Introduction to Supersymmetry in Elementary Particle Physics
Simon Albino II. Institute for Theoretical Physics at DESY, University of Hamburg simon@mail.desy.de
Every Thursday 8:30-10:00am, starting 17.04.2008, in seminar room 5, DESY
Lecture notes at www.desy.de/~simon/susy.html
Abstract
These lectures aim towards supersymmetry relevant for near-future high energy experiments, but some technical footing in supersymmetry and in symmetries in general is given first. We discuss various motivations for and consequences of a fermion-boson symmetry. The two most physically relevant types of supermultiplet are discussed, followed by a redetermination of their content and properties from the simpler superfield formalism in superspace, in which supersymmetry is naturally manifest. The construction of supersymmetric Lagrangians is determined, from which the minimally supersymmetric extension of the Standard Model and its consequences for grand unification are derived. The physically required soft supersymmetry breaking is applied to the MSSM to obtain constraints on the mass eigenstates and spectrum. We will begin with a self contained development of continuous internal and external symmetries of particles in general, followed by a determination of the external symmetry properties of fermions and bosons permitted in a relativistic quantum (field) theory, and we highlight the importance of the Lagrangian formalism in the implementation of symmetries and its applicability to the Standard Model and the MSSM. Contents
1 Quantum mechanics of particles 1
1.1 Basic principles ...... 1
1.2 Fermionic and bosonic particles ...... 3
2 Symmetries in QM 5
2.1 Unitary operators ...... 5
2.2 (Matrix) Representations ...... 9
2.3 External symmetries ...... 15
2.3.1 Rotation group representations ...... 15
2.3.2 Poincar´eand Lorentz groups ...... 19
2.3.3 Relativistic quantum mechanical particles ...... 21
2.3.4 Quantum field theory ...... 24
2.3.5 Causal field theory ...... 26
2.3.6 Antiparticles ...... 27 2.3.7 Spin in relativistic quantum mechanics ...... 28
2.3.8 Irreducible representation for fields ...... 30
2.3.9 Massive particles ...... 31
2.3.10 Massless particles ...... 32
2.3.11 Spin-statistics connection ...... 34
2.4 External symmetries: fermions ...... 36
1 2.4.1 Spin 2 fields ...... 36
1 2.4.2 Spin 2 in general representations ...... 43
2.4.3 The Dirac field ...... 47
2.4.4 The Dirac equation ...... 49
2.4.5 Dirac field equal time anticommutation relations ...... 50
2.5 External symmetries: bosons ...... 51
2.6 The Lagrangian Formalism ...... 54
2.6.1 Generic quantum mechanics ...... 54
2.6.2 Relativistic quantum mechanics ...... 55 2.7 Path-Integral Methods ...... 57
2.8 Internal symmetries ...... 58
2.8.1 Abelian gauge invariance ...... 60
2.8.2 Non-Abelian gauge invariance ...... 62
2.9 The Standard Model ...... 64
2.9.1 Higgs mechanism ...... 66
2.9.2 Some remaining features ...... 70
2.9.3 Grand unification ...... 72
2.9.4 Anomalies ...... 74
3 Supersymmetry: development 75
3.1 Why SUSY? ...... 75
3.2 Haag-Lopuszanski-Sohnius theorem ...... 79
3.3 Supermultiplets ...... 86
3.3.1 Field supermultiplets (the left-chiral supermultiplet) ...... 90
3.4 Superfields and Superspace ...... 94 3.4.1 Chiral superfield ...... 98
3.4.2 Supersymmetric Actions ...... 101
3.5 Spontaneous supersymmetry breaking ...... 105
3.5.1 O’Raifeartaigh Models ...... 106
3.6 Supersymmetric gauge theories ...... 107
3.6.1 Gauge-invariant Lagrangians ...... 112
3.6.2 Spontaneous supersymmetry breaking in gauge theories ...... 118
4 The Minimally Supersymmetric Standard Model 120
4.1 Left-chiral superfields ...... 120
4.2 Supersymmetry and strong-electroweak unification ...... 124
4.3 Supersymmetry breaking in the MSSM ...... 126
4.4 Electroweak symmetry breaking in the MSSM ...... 134
4.5 Sparticle mass eigenstates ...... 139
5 Supergravity 141 1 1 Quantum mechanics of particles
1.1 Basic principles
Physical states represented by directions of vectors (rays) i in Hilbert space of universe. | i
Write conjugate transpose i † as i , scalar product j † i as j i . | i h | | i · | i h | i
Physical observable represented by Hermitian operator A = A† such that A = i A i . h ii h | | i Functions of observables represented by same functions of their operators, f(A).
Errors i A2 i A 2 etc. vanish when i = a , h | | i−h ii | i | i where A a = a a , i.e. a is A eigenstate, real eigenvalue a. a form complete basis. | i | i | i | i If 2 observables A, B do not commute, [A, B] = 0, eigenstates of A do not coincide with those of B. 6 If basis X(a, b) are A, B eigenstates, any i = C X obeys [A, B] i = 0 = [A, B]=0. | i | i X iX| i | i ⇒ P If A, B commute, their eigenstates coincide.
AB a = BA a = aB a , so B a a . | i | i | i | i∝| i 2 Completeness relation: a a = 1 . a | ih | P Expand i = W a then act from left with a′ W ′ = a′ i , so i = a a i | i a ia| i h | −→ ia h | i | i a | ih | i P P 2 Probability to observe system in eigenstate a of A to be in eigenstate b of B: Pa b = b a . | i | i → |h | i| Iα Pa b are the only physically meaningful quantities, thus i and e i for any α represent same state. → | i | i
a Pb a = 1 for some state b as expected. b = a a b a . Act from left with b gives 1 = a a b b a . → | i | i h | i| i h | h | ih | i P P P Principle of reversibility: Pa b = Pb a. b a = a b ∗ → → h | i h | i
IHt Time dependence: Time evolution of states: i, t = e− i , H is Hamiltonian with energy eigenstates. | i | i 2 IHt Probability system in state i observed in state j time t later = Mi j , transition amplitude Mi j = j e− i . | i | i | → | → h | | i IHt IHt Average value of observable Q evolves in time as Q (t)= i e Qe− i . h ii h | | i Q is conserved [Q, H]=0 ( Q (t) independent of t). ⇐⇒ h i 3 1.2 Fermionic and bosonic particles
Particle’s eigenvalues = σ. Particle states σ, σ′, ... completely span Hilbert space. Vacuum is 0 = . | i | i |i
σ, σ′, ... = σ′, σ, ... for bosons/fermions. Pauli exclusion principle: σ, σ, σ′... =0 if σ fermionic. | i ±| i | i
Iα 2Iα Iα σ, σ′,... and σ′,σ,... are same state, σ, σ′,... = e σ′,σ,... = e σ, σ′,... = e = 1. | i | i | i | i | i ⇒ ±
Creation/annihilation operators: aσ† σ′,σ′′, ... = σ, σ′,σ′′, ... , so σ, σ′, ... = aσ† a† . . . 0 . | i | i | i σ′ | i
[aσ† , a† ] =[aσ, aσ ] = 0 (bosons/fermions). σ′ ∓ ′ ∓
σ, σ′,... = a† a† ′ ... = σ′,σ,... = a† ′ a† ... | i σ σ | i ±| i ± σ σ| i a removes σ particle = a 0 =0. σ ⇒ σ| i
E.g. (a σ′, σ′′ )† σ′′′ = σ′, σ′′ (a† σ′′′ ) = 0 unless σ = σ′, σ′′′ = σ′′ or σ = σ′′, σ′′′ = σ′. i.e. a σ′, σ′′ = δ ′′ σ′ δ ′ σ′′ . σ| i ·| i h | σ| i σ| i σσ | i± σσ | i
[aσ, a† ] = δσσ . σ′ ∓ ′
e.g. 2 fermions a† ′′ a† ′′′ 0 : Operator a† a ′ replaces any σ′ with σ, must still vanish when σ′′ = σ′′′. σ σ | i σ σ
Check: (a† a ′ )a† ′′ a† ′′′ 0 = a† a† ′′ a ′ a† ′′′ 0 + δ ′ ′′ a† a† ′′′ 0 = δ ′ ′′′ a† a† ′′ 0 + δ ′ ′′ a† a† ′′′ 0 . σ σ σ σ | i − σ σ σ σ | i σ σ σ σ | i − σ σ σ σ | i σ σ σ σ | i 4 ∞ ∞ † † Expansion of observables: Q = N=0 M=0 CNM;σ ...σ ;σ ...σ1 a ...a aσM ...aσ1. 1′ N′ M σ1′ σN′ P P Can always tune the CNM to give any values for 0 aσ′ ...aσ′ Qa† ...a† 0 . h | 1 L σ1 σK | i
Commutations with additive observables: [Q, aσ† ]= q(σ)aσ† (no sum) , where Q is an observable such that for σ, σ′,... , total Q = q(σ)+ q(σ′)+ . . . and Q 0 = 0 (e.g. energy). | i | i
Check for each particle state: Qa† 0 = q(σ)a† 0 + a† Q 0 = q(σ)a† 0 , σ| i σ| i σ | i σ| i
Qa† a† ′ 0 = a† Qa† ′ 0 + q(σ)a† a† ′ 0 = a† a† ′ Q 0 + q(σ′)a† a† ′ 0 + q(σ)a† a† ′ 0 = (q(σ) + q(σ′))a† a† ′ 0 etc. σ σ | i σ σ | i σ σ | i σ σ | i σ σ | i σ σ | i σ σ | i Note: Conjugate transpose is [Q, a ]= q(σ)a . σ − σ
Number operator for particles with eigenvalues σ is a† aσ (no sum). E.g. (a† aσ)a† a† a† ′ 0 = 2a† a† a† ′ 0 . σ σ σ σ σ | i σ σ σ | i
Additive observable: Q = σ Qσaσ† aσ . E.g. Q = H, (free) Hamiltonian, Qσ = Eσ, energy eigenvalues. P 5 2 Symmetries in QM
2.1 Unitary operators
Symmetry is powerful tool: e.g. relates different processes.
Symmetry transformation is change in our point of view (e.g. spatial rotation / translation), does not change experimental results. i.e. all i U i does not change any j i 2. | i −→ | i |h | i| Continuous symmetry groups G require U unitary:
j i j U †U i = j i , so U †U = UU † = 1 , includes U = 1. h | i→h | | i h | i Wigner + Weinberg: General physical symmetry groups require U unitary,
or antiunitary: j i j U †U i = j i ∗ = i j , e.g. (discrete) time reversal. h | i→h | | i h | i h | i
A unaffected (and f(A) in general), so must have A UAU † . h i h i →
IHt IHt Transition amplitude Mi j unaffected by symmetry transformation, i.e. j U †e− U i = j e− i , → h | | i h | | i which requires [U, H] = 0 if time translation and symmetry transformation commute. 6 Parameterize unitary operators as U = U(α), αi real, i = 1, ..., d(G). d(G) is dimension of G, minimum no. of paramenters required to distinguish elements.
Choose group identity at α = 0, i.e. U(0) = 1.
So for small α , can write U(α) 1 + It α . i ≈ i i ti are the linearly independent generators of G. Since U †U = 1, ti = ti†, i.e. ti are Hermitian .
[U, H]=0 = [t ,H] = 0, so conserved observables are generators. ⇒ i 1 Can replace all t t′ = M t if M invertible and real, then α′ = α M − real. i → i ij j i j ji
In general, U(α)U(β)= U(γ(α, β)) (up to possible phase eIρ, removable by enlarging group). 7 U(α) = exp [It α ] if Abelian limit is obeyed: for β α , U(α)U(β)= U(α + β) i i i ∝ i (usually true for physical symmetries, e.g. rotation about same line / translation in same direction).
Can write U(α)=[U(α/N)]N , then for N is [1 + It α /N + O(1/N 2)]N = exp[It α ] + O 1 . → ∞ i i i i N
Lie algebra: [ti, tj]= ICijktk , where Cijk are the structure constants
1 appearing in U(α)U(β)= U(α + β + 2ICαβ + cubic and higher)
2 2 (where (Cαβ)k = Cijkαiβj, and no O(α ) ensures U(α)U(0) = U(α), likewise no O(β )).
LHS: eIαteIβt 1 + Iαt 1(αt)2 1 + Iβt 1(βt)2 ≈ − 2 × − 2 1 + I(αt + βt) 1 (αt)2 + (βt)2 + 2(αt)(βt) ≈ − 2 h i I(α+β+ 1 ICαβ)t 1 1 1 2 RHS: e 2 1 + I(α + β + ICαβ)t (α + β + ICαβ)t ≈ 2 − 2 2 1 + I(αt + βt + 1ICαβt) 1 (αt)2 + (βt)2 + (αt)(βt) + (βt)(αt) , ≈ 2 − 2 h i 1 1 i.e. 2ICijkαiβjtk = 2 [αiti, βjtj].
Now take all α , β zero except e.g. α = β = ǫ IC t =[t ,t ] etc., gives Lie algebra. i j 1 2 → 12k k 1 2 8 In fact, Lie algebra completely specifies group in non-small neighbourhood of identity.
This means that for U(α)U(β)= U(γ), γ = γ(α, β) can be found from Lie algebra.
We have shown this above in small neighbourhood of identity, i.e. to 2nd order in α, β, only.
Check to 3rd order: Write X = αiti, Y = βiti, can verify that 1 I exp[IX] exp[IY ] = exp[I(X + Y ) [X,Y ]+ ([X, [Y, X]]+[Y, [X,Y ]]) + quadratic and higher]. − 2 12 has the form Iγiti, γi real | {z }
Lie algebra implies: 1. C = C (antisymmetric in i, j). Cijk can be chosen antisymmetric in i,j,k (see later). ijk − jik
2. Cijk real.
Conjugate of Lie Algebra is t†,t† = IC∗ t† , which is negative of Lie Algebra because t† = t . j i − ijk k i i h i
Thus Cijk∗ tk = Cijktk, but tk linearly independent so Cijk∗ = Cijk.
2 Iα t 2 Iα t 2 3. t = tjtj is invariant (commutes with all ti, so tranforming give e i it e− k k = t ).
[t2,t ] = t [t ,t ]+[t ,t ]t = IC t ,t = 0 by (anti)symmetry in (j, i) j,k. i j j i j i j jik{ j k}
Examples: Rest mass, total angular momentum. tjtj doesn’t have to include all j, only subgroup. 9 2.2 (Matrix) Representations
Physically, matrix representation of any symmetry group G of nature formed by particles:
( ) General transformation of aσ† : U(α)aσ† U †(α)= Dσσ (α)a† , with invariant vacuum: U(α) 0 = 0 . ′ σ′ | i | i
U(α)a† 0 is 1 particle state, so must be linear combination of a† ′ 0 , i.e. U(α)a† 0 = D ′ (α)a† ′ 0 . σ| i σ | i σ| i σσ σ | i
Thus U(α)a† a† ′ 0 = D ′′ (α)D ′ ′′′ (α)a† ′′ a† ′′′ 0 etc. σ σ | i σσ σ σ σ σ | i D α ti t , t IC t ( ) matrices furnish a representation of G , matrix generators ( )σ′σ with same Lie algebra [ i j]σσ′ = ijk( k)σσ′.
Since U(α)U(β) = U(γ), must have Dσ′′σ′ (α)Dσ′σ(β) = Dσ′′σ(γ).
Iαiti If Abelian limit of page 7 is obeyed, Dσ σ(α)= e . ′ σ′σ