gauge bosons

Interactions (low and high energies regimes)

Symmetries: internal, external, continuous, discrete

Lagrangians and Feynman diagrams (quantum field theory by
drawing)

Some processes


A closer look to some examples
SM: experimental status and tests

Beyond the forest: models and phenomenology

Some extensions: grand unification, supersymmetry, ...

And their observables: proton decay, sparticles, neutrino masses and
oscillations...
Gabriel González Sprinberg, July 2003
2
SOME HISTORY
before ’30
 e, p, ; nucleus (A
p, A - Z
e)
 1925/6 Heisenberg/Schrödinger QM
Pauli exclusion principle
 1927/8 Dirac’s electron relativistic wave equation
Quantum electrodynamics
Magnetic moment for the electron
  decay in nuclei: a total mess
1914, e with continuous spectrum
missing energy (34% !!)
N. Bohr: energy-momentum not conserved (noninvariance under translations of Poincare group)
1930, Pauli was not so radical: a new particle must
exist
neutrinos
Gabriel González Sprinberg, July 2003
3
SOME HISTORY
after ‘30
 1931 Dirac prediction of positron and antiproton
 1932
Anderson: positron
Chadwick: neutron (  + Be
C+n)
Heisenberg nuclei: protons and neutrons
spin-statistics accomodates
 1934
n  p  e   e
Pauli explanation of  decay:
Fermi theory of weak interactions
e
NiZ  N fZ1  e   e
H int
GF


p

n
e

e 

 
2
n
GF / 2
Gabriel González Sprinberg, July 2003
p
e
4
SOME HISTORY
 1935 Yukawa predicts 
 1936 Gamow-Teller extension of Fermi theory
 1937 Majorana neutrino theory;  discovered
 1947 Pontecorvo universality of weak interactions in decay
and capture processes;  discovered
 1949 Universality of weak interactions for hadrons and
leptons; QED is a renormalizable theory
 1950- Hundreds of particles/resonances are found
 1954 Yang-Mills gauge theories
 1956/7 Parity violation proposal and evidence
 1957 Neutrino two component theory; intermediate vector
boson for weak interactions
 1958 Feynman and Gell-Mann; Marshak and Sudarshan;
Sakurai: universal V-A weak interactions
 1959 Detection of anti-neutrino
Gabriel González Sprinberg, July 2003
5
SOME HISTORY
 1961 SSB; Glashow neutral boson
 1964 Gell-Mann/Zweig quark model; proposal of charm; CP
violation in K0 mesons decays; Higgs mechanism; color QN
 1967 Weinberg EW model
 1970 GIM lepton-quark symmetry and charmed quarks (FCNC)
 1971 Renormalization of SSB gauge theories
 1973 Kobayashi-Maskawa CP model; evidence of the
predicted neutral current; Gross, Wilczek, Politzer
asymtotic freedom; Fritzsch, Gell-Mann, Leutwyler QCD
 1974-5 SLAC J/, 
 1977 Fermilab 
 1979 Gluon jets
 1983 Charged W and neutral Z bosons
 1995 Top quark
 1998-9 Neutrino oscillations @ SuperKamiokande
Gabriel González Sprinberg, July 2003
6
PARTICLES & INTERACTIONS
(matter and gauge bosons)
QUARKS S1/2
LEPTONS S1/2
GAUGE BOSONS S1
Q  2/3
Q  1/3
Q  1
Q  0
quanta
uu u
m=(1-4) 10-3
dd d
m=(5-8) 10-3
e
m=5.11 10-4
e
m<3 10-9
g1 …… g8
m< a few 10-3
c c c
m=1.0-1.4
s s s
m=0.08-0.15

m=0.10566

m<1.9 10-4

m<2 10-25
t t t
m=174.35.1
bb b
m=4.0-4.5

m=1.7770

m<18.2 10-3
W  , Z0
mW=80.432 0.39,
mZ=91.1876 0.0021
(mass in Gev/c2)
(plus antiparticles!)
Gabriel González Sprinberg, July 2003
7
PARTICLES & INTERACTIONS
Besides, there are hadrons, atoms, molecules…
HADRONS: Mesons ( qq )
Baryons (qqq states- fermions)
Pentaquarks…?
 0 K  …  … J/ …
p n  …  … b …
Is there any order in the list?
1.
2.
3.
Matter particles are not the same as the messengers of the
interactions, the gauge bosons
Particles are sensitive to different forces:
quarks couple directly to gluons, photons, weak bosons
leptons only to photons and weak bosons
There is some order in mass in leptons, not so evident in quarks
Other way to find some order:
Relate:
Gabriel González Sprinberg, July 2003
SYMMETRY

INTERACTIONS
8
“QUARKS, NEUTRONS,MESONS. ALL THOSE
DAMN PARTICLES YOU CAN’T SEE. THAT’S
WHAT DROVE ME TO DRINK. BUT NOW I CAN
SEE THEM !! “
Gabriel González Sprinberg, July 2003
9
SYMMETRIES
In classical physics:
Symmetry
space translation
time translation
rotation
 Conservation laws

momentum

energy
 angular momentum
These are continuous and external symmetries.
Some others may also be discrete:
space inversion  parity
High energy physics :
Relativistic (Lorentz invariant)
Quantum
Field theory
Is there any other symmetry principle?
Is there any other guide in order to construct our theories?
Gabriel González Sprinberg, July 2003
10
SYMMETRIES AND GAUGE THEORIES
Relativistic quantum field theory (as QED) is not enough, we need a
GAUGE THEORY
WHY?
Nice features about GAUGE THEORIES:
once the symmetry is chosen (internal symmetry group) the
interactions are fixed!
quantum corrections can be computed and are finite
consistency of the theory motivate for the seach of new particles
and interactions
the theory is full of predictions…
It is a gauge, Lorentz invariant, quantum field theory what is needed
Gabriel González Sprinberg, July 2003
11
TWO SLIDES GAUGE THEORY PRIMER (I)
Electrodynamics as an example:


2
1
H
p  qA  q
2m
gives the Lorentz force for a particle
in an electromagnetic field
Electric and magnetic fields are described by

A  (, A)

E   
; B   A
t
Fields remain the same with the gauge transformation (G):

   '    ; A  A '  A  
t
  ( x, t )
!!!
Now, what happens in quantum mechanics?
We quantize the Hamiltonian with the prescription
Gabriel González Sprinberg, July 2003
p  i
12
TWO SLIDES GAUGE THEORY PRIMER (II)
The Schrödinger equation for a particle in an electromagnetic field is
2
 ( x, t )
 1


i


qA

q


(
x
,
t
)

i
 2m

t


G
If we make a gauge transformation: (, A)  ( ', A ')
and, at the same time, we transform the wave function as
G
 ( x, t )   '( x, t )  exp(iq( x, t ))( x, t )
we obtain the same equation and the same physics, described either by
the original field and wave function or the transformed ones
G
(, A, )  ( ', A ',  ')
A particle in interaction with the EM field has a whole class of
“equivalent” potentials and wave functions related by the gauge group
G, and only one generator in the group (only one function )
Gabriel González Sprinberg, July 2003
13
QUANTUM ELECTRODYNAMICS AS A GAUGE THEORY
QED
Gauge theory with only one freedom in the gauge
function; this means in the group language U(1)
abelian-symmetry and we end up with one gauge boson,
the photon, and one coupling constant e that couples
matter and radiation.
Free electron Lagrangian has a global phase invariance:
L  (i   )  m
  exp(i )
Introducing a gauge field A (photon field) with the above
transformation rules, we have an invariant lagrangian with
interactions:
L  (i   eA )    m
kinetic term
mass term
interaction term
Gabriel González Sprinberg, July 2003
14
ELECTRODYNAMICS AS A GAUGE THEORY
Up to know, the EM field has no dynamics. This is introduced in a natural
way by the gauge invariant field EM tensor
F    A   A
LA  
1
F F 
4
Finally, the Lagrangian is
L   (i   eA )    m 
kinetic
e+
e
e-

A photon mass term
Gabriel González Sprinberg, July 2003
interaction
1
F F 
4
mass
kinetic
represents the interaction term
coupling:
LmA  
=e2/4 1/137
1 2
m A A
2
is not gauge invariant !!!!
15
ELECTRODYNAMICS: Feynman diagrams
All physical observables can be obtained with the Feynman diagrams:
d  M2 d (P.S.)
d  M2 d (P.S.)
The amplitude M is computed with all the possible Feynmann diagram
that contribute to the reaction.
For example:
time
(i)
e- 
e- 
virtual
(f)
Compton Effect
Gabriel González Sprinberg, July 2003
16
ELECTRODYNAMICS: some processes
e+ e+ (tree level)
e+
+
e-
e+
Bhabha
e+
e+
e-
e-
e-
e+ ee+ e(tree level)
e-
e+






(first order)
Gabriel González Sprinberg, July 2003
17
ELECTRODYNAMICS: e magnetic moment
One of the best known quantities in physics
One of the best predictions of the physical theories
e = ( 1.001 159 652 187  0.000 000 000 004 )
2 B
Dirac’s equation prediction: gyromagnetic factor
Anomalous magnetic moment = e / 2B –1 = ae
Computed to first order:
= /2  0.0011623
Schwinger
One can also compute to higher orders; for example:
Gabriel González Sprinberg, July 2003
18
ELECTRODYNAMICS: e magnetic moment
Third order diagrams...

 
 
 
ae   0.328 478 965    1.181 241 456    1.509 8(384)    4.393(27)  1012
2
 
 
 
2
Gabriel González Sprinberg, July 2003
3
4
weak and hadronic contributions
19
ELECTRODYNAMICS: some comments
Gauge invariance
Other terms:

"

eA


"
minimal coupling interaction term

2

 boson mass " m A A "
spoils not only gauge
invariance but also renormalizability


 higher order terms "  F ; F F ..."
are forbidden by causality or renormalizability

"

F F " , a CP-odd one but it
 only exception is
is a divergence, i.e. a surface term that can be eliminated
in QED (it is “-8E×B
“)
 only D4 terms respect renormalization
Gabriel González Sprinberg, July 2003
20
ELECTRODYNAMICS: some comments
Renormalization:
all the quantum corrections to the processes can be
taken into account by renormalizing the fields (A,)
and constants (m,e) in the lagrangian plus some finite
contributions; in this way no infinite quantities appear
in the physical results
In diagrams:
orders
This also means:
Gabriel González Sprinberg, July 2003
tree level +
e0
e A0
A
one loop
m0
m
+ higher
0

21
ELECTRODYNAMICS: some comments
The coupling constant is renormalized and depends on the scale !!
(running coupling constant)
electron charge  e(Q2=0)
the coupling constant (Q2)=e2(Q2)/4  runs with the scale
(Q2=0) = e2(0)/4  = 1/137.03599976(50)
(Q2=MZ2) = e2(MZ2)/4  = 1/127.934(27)
Gabriel González Sprinberg, July 2003
22
Allright Ruth, I about got this one renormalized
Gabriel González Sprinberg, July 2003
23
ELECTRODYNAMICS as a tool
Quarks have, besides flavour, a new quantum number
COLOUR
 e e   





4  2

3 q2
4  2 2
 e e  qq 
eq eq=1/3, 2/3
3 q2




At a given energy:
4  2
 e e  X hadrons 
3 q2

Rhad 
 ee  X 
 ee      



e
2
q
at lowest order
all q
  2  2  1  2  1  2 
 3           2
  3   3   3  
2
  eq  
2
2
2
2
2
all q
  2   1   1   2   1   11
 3  3    3    3    3    3    3
           
Gabriel González Sprinberg, July 2003
below
charm
above
bottom
24
ELECTRODYNAMICS as a tool
R
bottom
charm
CM ENERGY in GeV
Gabriel González Sprinberg, July 2003
25
QUANTUM CROMODYNAMICS: SU(3) GAUGE THEORY
U(1)QED  SU(3)Color with eight generators
8
eA  g s 
c
c 1
3 means that we have
2
Gc;


c  1, ...8
for the quark colors
8

c
c  
L '  q  i   gs 
G   q  mqq;
c 1 2


q

q
q
 
q
 
q  u, d , s , c , b , t
we sum in all flavors (u,d,s…) and also in colour
1 8
LG    G c  G c  G c     G c   G c   g s f cabG a  G b
4 c 1
LQCD  L ' LG
Gabriel González Sprinberg, July 2003
THESE NON ABELIAN TERMS ARE THE
MAIN DIFFERENCE WITH QED
26
QUANTUM CROMODYNAMICS: SU(3) GAUGE THEORY
LQCD
8

c
 q  i   gs 
G c
c 1 2

 
1 8
c
c 

q

m
qq

G
G


q

4
c

1

INTERACTIONS
DIAGRAM
 gs
,a
this index says which of the 8 gluon is
,b,q
,c,r
COUPLING
a
2

igs f abc  g ( p  q )  g (q  r )  g ( r  p) 
group structure factor
,a,p
,b
,a
,c
,d
Gabriel González Sprinberg, July 2003
 gs2  f abe f cde ( g g  g g ) 
f ace f bde ( g g  g g ) 
f ade f cbe ( g g  g g )
27
QUANTUM CROMODYNAMICS: SU(3) GAUGE THEORY
LQCD
8

c
 q  i   gs 
G c
c 1 2

 
1 8
c
c 

q

m
qq

G
G


q

4
c

1


Quark-gluon interactions are flavour independent

Physical states are believed to be colorless (confinement)

QCD exhibits asymtotic freedom: the coupling constant
decreases at high energies (short distances) and, as
contrary as QED has an anti-screening property

The low energy regime is no perturbative (alternatives:
lattice gauge theory, large number of colours limit, chiral
perturbation theory,....)

Low up-down masses define a regime where QCD has a new
symmetry, chiral symmetry, softly broken by up and down
masses (isospin is understood as the mu=md limit)

The CP-odd term "  F a  F a " is not forbidden
but a limit can be obtained from the neutron EDM:  < 10-10
Gabriel González Sprinberg, July 2003
28
QUANTUM CROMODYNAMICS: running coupling constant
Gabriel González Sprinberg, July 2003
29
MORE ON SYMMETRIES

“EXACT”: U(1)EM, SU(3)QCD,...

“ANOMALIES”: a classical symmetry of the hamiltonian can
be violated by quantum efects

“ALMOST SYMMETRY”: isospin, broken by mumd and by
electromagnetism

“HIDDEN SYMMETRY”: in invariance of the lagrangian it is
not necessarily an invariance of the ground state; the
symmetry is not realized in the physical states.
1. spontaneously broken
2. broken by quantum dynamical effects
Gabriel González Sprinberg, July 2003
30
WEAK INTERACTIONS ( are left)
HELICITY, PARITY VIOLATION AND NEUTRINOS

s
p
ˆs
hp
For
massless
neutrinos
(left-)
handedness (helicity h = -1/2) is a
relativistic invariant
Are neutrinos left? In that case WI are parity violating
GOLDHABER etal experiment : within this experiment the photon
helicity is the neutrino helicity
e- + 152Eu
152Sm*
+ e
152Sm
Gabriel González Sprinberg, July 2003
+
31
WEAK INTERACTIONS ( are left)
e- + 152Eu 
Jp
0-
Momenta
152Eu

e- capture
1-
152Sm*
+ e
Spin
 h=1/2
 h=-1/2
electron
electron
Sm*
Sm*


Sm*

0+
152Sm*
152Sm
Only  along the recoiling
152Sm* selected
Helicities of the  and the  are the same !!
It was found that h=-1 always
THE
Gabriel González Sprinberg, July 2003
 IS ALWAYS LEFT-HANDED
32
WEAK INTERACTIONS (helicity and handedness)
Left and right particles in field theory:
(1   5 )
L 
 left handed particle
2
(1   5 )
R 
 right handed particle
2
(helicity and handedness are equal only in the m=0 limit)
Parity is not violated in a theory with a symmetric treatment of L and R
mass terms
   R L  L R
QED interaction
    L  L   R  R
WI are parity violating, so L and R fields are treated in a different way
Gabriel González Sprinberg, July 2003
33
WEAK INTERACTIONS (V-A)
The Fermi model for lepton/hadron interactions has to be extended
to explicitely include
1. parity violation
2. only left neutrinos
H int
GF

e   e      

2
H int
GF

e   1   5  e     1   5   

2
2eL  L
2 L   L
We may also have neutral currents, such as a combination of the terms:

 L  L ;

lL lL ;

lR lR
WI also imposes other constraints to the lagrangian.
Gabriel González Sprinberg, July 2003
34
WEAK INTERACTIONS ( flavours, leptons are left)
We do not observe
   e
   e e 
the decay
Br < 1.2x10-11; if the two neutrinos in
had the same “lepton flavour” this decay
would be possible: but we have different neutrinos!
  f  f ; f  e, 

We measure that in the process

the lepton is always right handed, then the anti-neutrino is also right
handed. If one assumes that only left-handed leptons participate in the
WI then this decay should be forbidden in the zero-mass limit (where
helicity is identical with handedness). The extended Fermi model
H int 
gives
Re / 


 
    e  e

   
G
u   1   5  d   e   1   5  e 

2
  m 1  m
 m 1  m
2
e
2
e
m2
2
2
m2

in agreement with experiment:
Gabriel González Sprinberg, July 2003

 1    (1.2352  0.0005)  10



4
QED
Re /   (1.230  0.004)  104
35
WEAK INTERACTIONS (IVB)
Intermediate vector boson:
the extended V-A Fermi Model is not renormalizable and at high
energies predicts
GF2 q 2


   e    e  

that violates the unitarity bound

2
q2
The extended Fermi hamiltonian:
Hint =
G  †
J J
2
J   u   (1-  5 )d    e  (1-  5 )e      (1-  5 )    ...
is only correct at low energies.
Gabriel González Sprinberg, July 2003
36
WEAK INTERACTIONS (IVB)
We assume that the charged current couples to a charged massive
vector boson:
g
Hint =
J W†  h.c.

2 2
The V-A interaction is generated through W-exchange:

-
-

W-
ee-
e
e
In the limit MW  
-1
1

q 2  M W2
M W2
we find
GF
g2

8M W2
2
Gabriel González Sprinberg, July 2003
( g < 1 implies MW < 123 GeV)
37
WEAK INTERACTIONS (neutral currents)
Neutral currents:
in 1973 the elastic scattering
confirms their existence
  e    e
Extensively analyzed in many experiments; in contrast to charged
interactions one finds that flavour changing neutral-currents (FCNC) are
very suppressed: the Z couplings are flavour diagonal
e-


    eee

 e  e 
  10

12
Z
e-
e+
(this diagram does not exist)
What are all the ingredients for a theory of WI?
Gabriel González Sprinberg, July 2003
38
WEAK INTERACTIONS (ingredients)
 intermediate spin-1 massive bosons Z0, W+ ,W- and  (4 of them)
 electroweak unification
that together with
gW
g
 Z e
2 2 2 2
GF
g2

8M W2
2
imply
MW  100 GeV
 The W field couples only to left handed doublets
 e 
 
 e L
  
 
  L
u 
 
 d ' L
 The Z only with flavour diagonal couplings (FCNC)
 Lepton number conservation
 Renormalizability
Gabriel González Sprinberg, July 2003
39
WEAK INTERACTIONS (the group)
Schwinger 1957 tried O(3); Bludman 1958 tried SU(2); finally Glashow
in 1960 proposed SU(2)U(1); Salam and Ward did something similar in
1964.
G  SU (2) L U (1)Y
L: only left fields are transformed by the gauge group
Y: hyphercharge
A total consistent theory can be written in this way for each family:
 e 
 
 e L
eR
u 
 
 d ' L
uR
dR
Gabriel González Sprinberg, July 2003
  
 
  L
c
R  
 s L
sR
cR
  
 
 L
t 
R  
 b L
tR
bR
40
A CLOSER LOOK TO THE WI GAUGE GROUP
u 
1   
 d L
 2  uR
 3  dR
 j  'j  exp i  j1 exp iY j   j
G
SU(2)L  3 generators  3 bosons W1 W2 W3
U(1)Y  1 generator  1 bosons B
Physical bosons W Z  are linear combinations of these fields:
W3 = cosW Z + sinW A
B = -sinW Z + cosW A
The kinetic terms for the gauge fields, the interaction terms obtained
from the gauge invariance give us all the terms that define the weak
interactions:
Gabriel González Sprinberg, July 2003
41
A CLOSER LOOK TO THE WI GAUGE GROUP
Lkin. gauge  
3
1
1
B B   W W 
4
4
L    j iD   j ;

j 1
D j  (   ig

2
 W  ig ' Y j B ) j
What do we have here?
What we do not have here!
1.
1. fermion masses
charged current interactions
2. neutral current interaction
2. gauge boson masses
3. QED
4. Gauge self interactions
How do we generate mass without breaking gauge invariance and
renormalizability?
Gabriel González Sprinberg, July 2003
42
WEAK INTERACTIONS (some diagrams)
W
, d
e, u
W
W,Z,A,Z
W
W,Z,A,A
e+, u, 
Z
, Z
e-, u, 
Gabriel González Sprinberg, July 2003
W
W
43
STANDARD MODEL (group, mass)
GSM  SU (3)C  SU (2) L U (1)Y
GEW  SU (2) L U (1)Y
In the GEW structure we have 6 different quark flavour (u, d, s, c, b,t),
3 different leptons (e, , ) with their neutrinos (e, , ).
These are organized in 3 identical copies (families) with masses as the
only difference.
Mass in a gauge renormalizable theory
1. Fermion masses:    R L  L R
L and R are mixed, so
gauge inv., but also renormalizability are spoiled by these terms.
2. Boson masses: no gauge invariance neither renormalizability with a
mass term.
A way out is provided by the Goldstone/Higgs mechanism
Gabriel González Sprinberg, July 2003
44
STANDARD MODEL (Higgs)
Complex scalar field with a
spontaneously broken symmetry:
1. this is the case with quadratic
plus quartic
terms in the
lagrangian (Mexican hat)
2. there are infinite states with
the minimum energy, and by
choosing a particular solution the
symmetry
gets
spontaneously
broken
3. fluctuations around this ground
state (1=v,
2=0) defines a
massless and a massive excitation
(Goldstone theorem: if a lagrangian is invariant unader a
continuous symmetry group G, but the vacuum is only
invariant under a subgroup H  G, then there must exist
as many massless spin-0 particles (Goldstone bosons) as
broken generators (i.e. generators of G which do not
belong to H)
Gabriel González Sprinberg, July 2003
45
STANDARD MODEL (Higgs)
4. What happens if the scalar field is in interaction with the gauge
bosons by means of a local gauge symmetry?
D  (   ig
 D 
†

2
 
   0

 W  ig ' Y B )

 0






v  H 

2
1
g2
2 g

†

 
D    H  H  v  H  
W W 
Z
Z


2
2
4
8
cos

W



And we have a mass term for the W and the Z:
M Z cosW  MW  vg
2
5. The same idea for the fermions, where the interaction term is the
most general gauge invariant interaction between the fermions and the
Higgs doublet (“Yukawa term”):
LYukawa
1

 v  H  c1ee  c2uu  c3dd 
2

me   c1v 2; mu   c2v 2; md   c3v 2
Gabriel González Sprinberg, July 2003
46
STANDARD MODEL (Higgs)
Using the equations
e  g sin W
GF
g2

8M W2
2
we have
M Z cosW  MW  vg
2
vacuum expectation value of the Higgs field
MW
  
 

 GF 2 
1
2
1
37.28GeV

;
sin W
sin W
v

2GF

1
2
 246GeV
Measuring the weak angle (or the Z mass) we have a prediction for the
masses, but what about MH? It is a free parameter...
We have also generated interaction terms for the Higgs particle with
the bosons and the fermions of the SM....
Gabriel González Sprinberg, July 2003
47
STANDARD MODEL (Higgs)
H
W
2
H
H
H
M

246GeV
Z
M Z2

246GeV
H
H
H
H
H
H
Z
W
H
Z
H
H
M W2

246GeV
W
H
W
f
H
Z
Gabriel González Sprinberg, July 2003

f
mf
246GeV
Note: Higgs physics
remains perturbative
and also  < MH iff
MH  102-3 GeV
48
STANDARD MODEL (mixing)
• The weak eigenstates (the ones that transforms with the EW
group) are linear combinations of the mass eigenstates (physical
states)
• This enters in the Yukawa coupling terms that generate the
fermion masses.
• For 3 families we need 3 angles and 1 phase in order to
parametrize this in the most general way: Cabibbo-KobayashiMaskawa (CKM) unitary matrix.
• This imaginary component is the only responsible for CP violation
in the SM.
Gabriel González Sprinberg, July 2003
49
STANDARD MODEL (mixing)
 dW

Weak eigenstates  sW
b
 W

 Vud Vus Vub   d 


 

V
V
V

 cd cs cb   s  Mass eigenstates

V V V   b 
 L  td ts tb    L
c12 = cos 12  0, etc...
Values obtained from weak quark decays and deep inelastic neutrino
scattering
Gabriel González Sprinberg, July 2003
50
STANDARD MODEL (parameters,status)
FREE PARAMETERS
Gauge and scalar sector:
, MZ, GF, MH (most precisely known)
Other, like MW, W, g, g’, Higgs self-coupling,
are determined from these ones
GF = ( 1.166 39  0.000 02)  10-5 GeV2
-1 = 137.035 999 76  0.000 000 50
MZ = 91.1876  0.0021 GeV2
Yukawa sector:
QCD:
Gabriel González Sprinberg, July 2003
9 masses (6 quarks, 3 leptons)
3 angles
1 phase
S(MZ2)
(  ???)
51
STANDARD MODEL (status)
There is a huge amount of data to support the SM:
cross sections, decay widths, branching ratios, asymmetries, polarization
measurements, ......
Many of them at the 1/1000 level.
Gabriel González Sprinberg, July 2003
52
Z-LEPTON COUPLINGS (Mt , MH)
f
Z
f

Gabriel González Sprinberg, July 2003
e
   gV  g A 5 
sin 2W
53
WW PRODUCTION AT LEP2
e+
( e+ e-  W+ W)
Gabriel González Sprinberg, July 2003
e- 
W+
W-
Z

54
W TO LEPTONS
Gabriel González Sprinberg, July 2003
55
TOP FROM LEP
Gabriel González Sprinberg, July 2003
56
NEUTRINO AND FAMILIES (number of l and q)
Number
of
light
neutrinos (m < 45 GeV)
For the Z:
inv = Z - 3 l - had
 inv = 500.1  1.9 GeV
 inv / l = 5.961  0.023
 inv = N  
(  /  l)SM=1.991  0.001
N = 2.9841  0.0083
SM fits to data
Gabriel González Sprinberg, July 2003
57
Z-LEPTON WIDTH AND WEAK ANGLE
Gabriel González Sprinberg, July 2003
58
W MASS AND WEAK ANGLE
Gabriel González Sprinberg, July 2003
59
H MASS AND WEAK ANGLE
Gabriel González Sprinberg, July 2003
60
HIGGS MASS (Mt , MW)
Gabriel González Sprinberg, July 2003
61
HIGGS MASS
For the Higgs physics to remain perturbative and also  < MH we need
MH  102-3 GeV
But:
1. From radiative corrections
MH < 190 GeV
2. No Higgs observation at LEP2
MH > 113 GeV
Gabriel González Sprinberg, July 2003
62
STANDARD MODEL (pull)
PULL=
Gabriel González Sprinberg, July 2003
data point-fit value
error on data point
63
HIGH ENERGY ACCELERATORS (mass)
Constituent CM Energy (GeV)
10
4
Accelerators
10
LHC
electron
hadron
3
Higgs boson
Tevatron
10
SppS
2
LEPII
SLC
TRISTAN
t quark
W, Z bosons
PEP
CESR
10
1
ISR
SPEAR
10
b quark
c quark
0
Prin-Stan
s quark
10
-1
1960
1970
1980
1990
2000
2010
Starting Year
Gabriel González Sprinberg, July 2003
64
SM CONCEPTUAL PROBLEMS
Why we just find the Higgs and declare the game is over?
(we did not find it yet!!!)
 Too many parameters
 Why such an strange EW group
 Why 3 families
 What is the origin of the masses ( MEW  GF-1/2  200 GeV)
 Why is the origin of the electric charge quantization
...............
From theory: hierarchy problem
From “experiment”:
Gabriel González Sprinberg, July 2003
• Coupling unification
• Neutrino masses
• Dark matter
• Baryogenesis
•••
65
BEYOND THE SM
WHAT WE SEE IS JUST A SMALL PART OF WHAT IS POSSIBLE !!!
Gabriel González Sprinberg, July 2003
66
BEYOND THE SM
First priority in particle physics:
Test by experiment the physics of the EW symmetry breaking sector
of the SM
Search for new physics beyond the SM: there are strong arguments to
expect new phenomena not far from the Fermi scale (at ≤ few TeV).
LHC has been designed for that.
2ECOM~14 TeV
Gabriel González Sprinberg, July 2003
Start in 2007
67
SUPERSYMMETRY (hierarchy problem)
The low energy theory must be renormalisable as a necessary
condition for insensitivity to physics at higher scale :
[the cutoff  can be seen as a parametrisation of our ignorance of
physics at higher scales]
But, as this scale  is so large, in addition the dependence of
renormalized masses and couplings on this scale must be reasonable:
e.g. a mass of order mW cannot be linear in the new scale 
But in SM indeed mh, mW...
are linear in  !!!!!!
(the scale of new physics beyond the SM)
Gabriel González Sprinberg, July 2003
68
SUPERSYMMETRY (hierarchy problem)
e.g. the top loop:
h
t
h
mh2=m2bare+mh2
M
2
H top
3GF 2 2
2

mt    0.3 
2
2
The hierarchy problem demands new physics near the weak scale
•  >> mZ: the SM is so good at LEP
•  ~ few times GF-1/2 ~ o(1TeV) for a natural explanation of MH or MW
Other conceptual problems (why 3 families, why such masses...)
has to be posponed to the time where the high energy theory will
be known
Gabriel González Sprinberg, July 2003
69
SUPERSYMMETRY (hierarchy problem)
Extra boson-fermion symmetry and then the
quadratic divergence is exactly cancelled
Gabriel González Sprinberg, July 2003
70
GRAND UNIFICATION (GUT’s and supersymmetry)
Is there a bigger group that naturally includes all the SM groups
without a direct product? If this is possible we have a grand
unification theory (EM,Weak,Strong). Quarks and lepton are then
organized in multiplets, and “weak” transition between them
becomes possible: proton decay ( p  0 + e+, ...)
From QED(mZ), sin2W measured at LEP predict  s(mZ) for
unification (assuming desert)
Non SUSY GUT's
EXP: s ( mZ ) = 0.119 ± 0.003
Present world average
s(mZ)=0.073±0.002
SUSY GUT's
s(mZ)=0.130±0.010
Proton decay: Far too fast without SUSY
Gabriel González Sprinberg, July 2003
71
GRAND UNIFCATION (supersymmetry)
Coupling unification: Precise matching of gauge couplings at MGUT
fails in SM and is well compatible in SUSY
SUSY is important for GUT's
Gabriel González Sprinberg, July 2003
72
BEYOND THE SM
WHAT WE SEE IS JUST A SMALL PART OF WHAT IS POSSIBLE !!!
 oscillations !!!!!!!
 masses !!!!
Gabriel González Sprinberg, July 2003
73
TO GO BEYOND THIS LECTURES
Elementary level:
more stress in phenomenology
D.H.Perkins, Intr. to high energy physics
F.Halzen, A.D.Martin, Quarks and leptons
more stress in theory
Leite Lopes, Gauge field theory, an introduction
Higher level:
I.J.R.Aitchison, Gauge theories in particle physics
more stress in phenomenology
E.D.Commins, P.H.Bucksbaum, Weak interactions
T.P.Cheng, L.F:Li, Gauge theories of elem. part. phys.
more stress in theory
Chanfray, Smajda, Les particules et leurs symetries
M.E.Peskin, D.V.Schroeder, Quantum Field Theory
Gabriel González Sprinberg, July 2003
74