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Gauge–Matter Systems, F- and D-Term Potentials, and FI Data

A rigid four-dimensional N=1\mathcal N=1 gauge–matter theory is determined at two derivatives by a Kähler target with a holomorphic gauge-group action, a gauge-invariant superpotential, a holomorphic gauge kinetic matrix, and any globally admissible Fayet–Iliopoulos data. The chiral auxiliaries measure failure of F-flatness; the vector auxiliaries are shifted moment maps. Eliminating both gives

V=VF+VD=gijˉWiWˉjˉ+12(Ref)1,abPaPb,V=V_F+V_D =g^{i\bar j}W_i\bar W_{\bar j} +\frac12(\operatorname{Re}f)^{-1,ab} \mathcal P_a\mathcal P_b,

with Pa=gμa+ξa\mathcal P_a=g\mu_a+\xi_a in the convention below. Positivity requires positive Kähler and gauge kinetic matrices. The formula is not complete until representations, global gauge form, moment-map normalization, anomaly status, and FI admissibility are recorded.

Required background. Supersymmetric Yang–Mills Actions fixes the vector normalization, Kähler Sigma Models fixes gijˉg_{i\bar j}, and Hamiltonian Group Actions and Moment Maps supplies the geometric moment map.

Helpful background. Global Form, Matter Representations, and the Faithful Gauge Group explains why the Lie algebra alone does not determine the model.

Gauge invariance is a condition on all defining data

Section titled “Gauge invariance is a condition on all defining data”

Let GG act on chiral coordinates ziz^i through holomorphic Killing vectors kai(z)k_a^i(z),

δαzi=αakai(z).\delta_\alpha z^i=\alpha^a k_a^i(z).

For a linear unitary representation, kai=i(Ta)ijzjk_a^i=i(T_a)^i{}_jz^j. Define the real moment map by

jˉμa=igijˉkai,\partial_{\bar j}\mu_a =-i g_{i\bar j}k_a^i,

with the conjugate relation. For canonical KK this gives μa=zTaz\mu_a=z^\dagger T_a z. An additive constant is possible only along an Abelian generator; that is the local origin of FI data.

The complete superspace action is schematically

S=d4xd4θK(Φ,Φe2gV)+d4x[d2θ(W(Φ)+14fab(Φ)WaαWαb)+h.c.]+2d4xd4θξaVa,\begin{aligned} S={}&\int d^4x\,d^4\theta\, K(\Phi,\Phi^\dagger e^{2gV})\\ &+\int d^4x\left[ \int d^2\theta\left( W(\Phi)+\frac14f_{ab}(\Phi)\mathcal W^{a\alpha} \mathcal W^b_\alpha \right)+\text{h.c.}\right]\\ &+2\int d^4x\,d^4\theta\,\xi_aV^a, \end{aligned}

where the final term is present only for admissible Abelian factors and its factor is tied to the chosen VV normalization. Gauge invariance requires:

  • the Kähler metric and symplectic form to be preserved by the action;
  • WW to obey kaiWi=0k_a^iW_i=0 for an ordinary rigid gauge symmetry;
  • fabf_{ab} to transform as an invariant symmetric tensor, including any chiral-field dependence;
  • the matter representation to descend to the declared global group; and
  • perturbative and global gauge anomalies to cancel.

A Kähler potential may transform by a holomorphic plus antiholomorphic term while the metric and rigid action remain invariant. That local freedom must not be confused with a globally defined FI constant or with an allowed supergravity coupling.

Auxiliary elimination produces the full scalar potential

Section titled “Auxiliary elimination produces the full scalar potential”

Suppressing fermion-dependent auxiliary shifts, the component auxiliary sector is

Laux=gijˉFiFˉjˉ+FiWi+FˉjˉWˉjˉ+12habDaDb+DaPa,\mathcal L_{\mathrm{aux}} =g_{i\bar j}F^i\bar F^{\bar j} +F^iW_i+\bar F^{\bar j}\bar W_{\bar j} +\frac12h_{ab}D^aD^b +D^a\mathcal P_a,

where hab=Refabh_{ab}=\operatorname{Re}f_{ab} and Pa=gμa+ξa\mathcal P_a=g\mu_a+\xi_a. Varying independent barred and unbarred fields gives

Fi=gijˉWˉjˉ,Da=h1,abPb.F^i=-g^{i\bar j}\bar W_{\bar j}, \qquad D^a=-h^{-1,ab}\mathcal P_b.

Completing both squares yields

Laux,on=gijˉWiWˉjˉ12h1,abPaPb,\mathcal L_{\mathrm{aux,on}} =-g^{i\bar j}W_i\bar W_{\bar j} -\frac12h^{-1,ab}\mathcal P_a\mathcal P_b,

so the potential is the positive expression in the opening when gg and hh are positive. The classical supersymmetric-vacuum equations are

Wi=0,Pa=0,W_i=0, \qquad \mathcal P_a=0,

modulo gauge equivalence, provided the metric matrices are nonsingular. These equations define a candidate classical vacuum space; stability, singular strata, invariant coordinates, and quantum corrections are treated in the next chapter.

For canonical matter, the principal fermion interactions are

Lferm,int=12Wijψiψj2gϕTaψλa+h.c.,\mathcal L_{\mathrm{ferm,int}} =-\frac12W_{ij}\psi^i\psi^j -\sqrt2g\,\phi^\dagger T^a\psi\,\lambda^a +\text{h.c.},

in addition to gauge-covariant kinetic terms. A nontrivial Kähler metric replaces WijW_{ij} by iWj\nabla_iW_j and covariantizes the gauge Yukawa term; field-dependent fabf_{ab} adds gaugino–matter couplings. These interactions are not optional decorations: their coefficients are fixed by the same superspace action as VFV_F and VDV_D. The canonical construction is worked out in Weinberg 2000, §§27.1 and 27.4, pp. 113–121 and 132–143.

An anomaly-free Abelian model checks every coefficient

Section titled “An anomaly-free Abelian model checks every coefficient”

Take G=U(1)G=U(1) with chiral fields Φ+\Phi_+ and Φ\Phi_- of charges +1+1 and 1-1, canonical KK, constant canonical gauge kinetic term, and

W=mΦ+Φ.W=m\Phi_+\Phi_-.

The opposite charges cancel the cubic and mixed gravitational U(1)U(1) anomalies in this two-field sector, and WW is gauge invariant. With FI parameter ξ\xi,

F+=mϕ,F=mϕ+,D=[g(ϕ+2ϕ2)+ξ].\begin{aligned} F_+&=-m^*\phi_-^*, &F_-&=-m^*\phi_+^*,\\ D&=-\left[g(|\phi_+|^2-|\phi_-|^2)+\xi\right]. \end{aligned}

Therefore

V=m2(ϕ+2+ϕ2)+12[g(ϕ+2ϕ2)+ξ]2.V=|m|^2(|\phi_+|^2+|\phi_-|^2) +\frac12\left[g(|\phi_+|^2-|\phi_-|^2)+\xi\right]^2.

The corresponding Yukawa terms are

LYukawa=mψ+ψ2g(ϕ+ψ+ϕψ)λ+h.c.\mathcal L_{\mathrm{Yukawa}} =-m\psi_+\psi_- -\sqrt2g(\phi_+^*\psi_+-\phi_-^*\psi_-)\lambda +\text{h.c.}

Three checks are immediate.

  1. Setting g=0g=0 reproduces two massive chiral multiplets.
  2. Setting m=0m=0 leaves the D-flat equation g(ϕ+2ϕ2)+ξ=0g(|\phi_+|^2-|\phi_-|^2)+\xi=0 modulo U(1)U(1).
  3. For m0m\neq0, F-flatness requires ϕ+=ϕ=0\phi_+=\phi_-=0; a nonzero ξ\xi then leaves D=ξD=-\xi, so no supersymmetric classical vacuum exists in this model.

The third conclusion is model-specific. It does not say that every FI theory breaks supersymmetry; additional charged fields or another superpotential can solve all auxiliary equations.

FI terms carry global and current-theoretic conditions

Section titled “FI terms carry global and current-theoretic conditions”

A constant linear term ξaDa\xi_aD^a is gauge invariant only when aa labels an Abelian direction admitting an invariant linear functional. A semisimple non-Abelian algebra has no such invariant vector. Even for U(1)U(1), one must record:

  • the compact or noncompact global group and charge normalization;
  • whether the FI parameter is compatible with large gauge transformations, boundaries, and the allowed bundles;
  • cancellation of gauge and mixed anomalies;
  • whether the U(1)U(1) is an ordinary symmetry or an RR symmetry; and
  • which supercurrent multiplet and background coupling remain globally available.

In a rigid local superspace calculation, d4θξV\int d^4\theta\,\xi V is supersymmetric and gauge invariant up to the usual chiral/full-superspace identity. But the Ferrara–Zumino multiplet obtained by a standard improvement is not gauge invariant in the presence of a genuine FI term. This obstruction and its consequences are established in Komargodski and Seiberg 2010, §§1, 3.1, pp. 2–4 and 11–13, Open PDF. It is therefore wrong to infer background or supergravity compatibility from the local scalar potential alone.

Before accepting a potential or vacuum equation, verify:

fieldrequired record
gauge dataglobal group, Lie algebra basis, T(R)T(R), charges, coupling placement, theta sectors
chiral datatarget patch, positive gijˉg_{i\bar j}, representation and faithful quotient
holomorphic datagauge invariance and dimensions of WW; covariance and positivity of fabf_{ab}
moment mapsign, additive constants, coupling factor, and equivariance
FI dataAbelian direction, global admissibility, anomaly and supercurrent implications
eliminationindependent F,Fˉ,DF,\bar F,D, algebraic Hessian, branch and positivity
quantum scoperegulator, scheme, Wilsonian/1PI destination and possible anomalies

The independent round trip is to recover the same FF and DD equations from the component action, from the superfield equations, and from the derivative of the final potential with respect to the auxiliary completion.

Writing VDV_D from charges but omitting g. Whether gg appears in the moment map or in the kinetic matrix depends on normalization. Translate the whole vector multiplet, not just DD.

Adding an FI constant to a non-Abelian generator. A constant shift must be invariant under the adjoint action; semisimple factors do not permit it.

Checking WW only infinitesimally. The representation and operator must also be well-defined under the global gauge group, including quotient identifications and large transformations.

1. Positivity by completing the square. Complete the DD square for a positive matrix habh_{ab}.

Solution 12DThD+DTP=12(D+h1P)Th(D+h1P)12PTh1P.\frac12D^{\mathsf T}hD+D^{\mathsf T}\mathcal P =\frac12(D+h^{-1}\mathcal P)^{\mathsf T}h (D+h^{-1}\mathcal P) -\frac12\mathcal P^{\mathsf T}h^{-1}\mathcal P.

Thus D=h1PD=-h^{-1}\mathcal P and VD=PTh1P/20V_D=\mathcal P^{\mathsf T}h^{-1}\mathcal P/2\geq0.

2. Gauge invariance of the mass term. Verify the U(1)U(1) charge of Φ+Φ\Phi_+\Phi_- and explain why Φ+2\Phi_+^2 is forbidden.

Solution

q(Φ+Φ)=+11=0q(\Phi_+\Phi_-)=+1-1=0, so the mass term is invariant. q(Φ+2)=+2q(\Phi_+^2)=+2, so it is not an operator of the compact U(1)U(1) gauge theory without an additional field or spurion carrying charge 2-2.

F- and D-Flatness and Gauge Quotients constructs the quotient and its singular strata. Supercurrent Multiplets, Improvements, Anomalies, and Background Sources records the FI obstruction, and SQCD: Fields, Symmetries, Invariants, and Classical Moduli Space applies the framework to non-Abelian matter.

  • Komargodski, Zohar, and Nathan Seiberg. “Comments on Supercurrent Multiplets, Supersymmetric Field Theories and Supergravity.” Journal of High Energy Physics 2010, no. 7 (2010): 017. DOI. Open PDF, arXiv v4.
  • Weinberg, Steven. The Quantum Theory of Fields, Volume III: Supersymmetry. Cambridge: Cambridge University Press, 2000, §§27.1 and 27.4, pp. 113–121 and 132–143. DOI.
  • Wess, Julius, and Jonathan Bagger. Supersymmetry and Supergravity. 2nd ed. Princeton, NJ: Princeton University Press, 1992, chs. 6, 22, and 24.