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Supercovariant Derivatives, Chirality, and Integrability

Supercovariant derivatives are the fermionic differential operators that commute in the graded sense with supertranslations. Their relative signs are fixed, not guessed: they are the right-invariant partners of the differential supercharges. A constraint built from them is supersymmetry invariant, but it defines a consistent multiplet only when its derivative distribution is integrable. In flat four-dimensional N=1\mathcal N=1 superspace, Dˉα˙Φ=0\bar D_{\dot\alpha}\Phi=0 is integrable and its general solution is an unconstrained function of (yμ,θα)(y^\mu,\theta^\alpha).

Required background. Superspace and Supertranslations derives the differential supercharges and chiral coordinates. Graded Algebra, Grassmann Variables, and Berezin Integration supplies the left-derivative rules used below.

Helpful background. Spinors, Conjugations, Bilinears, and Fierz Identities supplies the index identities needed for component projection.

Retain

Qα=∂α−iσαα˙μθˉα˙∂μ,Qˉα˙=−∂ˉα˙+iθασαα˙μ∂μ.\begin{aligned} Q_\alpha &=\partial_\alpha -i\sigma^\mu_{\alpha\dot\alpha} \bar\theta^{\dot\alpha}\partial_\mu,\\ \bar Q_{\dot\alpha} &=-\bar\partial_{\dot\alpha} +i\theta^\alpha\sigma^\mu_{\alpha\dot\alpha}\partial_\mu. \end{aligned}

Spinor indices are raised and lowered with ϵ12=ϵ21=1\epsilon^{12}=\epsilon_{21}=1. Thus Dα=ϵαβDβD^\alpha=\epsilon^{\alpha\beta}D_\beta and Dˉα˙=ϵα˙β˙Dˉβ˙\bar D^{\dot\alpha}=\epsilon^{\dot\alpha\dot\beta} \bar D_{\dot\beta}. The ordered quadratic operators used throughout this chapter are

D2≡DαDα,Dˉ2≡Dˉα˙Dˉα˙.D^2\equiv D^\alpha D_\alpha, \qquad \bar D^2\equiv \bar D_{\dot\alpha}\bar D^{\dot\alpha}.

The opposite-looking index order in the barred definition is deliberate: Lorentzian conjugation reverses the order of odd operators. With θθ=θαθα\theta\theta=\theta^\alpha\theta_\alpha and θˉθˉ=θˉα˙θˉα˙\bar\theta\bar\theta= \bar\theta_{\dot\alpha}\bar\theta^{\dot\alpha}, these definitions give

D2(θθ)=−4,Dˉ2(θˉθˉ)=−4D^2(\theta\theta)=-4, \qquad \bar D^2(\bar\theta\bar\theta)=-4

at the origin of odd coordinates.

Seek a first-order odd operator with the same leading coordinate derivative as QαQ_\alpha,

Dα=∂α+c iσαα˙μθˉα˙∂μ.D_\alpha =\partial_\alpha +c\,i\sigma^\mu_{\alpha\dot\alpha} \bar\theta^{\dot\alpha}\partial_\mu.

Let U\mathscr U be a homogeneous test superfield. Only the two cross terms in the anticommutator can be independent of θ\theta and θˉ\bar\theta:

{Dα,Qˉβ˙}U={∂α,iθγσγβ˙μ∂μ}U+{c iσαγ˙μθˉγ˙∂μ,−∂ˉβ˙}U=i(1−c)σαβ˙μ∂μU.\begin{aligned} \{D_\alpha,\bar Q_{\dot\beta}\}\mathscr U &= \left\{\partial_\alpha, i\theta^\gamma\sigma^\mu_{\gamma\dot\beta} \partial_\mu\right\}\mathscr U\\ &\quad+ \left\{c\,i\sigma^\mu_{\alpha\dot\gamma} \bar\theta^{\dot\gamma}\partial_\mu, -\bar\partial_{\dot\beta}\right\}\mathscr U\\ &=i(1-c)\sigma^\mu_{\alpha\dot\beta} \partial_\mu\mathscr U. \end{aligned}

The left-derivative Leibniz rule fixes the relative minus sign in the second line. Requiring the anticommutator to vanish for every U\mathscr U gives c=+1c=+1. Lorentzian conjugation then gives

Dα=∂∂θα+iσαα˙μθˉα˙∂μ,Dˉα˙=−∂∂θˉα˙−iθασαα˙μ∂μ.\begin{aligned} D_\alpha &= \frac{\partial}{\partial\theta^\alpha} +i\sigma^\mu_{\alpha\dot\alpha} \bar\theta^{\dot\alpha}\partial_\mu,\\ \bar D_{\dot\alpha} &= -\frac{\partial}{\partial\bar\theta^{\dot\alpha}} -i\theta^\alpha\sigma^\mu_{\alpha\dot\alpha}\partial_\mu. \end{aligned}

The same test-field calculation fixes the sign of the derivative algebra rather than importing it. For the mixed anticommutator,

{Dα,Dˉβ˙}U={∂α,−iθγσγβ˙μ∂μ}U+{iσαγ˙μθˉγ˙∂μ,−∂ˉβ˙}U=−2iσαβ˙μ∂μU.\begin{aligned} \{D_\alpha,\bar D_{\dot\beta}\}\mathscr U &= \left\{\partial_\alpha, -i\theta^\gamma\sigma^\mu_{\gamma\dot\beta} \partial_\mu\right\}\mathscr U\\ &\quad+ \left\{i\sigma^\mu_{\alpha\dot\gamma} \bar\theta^{\dot\gamma}\partial_\mu, -\bar\partial_{\dot\beta}\right\}\mathscr U\\ &=-2i\sigma^\mu_{\alpha\dot\beta} \partial_\mu\mathscr U. \end{aligned}

Terms with two coordinate factors cancel by Grassmann antisymmetry and commuting spacetime derivatives. The same-chirality cross terms vanish, so the complete derivative algebra is

{Dα,Dβ}=0,{Dˉα˙,Dˉβ˙}=0,{Dα,Dˉβ˙}=−2iσαβ˙μ∂μ.\begin{aligned} \{D_\alpha,D_\beta\}&=0, & \{\bar D_{\dot\alpha},\bar D_{\dot\beta}\}&=0,\\ \{D_\alpha,\bar D_{\dot\beta}\} &=-2i\sigma^\mu_{\alpha\dot\beta}\partial_\mu. \end{aligned}

Moreover,

{Dα,Qβ}=0,{Dα,Qˉβ˙}=0,{Dˉα˙,Qβ}=0,{Dˉα˙,Qˉβ˙}=0.\begin{aligned} \{D_\alpha,Q_\beta\}&=0, & \{D_\alpha,\bar Q_{\dot\beta}\}&=0,\\ \{\bar D_{\dot\alpha},Q_\beta\}&=0, & \{\bar D_{\dot\alpha},\bar Q_{\dot\beta}\}&=0. \end{aligned}

The DD algebra differs from the QQ algebra only in the mixed sign because it comes from the opposite group action. Gates, Grisaru, Roček, and Siegel 1983, § 3.4, pp. 83–88 develops this left/right-invariant construction.

Two useful consequences are

DαDβ=12ϵαβD2,Dˉα˙Dˉβ˙=−12ϵα˙β˙Dˉ2,D_\alpha D_\beta =\frac12\epsilon_{\alpha\beta}D^2, \qquad \bar D_{\dot\alpha}\bar D_{\dot\beta} =-\frac12\epsilon_{\dot\alpha\dot\beta}\bar D^2,

The relative minus sign follows from the declared order of Dˉ2\bar D^2; it is not optional shorthand. This is the same convention package used by

F=−14D2Φ∣,F∗=−14Dˉ2Φˉ∣,Wα=−14Dˉ2DαV.F=-\frac14D^2\Phi|, \qquad F^*=-\frac14\bar D^2\bar\Phi|, \qquad W_\alpha=-\frac14\bar D^2D_\alpha V.

Reversing the order in the definition of Dˉ2\bar D^2 flips the dotted reduction identity and must also flip every antichiral projector and field-strength formula derived from it.

The component-constraint atlas places these operators in the full path from supertranslations to constraints, gauge equivalences, and component fields.

Chirality is an integrable differential constraint

Section titled “Chirality is an integrable differential constraint”

A chiral scalar superfield obeys

Dˉα˙Φ=0.\bar D_{\dot\alpha}\Phi=0.

Applying a supersymmetry transformation preserves the constraint:

Dˉα˙δϵΦ=δϵ(Dˉα˙Φ)=0,\bar D_{\dot\alpha}\delta_\epsilon\Phi =\delta_\epsilon(\bar D_{\dot\alpha}\Phi)=0,

because the odd parameter contributes a second minus sign when Dˉ\bar D is moved through δϵ=ϵQ+ϵˉQˉ\delta_\epsilon=\epsilon Q+\bar\epsilon\bar Q: the even transformation δϵ\delta_\epsilon commutes with Dˉ\bar D. Compatibility between the two barred equations requires

{Dˉα˙,Dˉβ˙}Φ=0,\{\bar D_{\dot\alpha},\bar D_{\dot\beta}\}\Phi=0,

which holds identically in flat superspace. This is the graded Frobenius condition for the distribution spanned by the barred derivatives.

Introduce

yμ=xμ+iθσμθˉ.y^\mu=x^\mu+i\theta\sigma^\mu\bar\theta.

With left differentiation and yy held fixed,

Dˉα˙=−∂∂θˉα˙∣y,θ.\bar D_{\dot\alpha} =-\left. \frac{\partial}{\partial\bar\theta^{\dot\alpha}} \right|_{y,\theta}.

Therefore the general local solution is

Φ=Φ(y,θ),\Phi=\Phi(y,\theta),

with no independent θˉ\bar\theta dependence. Since there are two independent θ\theta components, its finite expansion is

Φ(y,θ)=A(y)+2 θψ(y)+θθF(y).\Phi(y,\theta) =A(y)+\sqrt2\,\theta\psi(y)+\theta\theta F(y).

This is an off-shell irreducibility constraint: AA, ψ\psi, and FF remain arbitrary functions of yy. It has not imposed a Klein–Gordon, Weyl, or auxiliary field equation.

The antichiral condition

DαΦˉ=0D_\alpha\bar\Phi=0

is solved in yˉμ=xμ−iθσμθˉ\bar y^\mu=x^\mu-i\theta\sigma^\mu\bar\theta by

Φˉ(yˉ,θˉ)=A∗(yˉ)+2 θˉψˉ(yˉ)+θˉθˉF∗(yˉ)\bar\Phi(\bar y,\bar\theta) =A^*(\bar y)+\sqrt2\,\bar\theta\bar\psi(\bar y) +\bar\theta\bar\theta F^*(\bar y)

in Lorentzian signature. The starred fields cease to be a valid pointwise Euclidean interpretation on the Euclidean page.

Taylor-expanding the coefficient fields about xμx^\mu gives

Φ(x,θ,θˉ)=  A+2 θψ+θθF+iθσμθˉ ∂μA−i2θθ ∂μψ σμθˉ+14θθθˉθˉ □A.\begin{aligned} \Phi(x,\theta,\bar\theta) =\;&A +\sqrt2\,\theta\psi +\theta\theta F +i\theta\sigma^\mu\bar\theta\,\partial_\mu A\\ &-\frac{i}{\sqrt2}\theta\theta\, \partial_\mu\psi\,\sigma^\mu\bar\theta +\frac14\theta\theta\bar\theta\bar\theta\,\Box A. \end{aligned}

The series terminates because every monomial beyond degree two in either θ\theta or θˉ\bar\theta vanishes. This expression passes three independent checks:

  1. applying Dˉα˙\bar D_{\dot\alpha} gives zero term by term;
  2. every term has the same engineering dimension when [θ]=−1/2[\theta]=-1/2;
  3. setting θˉ=0\bar\theta=0 returns the unconstrained polynomial in θ\theta.

The coefficient 1/41/4 in the final term follows from the second Taylor term and the identity

(θσμθˉ)(θσνθˉ)=−12θθθˉθˉ ημν.(\theta\sigma^\mu\bar\theta) (\theta\sigma^\nu\bar\theta) =-\frac12\theta\theta\bar\theta\bar\theta\,\eta^{\mu\nu}.

The constraint solution and its component expansion are derived in Martin 2016, §§ 4.1–4.3, pp. 31–37, Weinberg 2000, §§ 26.2–26.3, pp. 59–74, and structurally in Gates, Grisaru, Roček, and Siegel 1983, §§ 3.5–3.6, pp. 89–96.

Write a vertical bar for evaluation at θ=θˉ=0\theta=\bar\theta=0. With the present epsilon convention,

A=Φ∣,ψα=12DαΦ∣,F=−14D2Φ∣.A=\Phi|, \qquad \psi_\alpha=\frac1{\sqrt2}D_\alpha\Phi|, \qquad F=-\frac14D^2\Phi|.

The last sign is a normalization statement: here D2(θθ)∣=−4D^2(\theta\theta)|=-4. A source using D2θ2=+4D^2\theta^2=+4 must change the projection and every later FF-term formula together.

Apply δϵ=ϵQ+ϵˉQˉ\delta_\epsilon=\epsilon Q+\bar\epsilon\bar Q before projecting. The parameters and the spinor derivatives are both odd, so their relative sign must be shown explicitly. For example,

Dα(ϵβQβΦ)=−ϵβDαQβΦ=+ϵβQβDαΦ.D_\alpha\big(\epsilon^\beta Q_\beta\Phi\big) =-\epsilon^\beta D_\alpha Q_\beta\Phi =+\epsilon^\beta Q_\beta D_\alpha\Phi.

The first minus sign is the graded Leibniz sign; the second uses {Dα,Qβ}=0\{D_\alpha,Q_\beta\}=0. The same two signs occur in the barred term, so the even transformation δϵ\delta_\epsilon commutes with DαD_\alpha.

Now work through the fermion projection. At θ=θˉ=0\theta=\bar\theta=0, the differential supercharges reduce to the corresponding leading spinor derivatives, and therefore

δψα=12(ϵβDβDαΦ+ϵˉβ˙Dˉβ˙DαΦ)∣=12[2ϵαF+2i(σμϵˉ)α∂μA].\begin{aligned} \delta\psi_\alpha &=\frac1{\sqrt2} \left( \epsilon^\beta D_\beta D_\alpha\Phi +\bar\epsilon_{\dot\beta} \bar D^{\dot\beta}D_\alpha\Phi \right)\bigg|\\ &=\frac1{\sqrt2} \left[ 2\epsilon_\alpha F +2i(\sigma^\mu\bar\epsilon)_\alpha \partial_\mu A \right]. \end{aligned}

For the first term, DβDα=12ϵβαD2D_\beta D_\alpha=\tfrac12\epsilon_{\beta\alpha}D^2 and D2Φ∣=−4FD^2\Phi|=-4F. For the second, chirality removes DαDˉβ˙ΦD_\alpha\bar D^{\dot\beta}\Phi, while the mixed anticommutator supplies −2iϵβ˙γ˙σαγ˙μ∂μΦ-2i\epsilon^{\dot\beta\dot\gamma} \sigma^\mu_{\alpha\dot\gamma}\partial_\mu\Phi. The contraction ϵˉβ˙ϵβ˙γ˙=−ϵˉγ˙\bar\epsilon_{\dot\beta}\epsilon^{\dot\beta\dot\gamma} =-\bar\epsilon^{\dot\gamma} supplies the compensating minus sign. Thus the scalar, fermion, and top projections give

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}

Thus the superspace constraint reproduces the component multiplet exactly. Conversely, exponentiating the component transformations reconstructs the translated chiral superfield. This is the component–superspace round trip.

For a collection of covariant derivatives ∇A\nabla_A, a proposed constraint

∇rU=0\nabla_r\mathscr U=0

is consistent only if every graded commutator of constrained directions acts within the same constraint ideal:

[∇r,∇s}U=Trst∇tU+FrsU.[\nabla_r,\nabla_s\}\mathscr U =T_{rs}{}^t\nabla_t\mathscr U +\mathcal F_{rs}\mathscr U.

The torsion term is harmless when it points along already-constrained derivatives. The curvature term must vanish on the representation or be canceled by additional constraints. For gauge-covariant chirality,

∇ˉα˙Φ=0,\bar\nabla_{\dot\alpha}\Phi=0,

one needs the conventional integrability condition

{∇ˉα˙,∇ˉβ˙}=0\{\bar\nabla_{\dot\alpha},\bar\nabla_{\dot\beta}\}=0

on the relevant bundle. This condition is not automatic for an arbitrary connection; it is part of the superspace gauge geometry.

A differential condition may also be integrable yet dynamical. For the canonical free massless action

S0=∫d4x d4θ  ΦˉΦ,S_0=\int\mathrm d^4x\,\mathrm d^4\theta\; \bar\Phi\Phi,

with boundary conditions that make superspace and spacetime integration by parts legitimate, the superfield equation and its conjugate are

−14Dˉ2Φˉ=0,−14D2Φ=0.-\frac14\bar D^2\bar\Phi=0, \qquad -\frac14D^2\Phi=0.

They are chiral and antichiral, respectively, and algebraically consistent, but together their projections set F=0F=0 and impose the massless Weyl and Klein–Gordon equations.

The qualifier “massless” matters. Adding the quadratic superpotential in

Sm=S0+[∫d4x d2θ  m2Φ2+c.c.]S_m=S_0+\left[ \int\mathrm d^4x\,\mathrm d^2\theta\; \frac m2\Phi^2+\text{c.c.} \right]

changes the chiral equation to

−14Dˉ2Φˉ+mΦ=0.-\frac14\bar D^2\bar\Phi+m\Phi=0.

Its lowest projection is F∗+mA=0F^*+mA=0, and higher projections give the massive fermion equation and (□+∣m∣2)A=0(\Box+\lvert m\rvert^2)A=0. Chirality itself remains a kinematic off-shell constraint in both theories; only the action-dependent superfield equation puts the multiplet on shell. Integrability and off-shell status are therefore separate questions.

Many references choose at least one of the following alternatives:

ChoiceThis pageCommon alternative
Momentum operatorPμ=i∂μP_\mu=i\partial_\muPμ=−i∂μP_\mu=-i\partial_\mu
Chiral coordinatey=x+iθσθˉy=x+i\theta\sigma\bar\thetay=x−iθσθˉy=x-i\theta\sigma\bar\theta
Grassmann derivativeLeftRight
Auxiliary projectionF=−14D2Φ∣θ=θˉ=0F=-\tfrac14D^2\Phi\rvert_{\theta=\bar\theta=0}F=+14D2Φ∣θ=θˉ=0F=+\tfrac14D^2\Phi\rvert_{\theta=\bar\theta=0}

A safe translation changes QQ, DD, yy, the component expansion, and the projection rule as one system. The invariant checks are the super-Poincaré anticommutator, DˉΦ=0\bar D\Phi=0, and closure of the component transformations.

Covariant does not mean gauge covariant by itself. Flat DαD_\alpha is covariant under rigid supertranslations. A gauge-covariant derivative ∇α\nabla_\alpha includes a connection and has additional curvature constraints.

A consistent constraint need not be kinematic. Chirality selects an off-shell multiplet; a superfield Euler–Lagrange equation selects solutions. Both are supersymmetric differential constraints.

Component projection is convention sensitive. A wrong factor in D2Φ∣D^2\Phi| propagates into auxiliary equations, potentials, and closure checks.

Show that Dˉα˙yμ=0\bar D_{\dot\alpha}y^\mu=0 and conclude that every function Φ(y,θ)\Phi(y,\theta) is chiral.

Solution

At fixed xx, the left derivative of θσμθˉ\theta\sigma^\mu\bar\theta with respect to θˉ\bar\theta carries the graded sign that makes

−∂ˉα˙yμ=+iθβσβα˙μ.-\bar\partial_{\dot\alpha}y^\mu =+i\theta^\beta\sigma^\mu_{\beta\dot\alpha}.

This cancels the second term −iθβσβα˙μ∂μyν-i\theta^\beta\sigma^\mu_{\beta\dot\alpha}\partial_\mu y^\nu. The chain rule then gives Dˉα˙Φ(y,θ)=0\bar D_{\dot\alpha}\Phi(y,\theta)=0.

Starting from

Dα=∂α+c iσαα˙μθˉα˙∂μ,D_\alpha=\partial_\alpha +c\,i\sigma^\mu_{\alpha\dot\alpha} \bar\theta^{\dot\alpha}\partial_\mu,

compute {Dα,Qˉβ˙}\{D_\alpha,\bar Q_{\dot\beta}\} on a test superfield. Then use the resulting value of cc to recover the sign of {Dα,Dˉβ˙}\{D_\alpha,\bar D_{\dot\beta}\}.

Solution

The coordinate-derivative cross terms give

{Dα,Qˉβ˙}=i(1−c)σαβ˙μ∂μ.\{D_\alpha,\bar Q_{\dot\beta}\} =i(1-c)\sigma^\mu_{\alpha\dot\beta}\partial_\mu.

Covariance under the left supertranslation action therefore requires c=+1c=+1. Replacing the +iθσ∂+i\theta\sigma\partial term of Qˉ\bar Q by the −iθσ∂-i\theta\sigma\partial term of Dˉ\bar D makes the two cross terms add rather than cancel:

{Dα,Dˉβ˙}=−2iσαβ˙μ∂μ.\{D_\alpha,\bar D_{\dot\beta}\} =-2i\sigma^\mu_{\alpha\dot\beta}\partial_\mu.

Use the ordered definitions of D2D^2 and Dˉ2\bar D^2 to verify

F=−14D2Φ∣,F∗=−14Dˉ2Φˉ∣.F=-\frac14D^2\Phi|, \qquad F^*=-\frac14\bar D^2\bar\Phi|.
Solution

At the origin of odd coordinates, Dα=∂αD_\alpha=\partial_\alpha and Dˉα˙=−∂ˉα˙\bar D_{\dot\alpha}=-\bar\partial_{\dot\alpha}. The declared order gives

D2(θθ)=−4,Dˉ2(θˉθˉ)=−4.D^2(\theta\theta)=-4, \qquad \bar D^2(\bar\theta\bar\theta)=-4.

All lower-degree terms vanish after the two derivatives and projection, so the two displayed formulas return FF and F∗F^*. If one reverses the order in Dˉ2\bar D^2, its sign flips; the antichiral projector and Wα=−Dˉ2DαV/4W_\alpha=-\bar D^2D_\alpha V/4 must then be changed with it.

Suppose {∇ˉα˙,∇ˉβ˙}U=Fα˙β˙U\{\bar\nabla_{\dot\alpha},\bar\nabla_{\dot\beta}\}\mathscr U =\mathcal F_{\dot\alpha\dot\beta}\mathscr U. When is ∇ˉα˙U=0\bar\nabla_{\dot\alpha}\mathscr U=0 consistent?

Solution

It requires Fα˙β˙U=0\mathcal F_{\dot\alpha\dot\beta}\mathscr U=0. This may follow from a conventional curvature constraint, from U\mathscr U being neutral, or from an additional representation condition. Without one of these, applying two constrained derivatives produces an independent obstruction.

Chiral, Vector, Linear, and Field-Strength Superfields applies these derivative constraints to the standard N=1\mathcal N=1 multiplets. Euclidean Superspace, Conjugation, and Field-Space Complexification explains which conjugation statements survive analytic continuation.

  • 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.

  • Martin, Stephen P. “A Supersymmetry Primer.” In Perspectives on Supersymmetry II, edited by Gordon L. Kane, 1–153. Singapore: World Scientific, 2010. Version 7, 2016. arXiv:hep-ph/9709356. DOI.

  • Weinberg, Steven. The Quantum Theory of Fields. Volume III: Supersymmetry. Cambridge: Cambridge University Press, 2000, §§ 26.2–26.3. DOI.

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