supersymmetric field theories
play

Supersymmetric field theories Antoine Van Proeyen Antoine Van - PowerPoint PPT Presentation

Supersymmetric field theories Antoine Van Proeyen Antoine Van Proeyen KU Leuven Summer school on Differential Geometry and Supersymmetry, September 10-14, 2012, Hamburg Based on some chapters of the book Supergravity Wess, Zumino


  1. Supersymmetric field theories Antoine Van Proeyen Antoine Van Proeyen KU Leuven Summer school on Differential Geometry and Supersymmetry, September 10-14, 2012, Hamburg Based on some chapters of the book ‘Supergravity’

  2. Wess, Zumino Supersymmetry and supergravity � supersymmetry δ = ε ψ A x x ( ) ( ) Bosons and fermions ∂ δ ψ = γ µ ε x A x ( ) ( ) in one multiplet µ ∂ x � commutator gives general � commutator gives general coordinate transformations ∂ µ = γ Q Q P δ ε δ ε = ε γ ε µ { , } or [ ( ), ( )] µ ∂ µ x 1 2 2 1 ⇒ gauge theory contains gravity: Supergravity Freedman, van Nieuwenhuizen, Ferrara

  3. 1. Scalar field theory and its symmetries: A. Poincaré group Algebra SO(1, D-1) η νρ m [ �σ ] − η �ρ m [ νσ ] [ m [ �ν ] , m [ ρσ ] ] = Space with ( x � ) = ( t, � x ) − η νσ m [ �ρ ] + η �σ m [ νρ ] Metric d s 2 = − d t d t + d � x = d x � η �ν d x ν Act on fields: φ (x)= φ ´ (x ´ ) Act on fields: φ (x)= φ ´ (x ´ ) = − d t d t + d � x � d � x � d � d s x = d x η �ν d x φ ′ ( x ) = U (Λ) φ ( x ) = φ (Λ x ) Isometries (preserve metric) e − 1 x � = Λ �ν x ′ ν + a � 2 λ ρσ L [ ρσ ] U (Λ) ≡ Λ �ρ η �ν Λ νσ = η ρσ ≡ x ρ ∂ σ − x σ ∂ ρ L [ ρσ ] Expand More general if not scalar fields Λ �ν δ �ν + λ �ν + O ( λ 2 ) = J [ ρσ ] = L [ ρσ ] + m [ ρσ ] , � � � 1 2 λ ρσ m [ ρσ ] = e ν ψ ′ i ( x ) = U (Λ , a ) ij ψ j ( x ) � � i �ν δ � ρ η νσ − δ � �ν m [ ρσ ] ≡ σ η ρν = − m [ σρ ] e − 1 2 λ ρσ m [ ρσ ] j ψ j (Λ x + a ) =

  4. B. Other symmetries and currents

  5. Exercises on chapter 1 � Ex 1.5: Show that the action � � � η �ν ∂ � φ i ∂ ν φ i + m 2 φ i φ i � d D x L ( x ) = − 1 d D x S = 2 is invariant under the transformation Λ → φ ′ ( x ) ≡ φ (Λ x ) . → φ ′ i ( x ) ≡ φ i (Λ x ) . φ i ( x ) φ ( x ) − − Important: fields transform, not the integration variables [ L [ �ν ] , L [ ρσ ] ] � Ex.1.6: Compute the commutators and show that they agree with that for matrix generators. Show that to first order in λ ρσ 2 λ ρσ L [ ρσ ] φ i ( x � ) = φ i ( x � + λ �ν x ν ) φ i ( x � ) − 1

  6. 2. The Dirac field

  7. Exercise on chapter 2 � Show using the fundamental relation of gamma matrices that [Σ �ν , γ ρ ] = 2 γ [ � η ν ] ρ = γ � η νρ − γ ν η �ρ � Prove the consistency of � Prove the consistency of 2 λ �ν � δ Ψ = − 1 Ψ = 1 2 λ �ν Σ �ν Ψ , δ � ΨΣ �ν � Prove then the invariance of the action � d D x � Ψ[ γ � ∂ � − m ]Ψ( x ) S [ � Ψ , Ψ] = −

  8. 3. Clifford algebras and spinors � Determines the properties of - the spinors in the theory - the supersymmetry algebra � We should know � We should know - how large are the smallest spinors in each dimension - what are the reality conditions - which bispinors are (anti)symmetric (can occur in superalgebra)

  9. 3.1 The Clifford algebra in general dimension 3.1.1 The generating � matrices Hermiticity γ � † � γ � γ � γ � (hermitian for spacelike ) (hermitian for spacelike ) Hermiticity representations related by conjugacy by unitary S γ ′ � � Sγ � S − �

  10. 3.1.2 The complete Clifford algebra γ � 1 ...� r = γ [ � 1 . . . γ � r ] , γ �ν = 1 2 γ � γ ν − 1 2 γ ν γ � e.g. 3.1.3 Levi-Civita symbol ε 012( D − 1) = − 1 ε 012( D − 1) = 1 , 3.1.4 Practical � -gamma matrix manipulation γ � γ � = D , γ �ν γ ν = ( D − 1) γ �

  11. 3.1.5 Basis of the algebra for even dimension D = 2 m { Γ A = , γ � , γ � 1 � 2 , γ � 1 � 2 � 3 , � � � , γ � 1 ��� � D } with � 1 < � 2 < ...< � r reverse order list { Γ A = { Γ = , γ � , γ � 2 � 1 , γ � 3 � 2 � 1 , . . . , γ � D ��� � 1 } . } . , γ , γ , γ , . . . , γ Tr(Γ A Γ B ) = 2 m δ A B expansion for any matrix in spinor space M � 1 m A Γ A , M = m A = 2 m Tr( M Γ A ) A

  12. 3.1.6 The highest rank Clifford algebra element

  13. 3.1.7 Odd spacetime dimension D=2m+1 � matrices dan be constructed in two ways from those in D=2m : γ � 1 ...� r The set with all is overcomplete

  14. 3.2 Supersymmetry and symmetry of bi-spinors (intro) � E.g. a supersymmetry on a scalar is a symmetry transformation depending on a spinor ε: � For the algebra we should obtain a GCT � For the algebra we should obtain a GCT ξ ξ µ ξ ξ µ µ µ � Then the GCT parameter should be antisymmetric in the spinor parameters Thus, to see what is possible, we have to know the symmetry properties of bi-spinors

  15. 3.2 Spinors in general dimensions 3.2.1 Spinors and spinor bilinears Majorana conjugate � with anticommuting spinors Since symmetries of spinor bilinears are important for supersymmetry, we use the Majorana conjugate to define λ .

  16. 3.2.2 Spinor indices NW-SE convention

  17. 3.2.4 Reality Complex conjugation can be replaced by charge conjugation, an operation that acts as complex conjugation on scalars, and has a simple action on fermion bilinears. For example, it preserves the order of spinor factors.

  18. 3.3 Majorana spinors � A priori a spinor ψ has 2 Int[ D /2] (complex) components � Using e.g. ‘left’ projection P L = (1+ γ * )/2 if D is even (otherwise trivial) ‘Weyl spinors’ P L ψ = ψ � In some dimensions (and signature) there are reality conditions ψ =ψ C = B −1 ψ * ψ =ψ C = B −1 ψ * consistent with Lorentz algebra: ‘Majorana spinors’ � consistency requires t 1 = -1.

  19. Other types of spinors � If t 1 =1: Majorana condition not consistent � Define other reality condition (for an even number of spinors): � ‘Symplectic Majorana spinors’ � In some dimensions Weyl and Majorana can be combined, e.g. reality condition for Weyl spinors: ‘Majorana-Weyl spinors’

  20. Dim Spinor min.# comp Possibilities for susy depend on the properties of irreducible spinors 2 MW 1 in each dimension 3 M 2 4 M 4 � Dependent on signature. 5 S 5 S 8 8 Here: Minkowski Here: Minkowski 6 SW 8 � M: Majorana MW: Majorana-Weyl 7 S 16 S: Symplectic 8 M 16 SW: Symplectic-Weyl 9 M 16 10 MW 16 11 M 32

  21. 3.4 Majorana OR Weyl fields in D=4 � Any field theory of a Majorana spinor field Ψ can be rewritten in terms of a Weyl field P L Ψ and its complex conjugate. � Conversely, any theory involving the chiral field � Conversely, any theory involving the chiral field χ =P L χ and its conjugate χ C =P R χ C can be rephrased as a Majorana equation if one defines the Majorana field Ψ =P L χ +P R χ C . � Supersymmetry theories in D=4 are formulated in both descriptions in the physics literature.

  22. Exercise on chapter 3 � Ex. 3.40: Rewrite � S [Ψ] = − 1 d D x � Ψ[ γ � ∂ � − m ]Ψ( x ) 2 as � � � � � ( P L + P R )Ψ � � S [ ψ ] = − 1 d 4 x Ψ γ � ∂ � − m − − 2 � � � � � � d 4 x Ψ γ � ∂ � P L Ψ − 1 Ψ P L Ψ − 1 � 2 m � 2 m � = − Ψ P R Ψ . and prove that the Euler-Lagrange equations are / / ∂P L Ψ = mP R Ψ , ∂P R Ψ = mP L Ψ . Derive � P L,R Ψ = m 2 P L,R Ψ from the equations above

  23. 4. The Maxwell and Yang-Mills Gauge Fields 4.1 The Abelian gauge field A � (x)

  24. 4.3 Non-abelian gauge symmetry � Simplest: act by matrices and � Gauge fields for any generator � � ∂ � + gt A A A D � Ψ = Ψ cov. derivative: � � ( x ) = 1 g∂ � θ A + θ C ( x ) A B needs transform: δA A � ( x ) f BCA δA � ( x ) = g∂ � θ + θ ( x ) A � ( x ) f BC [ D � , D ν ]Ψ = gF A �ν t A Ψ � Curvatures F A �ν = ∂ � A A ν − ∂ ν A A � + gf BCA A B � A C ν � Typical action � � S [ A A Ψ α , Ψ α ] = d D x − 1 4 F A�ν F A � , � �ν Ψ α ( γ � D � − m )Ψ α � − �

  25. Exercise on chapter 4 � Ex. 4.17: Use the Jacobi identity to show that the C t C and D satisfy [t A ,t B ]= f AB matrices (t A ) D E =f AE therefore give a representation � Ex 4.21: Show that � Ex 4.21: Show that D � F A νρ + D ν F A ρ� + D ρ F A �ν = 0 A is written in the form is satisfied identically if F � ν F A �ν = ∂ � A A ν − ∂ ν A A � + gf BCA A B � A C ν

  26. 6. N=1 Global supersymmetry in D=4 � Classical algebra

  27. 6.2. SUSY field theories of the chiral multiplet � Transformation under SUSY � Algebra � Simplest action � Potential term

  28. 6.2.2 The SUSY algebra • A transformation is a parameter times a generator • Calculating a commutator • Calculating a commutator bosonic

  29. Calculating the algebra � Very simple on Z � On fermions: more difficult; needs Fierz rearrangement � With auxiliary field: algebra satisfied for all field configurations Without auxiliary field: satisfied modulo field equations. Without auxiliary field: satisfied modulo field equations. � auxiliary fields lead to - transformations independent of e.g. the superpotential - algebra universal : ‘closed off-shell’ - useful in determining more general actions - in local SUSY: simplify couplings of ghosts

  30. 6.3. SUSY gauge theories 6.3.1 SUSY Yang-Mills vector multiplet gauge)

  31. 6.3.2 Chiral multiplets in SUSY gauge theories

Download Presentation
Download Policy: The content available on the website is offered to you 'AS IS' for your personal information and use only. It cannot be commercialized, licensed, or distributed on other websites without prior consent from the author. To download a presentation, simply click this link. If you encounter any difficulties during the download process, it's possible that the publisher has removed the file from their server.

Recommend


More recommend