unification paradigm unification of strong, weak and electromagnetic interactions within grand...
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Unification ParadigmUnification Paradigm
• Unification of strong, weak and electromagnetic interactions within Grand Unified Theories is the new step in unification of all forces of Nature• Creation of a unified theory of everything based on string paradigm seems to be possible
3410 m
D=10
GUT
What is SUSY?What is SUSY?
• Supersymmetry is a boson-fermion symmetrythat is aimed to unify all forces in Nature including gravity within a singe framework
• Modern views on supersymmetry in particle physicsare based on string paradigm, though low energymanifestations of SUSY can be found (?) at moderncolliders and in non-accelerator experiments
| | | |Q boson fermion Q fermion boson
[ , ] 0, { , } 0 b b f f { , } 2 ( )ji ijQ Q P
{ , } 2 ( )ji ijQ Q P
First papers in 1971-1972
No evidence in particle physics yet
Motivation of SUSY in Motivation of SUSY in Particle PhysicsParticle Physics
Unification with Gravity
| | | |
2 3/2 1 1/2 0
Q boson fermion Q fermion boson
spin spin spin spin spin
| | | |
2 3/2 1 1/2 0
Q boson fermion Q fermion boson
spin spin spin spin spin
Unification of matter (fermions) with forces (bosons) naturally arisesfrom an attempt to unify gravity with the other interactions
{ , } 2 ( ) { , } 2( )
( ) local coordinate transf. (super)gravity
ji ijQ Q P P
x
{ , } 2 ( ) { , } 2( )
( ) local coordinate transf. (super)gravity
ji ijQ Q P P
x
Unification with Gravity Unification of gauge couplings Solution of the hierarchy problem Dark matter in the Universe Superstrings
Local supersymmetry = general relativity !
Motivation of SUSY in Motivation of SUSY in Particle PhysicsParticle Physics
Unification of gauge couplings
c L Y
3 2 1
SU (3) SU (2) U (1) (or + symm)
,
nGUT
GUT
Low Energy High Energy
G G
gluons W Z photon gauge bosons
quarks leptons fermions
g g g g
c L Y
3 2 1
SU (3) SU (2) U (1) (or + symm)
,
nGUT
GUT
Low Energy High Energy
G G
gluons W Z photon gauge bosons
quarks leptons fermions
g g g g
Running of the strong coupling
2
2( ) (distance)Qi i i
Motivation of SUSYMotivation of SUSY
1
2
( ) 128.978 0.027
sin 0.23146 0.00017
( ) 0.1184 0.0031
Z
MS
s Z
M
M
2 2 2 2 2, / 4 /16 , t=log(Q / )ii i i i i
db g
dt
1
2
3
0 4 / 3 1/10
: 22 / 3 4 / 3 1/ 6
11 4 / 3 0i Fam Higgs
b
SM b b N N
b
1
2
3
0 2 3/10
: 6 2 1/ 2
9 2 0i Fam Higgs
b
MSSM b b N N
b
RG Equations
Input
Output
3.4 0.9 0.4
15.8 0.3 0.1
-1GUT
10 GeV
10 GeV
26.3 1.9 1.0
SUSY
GUT
M
M
SUSY yields unification!
Unification of the Coupling Constantsin the SM and in the MSSM
Motivation of Motivation of SUSYSUSY
• Solution of the Hierarchy Problem
2
16
v 10 GeV
m V 10 GeV
Hm
-14 10 1Hm
m
Destruction of the hierarchy byradiative corrections
Cancellation of quadratic terms
2 2
bosons fermions
m m SUSY may also explain the originof the hierarchy due to radiativemechanism
Motivation of SUSYMotivation of SUSY• Dark Matter in the UniverseDark Matter in the Universe
SUSY provides a candidate for the Dark matter – a stable neutral particle
The flat rotation curves of spiral
galaxies provide the most direct
evidence for the existence of large
amount of the dark matter.
Spiral galaxies consist of a central
bulge and a very thin disc, and
surrounded by an approximately
spherical halo of dark matter
Cosmological Cosmological ConstraintsConstraints
New precise cosmological data
2 1
73%
23 4%
4%
vacuum
DarkMatter
Baryon
h
crit •Supernova Ia explosion• CMBR thermal fluctuations
(recent news from WMAP )
Dark Matter in the Universe:
Hot DM(not favoured by galaxy formation)
Cold DM(rotation curvesof Galaxies)
SUSYSUSY
SuperalgebraSuperalgebra
1 12 2
[ , ] 0,
( ) lg
Lorentz Algebra
SUSY
[ , ] ( ),
[ , ] ( ),
[ , ] [ , ] 0
,
[ , ] ( ) ,
Algebra
[ , ]
i i
i i i
P P P M i g P g P
M M i g M g M g M g M
Q P Q P
Q M Q Q M
Super A ebra
( ) ,
{ , } 2 ( ) ,
, , , 1, 2; , 1, 2,..., .
i
ji ij
Q
Q Q P
i j N
1 12 2
[ , ] 0,
( ) lg
Lorentz Algebra
SUSY
[ , ] ( ),
[ , ] ( ),
[ , ] [ , ] 0
,
[ , ] ( ) ,
Algebra
[ , ]
i i
i i i
P P P M i g P g P
M M i g M g M g M g M
Q P Q P
Q M Q Q M
Super A ebra
( ) ,
{ , } 2 ( ) ,
, , , 1, 2; , 1, 2,..., .
i
ji ij
Q
Q Q P
i j N
, ,
Superspace
x x , ,
Superspace
x x
Grassmannian parameters
, 1, 2
Q i
Q i
22 0, 0
SUSY Generators
The only possible graded Lie algebra that mixes integer and half-integer spins and changes statistics
22 0, 0Q Q
{ , } 2 ( )ji ijQ Q P
,
,
Supertranslation
x x i i
Quantum StatesQuantum StatesQuantum states: | ,E Vacuum = | , 0Q E
Energy helicity
State Expression # of states
vacuum 1
1-particle
2-particle
… … …
N-particle
| ,E
| , | , 1/ 2iQ E E
| , | , 1i jQ Q E E
1 2... | , | , / 2NQ Q Q E E N
1N N
( 1)2 2
N NN
1NN
Total # of states: 1 1
0
2 2 2N
N N N Nk
k
bosons fermions
[ , ] [ , ] 0i iQ P Q P
SUSY MultipletsSUSY MultipletsChiral multiplet
Vector multiplet
1, =0N helicity
# of states
-1/2 0 1/2
1 2 1
1, =1/2N helicity
# of states-1 -1/2 1/2 1 1 1 1 1
( , )
( , )A
scalar spinor
spinor vector
Members of a supermultiplet are called superpartners
N=4 SUSY YM helicity -1 –1/2 0 1/2 1
λ = -1 # of states 1 4 6 4 1
N=8 SUGRA helicity -2 –3/2 –1 –1/2 0 1/2 1 3/2 2
λ = -2 # of states 1 8 28 56 70 56 28 8 1
4N S spin4N 8N
For renormalizable theories (YM)
For (super)gravity
Simplest (N=1) SUSY Simplest (N=1) SUSY MultipletsMultiplets
( , ) ( , )A
Bosons and Fermions come in pairs
( , )g gSpin 0 Spin 1/2 Spin 1Spin 1/2 Spin 3/2 Spin 2
SUSY TransformationSUSY Transformation
14
( , ) ( ) 2 ( ) ( )
( ) ( ) ( )
2 ( ) / 2 ( ) ( )
y A y y F y
A x i A x A x
x i x F x
N=1 SUSY Chiral supermultiplet:
( )y x i
component fields
spin=0
spin=1/2
Auxiliary field
2 ,
2 2 ,
2
A
i A F
F i
2 ,
2 2 ,
2
A
i A F
F i
parameter of SUSY transformation(spinor)
(unphysical d.o.f. needed to close SYSY algebra )
SUSY multiplets Superfiled in Superspace
Expansion over grassmannian parametersuperfield
2 2 21 2 1 2, 0!
Gauge Gauge superfieldssuperfields
1 12 2
( , , ) ( ) ( ) ( ) ( ) ( )
( ) [ ( ) ( )] [ ( ) ( )]
[ ( ) ( )]
V x C x i x i x i M x i M x
v x i x i x i x i x
D x C x
Gauge transformationV V
*
*
2
2
( )
C C A A
i
M M iF
v v i A A
D D
*
*
2
2
( )
C C A A
i
M M iF
v v i A A
D D
Wess-Zumino gauge
0C M
physical fields
Field strength tensor
214
V VW D e D e
22 ( )iW i D F D
D i
Covariant derivatives
D i
Gauge superfield
0, d d
4 ( )Action d x L x 4 4 ( , , )d x d L x
How to write SUSY How to write SUSY LagrangiansLagrangians
Grassmannian integration in superspace
1st step
2nd step
( , , ) ( , )Field A Superfield V
3rd step
Take your favorite Lagrangian written in terms of fields
Replace
Replace
Superfield Superfield LagrangiansLagrangians
2 2 2 1 12 3 ( ) . .]i i i i ij i j ijk i j kL d d d m y h c
Grassmannian integration in superspace 0, d d
Gauge fields
2 2 21 1 14 2 4 L d W W d W W D F F i D
2 2 21 1 14 2 4 L d W W d W W D F F i D
Gauge transformation , , ( )ig ige e V V i
Gauge invariant interaction gVe
4 Action d x L 4 4 d x d L
Superpotential
Matter fields
Gauge Invariant SUSY Gauge Invariant SUSY LagrangianLagrangian
2 21 1 4 4
2 2 2 2
Tr(W ) Tr(W )
( ) ( ) ( )
SUSY YM
gV a bia ib i i
L d W d W
d d e d d
W W
1 1 4 2
†
† † †
2 2† 1 1
2 2† † †
( ) ( ) ( )
2 2
aa a a a aSUSY YM
a a a a a aii i i i i i
aa a a a aii i i i i i i
i ji i i ji i i j i j
L F F i D D D
A igv T A A igv T A i igv T
D gA T A i gA T i g T A F F
F FA A A A A A
W W W W
† †12, V=a a a a
i i i i ii
D gA T A F D D F FA
W