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Component Multiplets and Closure Records

A component-field supermultiplet is not just a list of spins. Its specification includes the fields and their reality conditions, transformation laws, gauge equivalences, auxiliary variables, and the exact result of applying two transformations. The four-dimensional N=1\mathcal N=1 chiral multiplet closes off shell after adding one complex auxiliary scalar; the vector multiplet closes off shell modulo a gauge transformation. Eliminating the auxiliaries preserves the classical dynamics but generally changes the closure class to on shell.

Required background. The Four-Dimensional N=1 Super-Poincaré Algebra supplies the algebra and conjugation used below. Spinors, Conjugations, Bilinears, and Fierz Identities supplies the two-component identities needed to reduce the commutators.

Helpful background. Gauge Fields, Redundancy, and Observable Content explains why a gauge term is not a failure of the algebra on physical configurations.

Work in four-dimensional Lorentzian spacetime with the site metric (+−−−)(+---). Use

σαα˙μ=(1,σ),σˉμα˙α=(1,−σ),ϵ12=ϵ21=1.\sigma^\mu_{\alpha\dot\alpha} =(\mathbf1,\boldsymbol\sigma), \qquad \bar\sigma^{\mu\dot\alpha\alpha} =(\mathbf1,-\boldsymbol\sigma), \qquad \epsilon^{12}=\epsilon_{21}=1.

The translation generator is Pμ=i∂μP_\mu=i\partial_\mu, and

{Qα,Qˉα˙}=2σαα˙μPμ.\{Q_\alpha,\bar Q_{\dot\alpha}\} =2\sigma^\mu_{\alpha\dot\alpha}P_\mu.

All spinor derivatives and component calculations use left Grassmann differentiation. Define the even transformation

δϵ=ϵαQα+ϵˉα˙Qˉα˙,\delta_\epsilon=\epsilon^\alpha Q_\alpha +\bar\epsilon_{\dot\alpha}\bar Q^{\dot\alpha},

where ϵ\epsilon and ϵˉ\bar\epsilon are constant Grassmann-odd parameters related by Lorentzian conjugation. With

ξμ=2i(ϵ2σμϵˉ1−ϵ1σμϵˉ2),\xi^\mu =2i\left( \epsilon_2\sigma^\mu\bar\epsilon_1 -\epsilon_1\sigma^\mu\bar\epsilon_2 \right),

the target algebra on an ordinary nongauge field is

[δ1,δ2]φ=ξμ∂μφ.[\delta_1,\delta_2]\varphi=\xi^\mu\partial_\mu\varphi.

A reproducible component specification answers six questions for every field:

EntryRequired statement
Field spaceLorentz representation, statistics, engineering dimension, and reality
RedundancyGauge transformations or other equivalences
TransformationAll coefficients, signs, and conjugates
Auxiliary statusWhether a field is algebraic in a named action
ClosureTranslation, gauge term, constraint term, and equation-of-motion term separately
CountIndependent real components off shell and physical modes on shell

The field count is a diagnostic, not a proof. Equal bosonic and fermionic counts do not establish the transformation algebra.

The chiral multiplet closes without field equations

Section titled “The chiral multiplet closes without field equations”

Let (A,ψα,F)(A,\psi_\alpha,F) consist of a complex scalar, a left Weyl spinor, and a complex scalar auxiliary field. Their engineering dimensions for a canonical four-dimensional action are 11, 3/23/2, and 22. Choose

δA=2 ϵψ,δψα=i2 (σμϵˉ)α∂μA+2 ϵαF,δF=i2 ϵˉσˉμ∂μψ,\begin{aligned} \delta A &=\sqrt2\,\epsilon\psi,\\ \delta\psi_\alpha &=i\sqrt2\,(\sigma^\mu\bar\epsilon)_\alpha \partial_\mu A +\sqrt2\,\epsilon_\alpha F,\\ \delta F &=i\sqrt2\,\bar\epsilon\bar\sigma^\mu \partial_\mu\psi, \end{aligned}

together with the complex-conjugate rules. These are the component projections of a chiral superfield in the convention developed later in this chapter.

The scalar check is immediate:

[δ1,δ2]A=2i(ϵ2σμϵˉ1−ϵ1σμϵˉ2)∂μA+2(ϵ2ϵ1−ϵ1ϵ2)F=ξμ∂μA.\begin{aligned} [\delta_1,\delta_2]A &= 2i\left( \epsilon_2\sigma^\mu\bar\epsilon_1 -\epsilon_1\sigma^\mu\bar\epsilon_2 \right)\partial_\mu A\\ &\quad +2(\epsilon_2\epsilon_1-\epsilon_1\epsilon_2)F =\xi^\mu\partial_\mu A. \end{aligned}

The displayed ordering of odd parameters matters. Because the spinor metric is antisymmetric while the parameters themselves anticommute, the contraction of two Grassmann-odd Weyl spinors is symmetric: ϵ2ϵ1=ϵ1ϵ2\epsilon_2\epsilon_1=\epsilon_1\epsilon_2. The apparent FF term therefore cancels.

For the fermion, the variation of the derivative of AA and the variation of FF both produce derivatives of ψ\psi. The convention-sensitive identity needed below is

χβ(σμηˉ)α+χα(ηˉσˉμ)β=δαβ(χσμηˉ).\chi^\beta(\sigma^\mu\bar\eta)_\alpha +\chi_\alpha(\bar\eta\bar\sigma^\mu)^\beta =\delta_\alpha{}^\beta(\chi\sigma^\mu\bar\eta).

Here every bilinear is ordered with the unbarred odd spinor first. Keeping the two variation routes separate gives

[δ1,δ2]ψα=2i[(σμϵˉ2)αϵ1β−(σμϵˉ1)αϵ2β+ϵ2αϵˉ1α˙σˉμα˙β−ϵ1αϵˉ2α˙σˉμα˙β]∂μψβ.\begin{aligned} [\delta_1,\delta_2]\psi_\alpha =2i\Big[& (\sigma^\mu\bar\epsilon_2)_\alpha\epsilon_1{}^\beta -(\sigma^\mu\bar\epsilon_1)_\alpha\epsilon_2{}^\beta\\ &+\epsilon_{2\alpha}\bar\epsilon_{1\dot\alpha} \bar\sigma^{\mu\dot\alpha\beta} -\epsilon_{1\alpha}\bar\epsilon_{2\dot\alpha} \bar\sigma^{\mu\dot\alpha\beta} \Big]\partial_\mu\psi_\beta. \end{aligned}

The second row is precisely the contribution from δF\delta F. Before using the identity, move the unbarred parameter in the first row to the left; for example,

(σμϵˉ2)αϵ1β=−ϵ1β(σμϵˉ2)α.(\sigma^\mu\bar\epsilon_2)_\alpha\epsilon_1{}^\beta =-\epsilon_1{}^\beta(\sigma^\mu\bar\epsilon_2)_\alpha.

The four terms then group into two complete spinor matrices:

[δ1,δ2]ψα=2i{[ϵ2β(σμϵˉ1)α+ϵ2α(ϵˉ1σˉμ)β]−[ϵ1β(σμϵˉ2)α+ϵ1α(ϵˉ2σˉμ)β]}∂μψβ=2i(ϵ2σμϵˉ1−ϵ1σμϵˉ2)∂μψα=  ξμ∂μψα.\begin{aligned} [\delta_1,\delta_2]\psi_\alpha =2i\Big\{& \big[ \epsilon_2{}^\beta(\sigma^\mu\bar\epsilon_1)_\alpha +\epsilon_{2\alpha}(\bar\epsilon_1\bar\sigma^\mu)^\beta \big]\\ &- \big[ \epsilon_1{}^\beta(\sigma^\mu\bar\epsilon_2)_\alpha +\epsilon_{1\alpha}(\bar\epsilon_2\bar\sigma^\mu)^\beta \big] \Big\}\partial_\mu\psi_\beta\\ =2i\big(& \epsilon_2\sigma^\mu\bar\epsilon_1 -\epsilon_1\sigma^\mu\bar\epsilon_2 \big)\partial_\mu\psi_\alpha\\ =\;&\xi^\mu\partial_\mu\psi_\alpha. \end{aligned}

For the top component, applying δ1\delta_1 to δ2F\delta_2F and subtracting the reverse order gives

[δ1,δ2]F=  −2(ϵˉ2σˉμσνϵˉ1−ϵˉ1σˉμσνϵˉ2)∂μ∂νA+2i(ϵˉ2σˉμϵ1−ϵˉ1σˉμϵ2)∂μF.\begin{aligned} [\delta_1,\delta_2]F =\;&-2\Big( \bar\epsilon_2\bar\sigma^\mu\sigma^\nu\bar\epsilon_1 -\bar\epsilon_1\bar\sigma^\mu\sigma^\nu\bar\epsilon_2 \Big)\partial_\mu\partial_\nu A\\ &+2i\Big( \bar\epsilon_2\bar\sigma^\mu\epsilon_1 -\bar\epsilon_1\bar\sigma^\mu\epsilon_2 \Big)\partial_\mu F. \end{aligned}

Only the symmetric part of σˉμσν\bar\sigma^\mu\sigma^\nu survives against ∂μ∂ν\partial_\mu\partial_\nu. It is proportional to ημν\eta^{\mu\nu}, and its coefficient vanishes because the contraction of the two dotted odd spinors is symmetric. Finally,

ϵˉ2σˉμϵ1−ϵˉ1σˉμϵ2=ϵ2σμϵˉ1−ϵ1σμϵˉ2,\bar\epsilon_2\bar\sigma^\mu\epsilon_1 -\bar\epsilon_1\bar\sigma^\mu\epsilon_2 =\epsilon_2\sigma^\mu\bar\epsilon_1 -\epsilon_1\sigma^\mu\bar\epsilon_2,

so [δ1,δ2]F=ξμ∂μF[\delta_1,\delta_2]F=\xi^\mu\partial_\mu F.

No action or field equation has entered. This is exact off-shell closure. The independent real count is

2A+2F⏟4 bosonic=4ψ⏟4 fermionic.\underbrace{2_A+2_F}_{4\ {\rm bosonic}} = \underbrace{4_\psi}_{4\ {\rm fermionic}}.

The classic direct construction and its auxiliary completion are given in Weinberg 2000, § 26.1, pp. 55–59; the original four-dimensional multiplet construction appears in Wess and Zumino 1974, pp. 39–50.

Eliminating the auxiliary changes the closure class

Section titled “Eliminating the auxiliary changes the closure class”

For the free massless action, the algebraic field equation is F=0F=0. If one deletes FF and uses only

δA=2 ϵψ,δψα=i2(σμϵˉ)α∂μA,\delta A=\sqrt2\,\epsilon\psi, \qquad \delta\psi_\alpha =i\sqrt2(\sigma^\mu\bar\epsilon)_\alpha\partial_\mu A,

then the scalar still closes by translation. The fermion commutator is

[δ1,δ2]ψα=2i[(σμϵˉ2)αϵ1β−(σμϵˉ1)αϵ2β]∂μψβ.[\delta_1,\delta_2]\psi_\alpha = 2i\left[ (\sigma^\mu\bar\epsilon_2)_\alpha\epsilon_1{}^\beta -(\sigma^\mu\bar\epsilon_1)_\alpha\epsilon_2{}^\beta \right]\partial_\mu\psi_\beta.

Subtracting the translation and applying the same completeness identity gives the exact remainder

Rα=2i(ϵ1αϵˉ2α˙−ϵ2αϵˉ1α˙)σˉμα˙β∂μψβ.\mathcal R_\alpha =2i\left( \epsilon_{1\alpha}\bar\epsilon_{2\dot\alpha} -\epsilon_{2\alpha}\bar\epsilon_{1\dot\alpha} \right) \bar\sigma^{\mu\dot\alpha\beta} \partial_\mu\psi_\beta.

Thus Rα\mathcal R_\alpha is explicitly a parameter-dependent linear combination of

σˉμα˙β∂μψβ,\bar\sigma^{\mu\dot\alpha\beta}\partial_\mu\psi_\beta,

which is the free Weyl equation. Thus

[δ1,δ2]ψα=ξμ∂μψα+Rα,Rα=0only on shell.[\delta_1,\delta_2]\psi_\alpha =\xi^\mu\partial_\mu\psi_\alpha+\mathcal R_\alpha, \qquad \mathcal R_\alpha=0\quad\text{only on shell}.

For one chiral field with canonical Kähler metric, an interacting Wess–Zumino model replaces FF by −W′(A)‾-\overline{W'(A)} in this convention. With a nontrivial Kähler metric, its inverse and connection-dependent fermion terms enter the auxiliary equation. In either case, the corresponding remainder is proportional to the interacting fermion equation, not merely the free Weyl operator. Algebraic elimination therefore preserves the action-level theory while removing an off-shell representation on the reduced fields. Weinberg 2000, § 26.4, pp. 75–82 makes this distinction explicit.

For an Abelian vector multiplet in Wess–Zumino gauge, take a real gauge potential AμA_\mu, a Weyl gaugino λα\lambda_\alpha, and a real auxiliary scalar DD. Define

σμν=14(σμσˉν−σνσˉμ)\sigma^{\mu\nu} =\frac14\left( \sigma^\mu\bar\sigma^\nu-\sigma^\nu\bar\sigma^\mu \right)

and use

δAμ=iϵσμλˉ−iλσμϵˉ,δλα=(σμνϵ)αFμν+iϵαD,δD=−ϵσμ∂μλˉ−∂μλ σμϵˉ.\begin{aligned} \delta A_\mu &=i\epsilon\sigma_\mu\bar\lambda -i\lambda\sigma_\mu\bar\epsilon,\\ \delta\lambda_\alpha &=(\sigma^{\mu\nu}\epsilon)_\alpha F_{\mu\nu} +i\epsilon_\alpha D,\\ \delta D &=-\epsilon\sigma^\mu\partial_\mu\bar\lambda -\partial_\mu\lambda\,\sigma^\mu\bar\epsilon. \end{aligned}

The conjugate gaugino transformation needed below is

δλˉα˙=(σˉμνϵˉ)α˙Fμν−iϵˉα˙D,σˉμν:=14(σˉμσν−σˉνσμ).\delta\bar\lambda_{\dot\alpha} =(\bar\sigma^{\mu\nu}\bar\epsilon)_{\dot\alpha}F_{\mu\nu} -i\bar\epsilon_{\dot\alpha}D, \qquad \bar\sigma^{\mu\nu} :=\frac14\left( \bar\sigma^\mu\sigma^\nu-\bar\sigma^\nu\sigma^\mu \right).

The two routes through the gaugino commutator have distinct roles. The part obtained by varying FμνF_{\mu\nu} reduces by the three-sigma identities to

[δ1,δ2]F-routeλα=ξμ∂μλα−Δα(D),\big[\delta_1,\delta_2\big]_{F\text{-route}}\lambda_\alpha =\xi^\mu\partial_\mu\lambda_\alpha -\Delta^{(D)}_\alpha,

where the contribution from varying the explicit iϵDi\epsilon D term is

Δα(D):=iϵ2αδ1D−iϵ1αδ2D=  −iϵ2α(ϵ1σμ∂μλˉ+∂μλ σμϵˉ1)+iϵ1α(ϵ2σμ∂μλˉ+∂μλ σμϵˉ2).\begin{aligned} \Delta^{(D)}_\alpha :={}&i\epsilon_{2\alpha}\delta_1D -i\epsilon_{1\alpha}\delta_2D\\ =\;&-i\epsilon_{2\alpha}\Big( \epsilon_1\sigma^\mu\partial_\mu\bar\lambda +\partial_\mu\lambda\,\sigma^\mu\bar\epsilon_1 \Big)\\ &+i\epsilon_{1\alpha}\Big( \epsilon_2\sigma^\mu\partial_\mu\bar\lambda +\partial_\mu\lambda\,\sigma^\mu\bar\epsilon_2 \Big). \end{aligned}

The two pieces cancel without a gaugino equation, leaving [δ1,δ2]λα=ξμ∂μλα[\delta_1,\delta_2]\lambda_\alpha=\xi^\mu\partial_\mu\lambda_\alpha.

The calculation on DD separates just as cleanly. The part containing FρσF_{\rho\sigma} is

B:=[−ϵ2σμσˉρσϵˉ1−(σρσϵ1)σμϵˉ2+ϵ1σμσˉρσϵˉ2+(σρσϵ2)σμϵˉ1]∂μFρσ.\begin{aligned} \mathcal B:=\Big[& -\epsilon_2\sigma^\mu\bar\sigma^{\rho\sigma}\bar\epsilon_1 -(\sigma^{\rho\sigma}\epsilon_1)\sigma^\mu\bar\epsilon_2\\ &+\epsilon_1\sigma^\mu\bar\sigma^{\rho\sigma}\bar\epsilon_2 +(\sigma^{\rho\sigma}\epsilon_2)\sigma^\mu\bar\epsilon_1 \Big]\partial_\mu F_{\rho\sigma}. \end{aligned}

The metric terms in the three-sigma identities cancel pairwise, while the remaining totally antisymmetric term is proportional to ∂[μFρσ]\partial_{[\mu}F_{\rho\sigma]} and vanishes by the Bianchi identity. The variations of the iϵDi\epsilon D and −iϵˉD-i\bar\epsilon D terms supply ξμ∂μD\xi^\mu\partial_\mu D. Thus

[δ1,δ2]D=ξμ∂μDwithout a field equation.[\delta_1,\delta_2]D=\xi^\mu\partial_\mu D \qquad\text{without a field equation}.

On the connection,

[δ1,δ2]Aμ=ξνFνμ=ξν∂νAμ+∂μΩ,Ω=−ξνAν.\begin{aligned} [\delta_1,\delta_2]A_\mu &=\xi^\nu F_{\nu\mu}\\ &=\xi^\nu\partial_\nu A_\mu +\partial_\mu\Omega, \qquad \Omega=-\xi^\nu A_\nu. \end{aligned}

No equation of motion was used. The algebra closes off shell on the gauge-equivalence class and modulo an Abelian gauge transformation on a representative. The original vector multiplet and its auxiliary completion are exhibited in Wess and Zumino 1974, pp. 42–48; Weinberg 2000, §§ 27.2–27.3, pp. 122–131 gives the corresponding two-component construction.

For the non-Abelian extension, retain the site’s Hermitian-generator convention and place the gauge coupling in the connection:

Fμν:=∂μAν−∂νAμ−ig[Aμ,Aν],DμX:=∂μX−ig[Aμ,X],δΩAμ:=DμΩ.\begin{aligned} F_{\mu\nu} &:=\partial_\mu A_\nu-\partial_\nu A_\mu-ig[A_\mu,A_\nu],\\ D_\mu X&:=\partial_\mu X-ig[A_\mu,X],\\ \delta_\Omega A_\mu&:=D_\mu\Omega. \end{aligned}

Then

ξνFνμ=ξν∂νAμ+Dμ(−ξνAν),\xi^\nu F_{\nu\mu} =\xi^\nu\partial_\nu A_\mu +D_\mu(-\xi^\nu A_\nu),

so Ω=−ξνAν\Omega=-\xi^\nu A_\nu is Lie-algebra valued. This is a translation plus a field-dependent gauge transformation in the stated convention.

The off-shell count is

(4−1)Aμ+1D⏟4 bosonic=4λ⏟4 fermionic.\underbrace{(4-1)_{A_\mu}+1_D}_{4\ {\rm bosonic}} = \underbrace{4_\lambda}_{4\ {\rm fermionic}}.

This local count is made for a generic nonzero Fourier mode, equivalently at the level of the principal symbol: the subtraction by one is a local gauge function, not an on-shell polarization count. Global zero modes and boundary data require a separate count. After imposing the Maxwell equation and quotienting residual gauge transformations, the photon has two physical helicities; the on-shell Weyl gaugino also has two real physical modes.

For pure Abelian super-Yang–Mills theory, the auxiliary sector is LD=12D2\mathcal L_D=\tfrac12D^2, so the algebraic equation is D=0D=0. Deleting DD also deletes the iϵDi\epsilon D term in δλ\delta\lambda. The connection still closes modulo gauge, but the reduced gaugino transformation obeys

[δ1(0),δ2(0)]λα=ξμ∂μλα+Rα(D),Rα(D)=−Δα(D)=iϵ2α(ϵ1σμ∂μλˉ+∂μλ σμϵˉ1)−iϵ1α(ϵ2σμ∂μλˉ+∂μλ σμϵˉ2).\begin{aligned} [\delta^{(0)}_1,\delta^{(0)}_2]\lambda_\alpha &=\xi^\mu\partial_\mu\lambda_\alpha +\mathcal R^{(D)}_\alpha,\\ \mathcal R^{(D)}_\alpha &=-\Delta^{(D)}_\alpha\\ &=i\epsilon_{2\alpha}\Big( \epsilon_1\sigma^\mu\partial_\mu\bar\lambda +\partial_\mu\lambda\,\sigma^\mu\bar\epsilon_1 \Big)\\ &\quad-i\epsilon_{1\alpha}\Big( \epsilon_2\sigma^\mu\partial_\mu\bar\lambda +\partial_\mu\lambda\,\sigma^\mu\bar\epsilon_2 \Big). \end{aligned}

The remainder vanishes only after imposing the conjugate free Weyl equations σμ∂μλˉ=0\sigma^\mu\partial_\mu\bar\lambda=0 and (∂μλ)σμ=0(\partial_\mu\lambda)\sigma^\mu=0. Evaluating the already-closed full commutator at D=0D=0 would hide this change of representation, just as evaluating the full chiral commutator at F=0F=0 hides the reduced fermion remainder.

Wess–Zumino gauge requires a compensator

Section titled “Wess–Zumino gauge requires a compensator”

An unconstrained real vector superfield contains additional scalar and spinor components. A supergauge transformation removes them to reach Wess–Zumino gauge. A bare superspace translation generally regenerates the removed components, so the component transformation above is actually

δWZ=δSUSY+δsupergauge(Λcomp),\delta_{\rm WZ} =\delta_{\rm SUSY} +\delta_{\rm supergauge}(\Lambda_{\rm comp}),

where the compensating chiral parameter depends on the supersymmetry parameter and the fields. Consequently the commutator contains the ordinary gauge transformation displayed above. Saying that “supersymmetry does not close in Wess–Zumino gauge” is incomplete: it closes on the gauge orbit, and the compensator is part of the transformation law. The prepotential and compensator structure are developed in Gates, Grisaru, Roček, and Siegel 1983, §§ 3.9–3.10, pp. 108–119, and § 4.2, pp. 159–177.

Object being countedChiral exampleVector example
Covariant off-shell fieldsA,ψ,FA,\psi,FAμ,λ,DA_\mu,\lambda,D modulo gauge
Auxiliary variablesComplex FFReal DD
On-shell one-particle contentComplex scalar plus Weyl fermion, with CPT completion as requiredHelicity ±1\pm1 gauge boson plus helicity ±12\pm\tfrac12 gaugino
Closure statementExact before eliminating FF; on shell afterwardExact modulo gauge before eliminating DD; on shell modulo gauge afterward

Off-shell component equality concerns functions on spacetime before equations of motion. On-shell state equality concerns physical polarizations at fixed momentum. Gauge fixing, constraints, CPT completion, and auxiliary elimination affect the two counts differently.

A translation plus gauge is not failed closure. The gauge potential is not itself a gauge-invariant observable. The correct representation space is the space of connections modulo gauge transformations.

An algebraic field is not automatically auxiliary. “Auxiliary” refers to its role in a specified action and transformation system. A Lagrange multiplier, Stückelberg field, compensator, and gauge-removable component have different functions even when none propagates.

Degree matching is necessary, not sufficient. Incorrect transformation coefficients can preserve a 4=44=4 count while violating the commutator. Closure must be calculated field by field.

Using the chiral transformations, show explicitly that the two FF terms in [δ1,δ2]A[\delta_1,\delta_2]A cancel.

Solution

The relevant contribution is

2ϵ2αϵ1αF−2ϵ1αϵ2αF.2\epsilon_2^\alpha\epsilon_{1\alpha}F -2\epsilon_1^\alpha\epsilon_{2\alpha}F.

Moving the odd parameters to the same order shows that ϵ2ϵ1=ϵ1ϵ2\epsilon_2\epsilon_1=\epsilon_1\epsilon_2: the minus sign from exchanging the Grassmann-odd parameters cancels the minus sign from the antisymmetric spinor metric. The two FF terms are therefore equal and opposite. The derivative terms combine into ξμ∂μA\xi^\mu\partial_\mu A.

Starting from δF=i2 ϵˉσˉμ∂μψ\delta F=i\sqrt2\,\bar\epsilon\bar\sigma^\mu\partial_\mu\psi, identify separately the terms proportional to ∂μ∂νA\partial_\mu\partial_\nu A and ∂μF\partial_\mu F in [δ1,δ2]F[\delta_1,\delta_2]F.

Solution

The direct calculation gives

[δ1,δ2]F=  −2(ϵˉ2σˉμσνϵˉ1−ϵˉ1σˉμσνϵˉ2)∂μ∂νA+2i(ϵˉ2σˉμϵ1−ϵˉ1σˉμϵ2)∂μF.\begin{aligned} [\delta_1,\delta_2]F =\;&-2\Big( \bar\epsilon_2\bar\sigma^\mu\sigma^\nu\bar\epsilon_1 -\bar\epsilon_1\bar\sigma^\mu\sigma^\nu\bar\epsilon_2 \Big)\partial_\mu\partial_\nu A\\ &+2i\Big( \bar\epsilon_2\bar\sigma^\mu\epsilon_1 -\bar\epsilon_1\bar\sigma^\mu\epsilon_2 \Big)\partial_\mu F. \end{aligned}

The antisymmetric part of σˉμσν\bar\sigma^\mu\sigma^\nu is killed by the symmetric derivative, while the remaining dotted-spinor contraction cancels between the two orderings. Reordering the last line puts the unbarred parameters first and gives ξμ∂μF\xi^\mu\partial_\mu F. No field equation was used.

Rewrite ξνFνμ\xi^\nu F_{\nu\mu} as a translation plus an Abelian gauge transformation.

Solution

Because ξν\xi^\nu is constant,

ξνFνμ=ξν∂νAμ−ξν∂μAν=ξν∂νAμ+∂μ(−ξνAν).\xi^\nu F_{\nu\mu} =\xi^\nu\partial_\nu A_\mu -\xi^\nu\partial_\mu A_\nu =\xi^\nu\partial_\nu A_\mu +\partial_\mu(-\xi^\nu A_\nu).

Thus Ω=−ξνAν\Omega=-\xi^\nu A_\nu. No Maxwell equation occurs, so the result is off shell modulo gauge.

Why is setting F=0F=0 before computing the commutator different from computing the off-shell commutator and then evaluating it on the solution F=0F=0?

Solution

In the full multiplet, δF\delta F participates in the cancellation of terms in [δ1,δ2]ψ[\delta_1,\delta_2]\psi. If FF is deleted, that variation is unavailable and an equation-of-motion remainder remains. Evaluating the already-closed full commutator at F=0F=0 hides this loss of a transformation variable.

Set D=0D=0 in pure Abelian super-Yang–Mills theory and delete the iϵDi\epsilon D term from δλ\delta\lambda. Which part of the full commutator has been lost, and when does the reduced commutator close?

Solution

The lost route is

Δα(D)=iϵ2αδ1D−iϵ1αδ2D.\Delta^{(D)}_\alpha =i\epsilon_{2\alpha}\delta_1D -i\epsilon_{1\alpha}\delta_2D.

The FμνF_{\mu\nu} route by itself therefore gives

[δ1(0),δ2(0)]λα=ξμ∂μλα−Δα(D).[\delta^{(0)}_1,\delta^{(0)}_2]\lambda_\alpha =\xi^\mu\partial_\mu\lambda_\alpha-\Delta^{(D)}_\alpha.

Substituting the full transformation of DD shows that −Δα(D)-\Delta^{(D)}_\alpha is a parameter-dependent linear combination of σμ∂μλˉ\sigma^\mu\partial_\mu\bar\lambda and (∂μλ)σμ(\partial_\mu\lambda)\sigma^\mu. It vanishes only on the free gaugino equations and their conjugates. Thus the reduced vector system closes on shell modulo gauge, even though the full (Aμ,λ,D)(A_\mu,\lambda,D) system closes off shell modulo gauge.

Superspace and Supertranslations packages these transformations as geometry. Superfield constraints and closure comparison organizes the same multiplets by constraint, gauge equivalence, component content, and closure class. The off-shell auxiliary closure map then compares the counting and elimination logic, including the limitations for extended supersymmetry.

  • Gates, S. James, Jr., Marcus T. Grisaru, Martin Roček, and Warren Siegel. Superspace, or One Thousand and One Lessons in Supersymmetry. Frontiers in Physics 58. Reading, MA: Benjamin/Cummings, 1983. Corrected open edition, 2001. arXiv:hep-th/0108200.

  • Weinberg, Steven. The Quantum Theory of Fields. Volume III: Supersymmetry. Cambridge: Cambridge University Press, 2000, §§ 26.1–26.4. DOI.

  • Wess, Julius, and Bruno Zumino. “Supergauge Transformations in Four Dimensions.” Nuclear Physics B 70 (1974): 39–50. DOI. CERN record.

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