Docsity
Docsity

Prepare for your exams
Prepare for your exams

Study with the several resources on Docsity


Earn points to download
Earn points to download

Earn points by helping other students or get them with a premium plan


Guidelines and tips
Guidelines and tips

Quantum Field Theory - Assignment 7 Solutions | PHY 396K, Assignments of Physics

Material Type: Assignment; Class: QUANTUM FIELD THEORY I; Subject: Physics; University: University of Texas - Austin; Term: Unknown 2003;

Typology: Assignments

Pre 2010

Uploaded on 08/30/2009

koofers-user-g5d
koofers-user-g5d 🇺🇸

10 documents

1 / 7

Toggle sidebar

Related documents


Partial preview of the text

Download Quantum Field Theory - Assignment 7 Solutions | PHY 396K and more Assignments Physics in PDF only on Docsity! PHY–396 K. Solutions for problem set #7. Problem 1(a): γµγν = ±γνγµ where the sign is ‘+’ for µ = ν and ‘−’ otherwise. Hence for any product Γ of the γ matrices, γµΓ = (−1)nµΓγµ where nµ is the number of γ ν 6=µ factors of Γ. For Γ = γ5 ≡ iγ0γ1γ2γ3, nµ = 3 for any µ = 0, 1, 2, 3; thus γ µγ5 = −γ5γµ. Problem 1(b): First, ( γ5 ≡ iγ0γ1γ2γ3 )† = −i(γ3)†(γ2)†(γ1)†(γ0)† = +iγ3γ2γ1γ0 = +i((γ3γ2)γ1)γ0 = (−1)3i γ0((γ3γ2)γ1) = (−1)3+2i γ0(γ1(γ3γ2)) = (−1)3+2+1i γ0(γ1(γ2γ3)) = +iγ0γ1γ2γ3 ≡ +γ5. (S.1) Second, (γ5)2 = γ5(γ5)† = (iγ0γ1γ2γ3)(iγ3γ2γ1γ0) = −γ0γ1γ2(γ3γ3)γ2γ1γ0 = +γ0γ1(γ2γ2)γ1γ0 = −γ0(γ1γ1)γ0 = +γ0γ0 = +1. (S.2) Problem 1(c): Any four distinct γκ, γλ, γµ, γν are γ0, γ1, γ2, γ3 in some order. They all anticommute with each other, hence γκγλγµγν = ²κλµνγ0γ1γ2γ3 ≡ −i²κλµνγ5. The rest is obvious. Problem 1(d): i²κλµν γκγ 5 = γκ γ [κγλγµγν] = 14 γκ ( γκγ[λγµγν] − γ[λ)γκγ(µγν] + γ[λγµ)γκγ(ν] − γ[λγµγν]γκ ) = 14 ( 4γ[λγµγν] + 2γ[λγµγν] + 4g[λµγν] + 2γ[νγµγλ] ) = 14(4 + 2 + 0− 2)γ [λγµγν] = γ[λγµγν]. (S.3) 1 Problem 1(e): Proof by inspection: In the Weyl basis, the 16 matrices are 1 = ( 1 0 0 1 ) , γµ = ( 0 σµ σ̄µ 0 ) , γ[µγν] = ( σ[µσ̄ν] 0 0 σ̄[µσν] ) , γ5γµ = ( 0 −σµ σ̄µ 0 ) , γ5 = ( −1 0 0 +1 ) , (S.4) and their linear independence is self-evident. Since there are only 16 independent 4× 4 matrices altogether, any such matrix Γ is a linear combination of the matrices (S.4). Q.E .D. Algebraic Proof: Without making any assumption about the matrix form of the γµ operators, let us consider the Clifford algebra γµγν+γνγµ = 2gµν . Because of these anticommutation relations, one may re-order any product of the γ’s as ±γ0 · · · γ0 γ1 · · · γ1 γ2 · · · γ2 γ3 · · · γ3 and then further simplify it to ±(γ0 or 1) × (γ1 or 1) × (γ2 or 1) × (γ3 or 1). The net result is (up to a sign or ±i factor) one of the 16 operators 1, γµ, γ[µγν], γ5γµ (cf. (d)) or γ5 (cf. (c)). Consequently, any operator Γ algebraically constructed of the γµ’s is a linear combination of these 16 operators. Incidentally, the algebraic argument explains why the γµ (and hence all their products) should be realized as 4 × 4 matrices since any lesser matrix size would not accommodate 16 independent products. That is, the γ’s are 4× 4 matrices in four spacetime dimensions; different dimensions call for different matrix sizes. Specifically, in spacetimes of even dimensions d, there are 2d independent products of the γ operators, so we need matrices of size 2d/2 × 2d/2: 2× 2 in two dimensions, 4× 4 in four, 8× 8 in six, 16× 16 in eight, 32× 32 in ten, etc.,etc.. In odd dimensions, there are only 2d−1 independent operators because γd+1 ≡ (i)γ0γ1 · · · γd−1 — the analogue of the γ5 operator in 4d — commutes rather than anticommutes with all the γµ and hence with the whole algebra. Consequently, one has two distinct representations of the Clifford algebra — one with γd+1 = +1 and one with γd+1 = −1 — but in each repre- sentation there are only 2d−1 independent operator products, which call for the matrix size of 2(d−1)/2 × 2(d−1)/2. For example, in three spacetime dimensions (two space, one time), can take (γ0, γ1, γ2) = (σ3, iσ1, iσ2) for γ 4 ≡ iγ0γ1γ2 = +1 or (γ0, γ1, γ2) = (σ3, iσ1,−iσ2) for γ 4 = −1, but in both cases we have 2× 2 matrices. Problem 1(f): Under a continuous Lorentz symmetry x 7→ x′ = Lx, the Dirac spinor field and its conjugate 2 Problem 4(a): The overall statistics of the operator product B̂Ĉ corresponds to (−1)A(BC) = (−1)AB(−1)AC . Therefore, [Â, B̂Ĉ} def = ÂB̂Ĉ − (−1)AB(−1)ACB̂Ĉ = ( ÂB̂ − (−1)ABB̂ ) Ĉ + (−1)ABB̂ ( ÂĈ − (−1)ACĈ ) = [Â, B̂}Ĉ + (−1)ABB̂[Â, Ĉ}. (S.13) Likewise, [ÂB̂, Ĉ} = ÂB̂Ĉ − (−1)AC(−1)BCĈÂB̂ =  ( B̂Ĉ − (−1)BCĈB̂ ) + (−1)BC ( ÂĈ − (−1)ACĈ ) B̂ = Â[B̂, Ĉ} + (−1)BC [Â, Ĉ}B̂. (S.14) Problem 4(b): [ÂB̂, ĈD̂} = Â[B̂, ĈD̂} + (−1)BC(−1)BD[Â, ĈD̂}B̂ = Â[B̂, Ĉ}D̂ + (−1)BCÂĈ[B̂, D̂} + (−1)BC(−1)BD[Â, Ĉ}D̂B̂ + (−1)AC(−1)BC(−1)BDĈ[Â, D̂}B̂. (S.15) Problem 4(c): (−1)CA[Â, [B̂, Ĉ}} = (−1)CAÂB̂Ĉ − (−1)BC(−1)CAÂĈB̂ − (−1)ABB̂Ĉ + (−1)AB(−1)BCĈB̂Â, (−1)BC [Ĉ, [Â, B̂}} = (−1)BCĈÂB̂ − (−1)AB(−1)BCĈB̂ − (−1)CAÂB̂Ĉ + (−1)CA(−1)ABB̂ÂĈ, (−1)AB[B̂, [Ĉ, Â}} = (−1)ABB̂Ĉ − (−1)CA(−1)ABB̂ÂĈ − (−1)BCĈÂB̂ + (−1)BC(−1)CAÂĈB̂. (S.16) Upon adding these three equations together, their right hand sides cancel out while the left hand sides add up to the Jacobi identity (4). 5 Problem 5(a): Using the Leibniz rules (S.13) and (S.14) and the anticommutation relations (6), the calculation is straightforward. [â†αâβ, â † γ ] = δβγ â † α , [â†αâβ, âδ] = −δαδ âβ , [â†αâβ, â † γ âδ] = δβγ â † αâδ − δαδ â † γ âβ . (S.17) Problem 5(b): According to eq. (S.17), the commutator [â†αâβ, â † γ âδ] has exactly the same form as its bosonic counterpart. Hence, the proof of [Â, B̂] = Ĉ proceeds exactly as in the bosonic case, cf. homework set #2 (problem 3(b)). Problem 5(c): Using the Leibniz rules and eqs. (S.17), [↵âν , â † αâ † β âγ âδ] = δναâ † µâ † β âγ âδ + δνβ â † µâ † αâγ âδ − δµγ â † αâ † β âν âδ − δµδâ † αâ † β âγ âν . (S.18) Problem 5(d): Again, we have a fermionic analogue to the bosonic second-quantized operators we studied in homework set #3 (problem 1(d)). Given eqs. (7) and (S.18) (in which we exchange γ ↔ δ), we have [ Â, â†αâ † β âδâγ ] = ∑ µ,ν 〈µ| Â1 |ν〉 [ ↵âν , â † αâ † β âδâγ ] = ∑ µ 〈µ| Â1 |α〉 â † µâ † β âδâγ + ∑ µ 〈µ| Â1 |β〉 â † αâ † µâδâγ − ∑ ν 〈δ| Â1 |ν〉 â † αâ † β âν âγ − ∑ ν 〈γ| Â1 |ν〉 â † αâ † β âδâν (S.19) 6 and consequently, in light of eq. (8), [ Â, B̂ ] = ∑ α,β,γ,δ 〈α⊗ β| B̂2 |γ ⊗ δ〉 [∑ µ 〈µ| Â1 |α〉 â † µâ † β âδâγ + ∑ µ 〈µ| Â1 |β〉 â † αâ † µâδâγ − ∑ ν 〈δ| Â1 |ν〉 â † αâ † β âν âγ − ∑ ν 〈γ| Â1 |ν〉 â † αâ † β âδâν ] = ∑ µ,β,γ,δ 〈µ⊗ β| Â1(1 st)B̂2 |γ ⊗ δ〉 â † µâ † β âδâγ + ∑ α,µ,γ,δ 〈α⊗ µ| Â1(2 nd)B̂2 |γ ⊗ δ〉 â † αâ † µâδâγ − ∑ α,β,γ,ν 〈α⊗ β| B̂2Â1(2 nd) |γ ⊗ ν〉 â†αâ † β âν âγ − ∑ α,β,ν,δ 〈α⊗ β| B̂2Â1(1 st) |ν ⊗ δ〉 â†αâ † β âδâν 〈〈renaming indices〉〉 = ∑ α,β,γ,δ 〈α⊗ β| [( A1(1 st) + A1(2 nd) ) , B̂2 ] |γ ⊗ δ〉 × â†αâ † β âδâγ = ∑ α,β,γ,δ 〈α⊗ β| Ĉ2 |γ ⊗ δ〉 × â † αâ † β âδâγ ≡ Ĉ. Q. E . D. 7
Docsity logo



Copyright © 2024 Ladybird Srl - Via Leonardo da Vinci 16, 10126, Torino, Italy - VAT 10816460017 - All rights reserved