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Off-shell N=1 supersymmetry of the Wess–Zumino sigma-model action

Physical scope

Conditional classical supersymmetry and off-shell closure for the adopted rigid N=1 chiral sigma-model action on flat four-dimensional Minkowski spacetime, for smooth compactly supported component fields and the stated Kähler patch. No gauge, supergravity, quantum, continuum-limit, or empirical conclusion is asserted.

Statement

Use the rigid N=1 Wess–Zumino sigma-model postulate on M=R1,3 with η=diag⁡(−1,1,1,1), Kähler coordinate patch U⊆Cn, smooth positive metric gijˉ=∂i∂jˉK, holomorphic superpotential W, and full formal components ai,Fi:M→G0ˉ and ψαi:M→G1ˉ with coefficientwise compact support on M, using the involution and parameter conventions of the postulate. The scalar body lies in U. For external parameters in the finite exterior algebra E of the chiral-superfield convention, embed the component algebra into Gϵ=G⊗^E by a↦a⊗1 and interpret variations in that graded scalar extension, with total parity and the induced order-reversing involution. All formulas and the finite Taylor action extend coefficientwise to this algebra. Under the global supersymmetry variation δΦi=(ϵαQα+ϵˉα˙Qˉα˙)Φi with constant Grassmann-odd parameters and the fixed chiral-superfield supercharges, the variation of the adopted superspace Lagrangian is a spacetime divergence; consequently δSWZ=0. The supercharges satisfy {Qα,Qβ}=0, {Qˉα˙,Qˉβ˙}=0, and {Qα,Qˉβ˙}=2iσαβ˙μ∂μ. Their induced transformations on the scalar, Weyl-fermion, and auxiliary components close on translations without using equations of motion, with the auxiliary fields retained.

Facts & Assumptions

Given: The adopted action, Kähler patch, holomorphic superpotential, and compactly supported component fields from the Statement.

[A1]

Rigid four-dimensional N=1 Wess–Zumino sigma-model action: SWZ=∫d4x{[K(Φˉ,Φ)]D+[W(Φ)]F+h.c.} with physical brackets [U]D=−ID(U)/4, [Y]F=IF(Y)/2, and Hermitian conjugation only on the F action; the full components are smooth coefficient maps with compact support on spacetime, and the explicitly defined involution reverses products; the supersymmetry parameters are constant and odd, with the conjugation-compatible real convention as specified there.

[F1]

Four-dimensional N=1 chiral superfield on flat superspace: a chiral superfield is a smooth element of C∞(R1,3,A⊗Λ4) with unique component expansion in the nilpotently shifted coordinate y=x+iθσθˉ; Qα=∂θαL−iσαβ˙μθˉβ˙∂μ and Qˉα˙=−∂θˉα˙L+iθβσβα˙μ∂μ.

[F2]

Chiral-coordinate solution and supersymmetry covariance: the chiral constraint is Dˉα˙Φ=0; in (y,θ,θˉ) coordinates this is independence of θˉ, and the supercharges anticommute with Dˉ, so the supersymmetry variation preserves chirality.

[F3]

Four-dimensional N=1 superspace Grassmann algebra and Berezin integration: the four ordered odd generators form a finite basis, left derivatives obey the odd Leibniz rule, and the ordered Berezin measures extract the corresponding top coefficients.

Proof

Given: [A1] and the superfield, differential-operator, and Berezin conventions in [F1]–[F3].

1.1A1F1F3algebra

For any even smooth superspace function X, substitute the operators from [F1] into δX. Since the odd parameters are constant, the odd Leibniz rule gives ϵα∂θαLX=−∂θαL(ϵαX) and −ϵˉα˙∂θˉα˙LX=∂θˉα˙L(ϵˉα˙X). The remaining terms are ordinary spacetime derivatives, so δX=−∂θαL(ϵαX)+∂θˉα˙L(ϵˉα˙X)+∂μ(−iϵασαβ˙μθˉβ˙X+iϵˉα˙θβσβα˙μX).

1.2F1F2F3algebra

For a chiral superfield X(y,θ), use y=x+iθσθˉ and the left-derivative rules in [F1]–[F3]. The chain rule gives Qα=∂θαL∣y and Qˉα˙=−∂θˉα˙L∣y+2iθβσβα˙μ∂yμ. Since X is independent of θˉ, δX=ϵα∂θαLX+2iϵˉα˙θβσβα˙μ∂μX.

1.3F1F3algebra

Expand the supercharge anticommutators from [F1]. The only nonzero terms in {Qα,Qˉβ˙} are {∂θαL,iθγσγβ˙μ∂μ}=iσαβ˙μ∂μ and {−iσαγ˙μθˉγ˙∂μ,−∂θˉβ˙L}=iσαβ˙μ∂μ. Terms with two odd coordinates cancel under symmetrization, and derivatives in distinct generators anticommute by [F3]. Hence {Qα,Qˉβ˙}=2iσαβ˙μ∂μ and both same-chirality anticommutators are zero.

2.1A1F3step 1.1

Apply step 1.1 to the even D-term integrand X=K(Φˉ,Φ), whose finite nilpotent Taylor expansion is smooth. Each odd-coordinate derivative has zero top coefficient in the ordered Grassmann basis from [F3], so its Berezin integral vanishes. The spacetime-divergence term integrates to zero because the field-dependent part of K is compactly supported and its constant exterior value has zero supersymmetry variation. The fixed physical factor −1/4 multiplies zero, so the D-term action is invariant.

3.1A1F1F2F3step 1.2algebra

The first term in step 1.2 integrates to zero under d2θ by the same coefficient-extraction calculation as step 2.1. The second is the spacetime divergence ∂μ(2iϵˉα˙θβσβα˙μX); compact support removes its boundary term. For the finite Taylor extension in the postulate, holomorphicity ∂iˉW=0 and the odd derivation rule give the chain identity Dˉα˙W(Φ)=∑iWi(Φ)Dˉα˙Φi=0, because each Φi is chiral; hence W(Φ) is chiral. Complex conjugation gives the corresponding antichirality of its conjugate. The fixed physical factor 1/2 and its conjugate preserve this zero variation, so the F-term action is invariant.

4.1F1F2step 1.3∎

Work in Gϵ for one variation, and adjoin a second independent exterior parameter copy for commutators of two variations. The operators extend by the graded derivative rule and annihilate the coefficient algebra, exactly as in [F1]. By [F2], the transformations preserve the chiral constraint, so the transformed field has the unique component expansion in [F1]. Coefficient extraction is linear; therefore the operator identities in step 1.3 induce the same translation algebra on every full formal component, including the independent even auxiliary coefficient Fi. Products of odd parameters and odd component maps lie in the total even subspace (Gϵ)0ˉ, while fermionic variations lie in its total odd subspace, and derivatives preserve coefficientwise compact support; thus this argument does not restrict the auxiliary coefficient to C or assert closure on the bosonic slice. No Euler–Lagrange equation was used, proving off-shell closure.

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