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Quantum Electrodynamics (QED), Winter 2015/16 Fermions - Reference Dirac Algebra The Dirac algebra is introduced to define the 4-dimensional representation appropriate for fields carrying spin-1/2. {γ µ , γ ν } = γ µ γ ν + γ ν γ µ = 2 g µν 1 , where g µν is the Minkowski metric and 1 is the 4×4 identity for the matrix representation and ! ! i 0 1 0 σ γ0 = γi = 1 0 −σ i 0 with Pauli sigma matrices σ i . The 4-dimensional representation of the Lorentz group is given by S µν = generators ! 0 i σi 0i , S =− 2 0 −σ i i 4 [γ µ , γ ν ] with boost and rotation generators S ij 1 = − ijk 2 σk 0 0 σk ! 1 = ijk Σk . 2 Some useful identitiesand trace identities involving γ matrices are γ µ γµ = 41 , γ µ γ ν γµ = −2γ ν , γ µ γ ν γ ρ γµ = 4g νρ 1 , and Tr γ µ = 0 , Tr γ µ γ ν = 4g µν , Tr γ µ γ ν γ ρ = 0 Tr γ µ γ ν γ ρ γ σ = 4g µν g ρσ − 4g µρ g νσ + 4g µσ g νρ . Dirac Spinors ψ(x) is a 4-component field that transforms under S. To define Lorentz scalars involving ψ we have to introduce ψ̄(x) = ψ † γ 0 , such that ψ̄ψ transforms as a scalar. The simpler combination ψ † ψ does not transform as a Lorentz scalar (Lorentz boosts are not Hermitian in this representation). Lorentz vectors can be constructed as ψ̄γ µ ψ . 1 Quantum Electrodynamics (QED), Winter 2015/16 Fermions - Reference The bar notation will be generalised such that eg. Ō ≡ O† γ 0 . It is useful to keep track of spinor indices if you are not familiar with the spinor algebra so eg. µ z µ = ψ̄a γab ψb . Sometimes we will use this convention when highlighting the spinor indices in products - ie. a, b etc with no raising or lowering convention (they will appear up or down, wherever convenient). Having defined a scalar quantity we can define the Dirac action µ LD = ψ̄a (iγab ∂µ − m × 1ab )ψb , µ which is normally written simply as LD = ψ̄(i∂/ − m)ψ with notation ∂/ab = γab ∂µ . Varying with respect to ψ̄ we get the Dirac equation (i∂/ − m)ψ = 0 . The Dirac equation reduces to the Klein–Gordon equation if we consider just a scalar field (ie. field that carries only linear momentum). This indicates that the solution (in momentum frame) to the Dirac equation can be split into a plane wave part satisfying the Klein–Gordon equation and a second part that carries all the angular momentum information ψa (p) ∝ ua (p) e−i p·x . Considering the u(p) part of the solution we can obtain the properly normalised function ! √ s p · σ ξ us (p) = √ , p · σ̄ ξ s with s = 1, 2 labeling the two independent solutions. The general solution is then X ψ(p) = us (p) e−i p·x + v s (p) ei p·x , s with v s (p) = ! √ p · σ ηs , √ − p · σ̄ η s ie. positive and negative frequency (plane wave direction) modes under the assumption that both modes have positive energy p0 > 0. Here σ = (1, σ) and σ̄ = (1, −σ) with a useful identity being (p · σ)(p · σ̄) = p2 = m2 . The two component spinors ξ s and η s define a spin basis. For our purposes we can always consider them as eigenstates of eg. σ 3 such that eg. ! ! p p 1 0 E − p3 E − p3 0 1! 2 1 , ! u (p) = , u (p) = p p 1 0 E + p3 E + p3 0 1 2 Quantum Electrodynamics (QED), Winter 2015/16 Fermions - Reference are spin “up” and “down”. Orthonormal properties of the full solutions are given by ūr (p)us (p) = 2mδ rs , ur† (p)us (p) = 2Ep δ rs , v̄ r (p)v s (p) = −2mδ rs , v r† (p)v s (p) = 2Ep δ rs , ūr (p)v s (p) = v̄ r (p)us (p) = 0 . Completeness relations will be very useful X ξ s ξ s† = 1 , s X s u (p)ū(p)s = γ · p + m = p/ + m , s X v s (p)v̄(p)s = γ · p − m = p/ − m . s Quantisation Introduce ladder expansion, now we need to ladder operators for both modes Z i Xh d3 p 1 s s −i p·x s† s i p·x p ψ(x) = . a u (p) e + b v (p) e p p (2π)3 2 Ep s For fermions we must impose anti-commutations as the equal-time, canonical commutation relations. This will ensure the correct statistics and ensure consistency with microcausality with respect to commutations of operators o n {ψa (x), ψb (y)} = ψa† (x), ψb† (y) = 0 , n o ψa (x), ψb† (y) = δab δ (3) (x − y) , or, in terms of ladder operators, n o n o arp , as† = brp , bs† = (2π)3 δ rs δ (3) (p − q) , q q r s r s ap , aq = bp , bq = ... = 0 . The Hamiltonian density can be obtained by defining the momentum conjugate π= ∂LD = i ψ̄γ 0 = iψ † , ∂ ψ̇ which is not the velocity because the Lagrangian is first order in ψ. Then H = π ψ̇ − LD and we can write Z i Xh d3 p s† s s s† H= E a a − b b p p p p p , (2π)3 s Z i Xh d3 p s† s s† s 3 (3) = E a a + b b + (2π) δ (0) , p p p p p (2π)3 s 3 Quantum Electrodynamics (QED), Winter 2015/16 Fermions - Reference giving h i s† H, as† p = Ep a , etc.. The vacuum is then defined as asp |0i = bsp |0i = 0 and we can interpret as† p as creating a particle s† (positive frequency) with spin s, momentum p, and energy Ep and bp as creating an anti-particle (negative frequency) with spin s, momentum p, and energy Ep and bs† p. One particle and anti-particle states are labeled as eg. |p, s, −i = p 2Ep as† p |0i , |p, s, +i = p 2Ep bs† p |0i , and two particle states as |p, s, −; q, r, −i = p p r† 2Ep 2Eq as† p aq |0i , etc. Notice that under interchange of fermions the state is equal to the negative of itself giving rise to Fermi–Dirac statistics and the Pauli exclusion principle for the case where p = q and s = r. Feynman Propagator The propagator defined using the same choice of contours as the scalar case is (in momentum expansion) i(p/ + m) i = 2 . S F (p) = p/ − m + i p − m2 + i The first form is defines the Green’s functions of the Dirac equation and the second form can be obtained by inserting the completeness relation p/ +m in the numerator and using the identity {p, q} = 2 p · q in the denominator. The second form helps in keeping the matrix nature of the propagator implicit but you can always keep the explicit notation eg. F Sab (x − y) = h0| T ψa (x)ψ̄b (y) |0i . Note that time ordering is modified for fermions to account for the statistics ( h0| ψa (x)ψ̄b (y) |0i for x0 > y 0 , h0| T ψa (x)ψ̄b (y) |0i = − h0| ψ̄b (y)ψa (x) |0i for y 0 > x0 . This ensures that ψ(x), ψ̄(y) = 0 outside the light-cone when (x − y)2 < 0 4