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F- and D-Term Breaking, Vacuum Energy, and the Goldstino

In a two-derivative rigid four-dimensional N=1\mathcal N=1 chiral–vector theory with positive auxiliary-field metrics, nonzero on-shell F- or D-terms at a Lorentz-invariant vacuum are equivalent to positive vacuum energy. More generally, when the global supercharges and the usual Goldstone-theorem hypotheses are valid, positive vacuum energy means that supersymmetry is broken and forces a massless fermionic pole in the supercurrent. That fermion can be an elementary field combination in weak coupling or a composite state in a strongly interacting theory. This page derives both levels of the statement, identifies the goldstino in a mixed chiral–vector model, and marks where stationarity, gauge invariance, boundaries, or supergravity change the conclusion.

Required background. Use the component normalizations and auxiliary equations from Gauge–Matter Systems, F- and D-Term Potentials, and the positive-energy argument from Four-Dimensional N=1 Supersymmetry.

Helpful background. The current-algebra step uses the charge and surface-term conditions developed in Spacetime Currents, Stress Tensors, and Charge Algebras.

Auxiliary fields and the positive potential

Section titled “Auxiliary fields and the positive potential”

Take chiral multiplets (ϕi,ψi,Fi)(\phi^i,\psi^i,F^i) in a unitary representation of a compact gauge group and vector multiplets (Aμa,λa,Da)(A_\mu^a,\lambda^a,D^a). For the explicit component derivation, assume canonical Kähler metric, constant gauge couplings gag_a, no boundary, and a gauge-invariant superpotential W(ϕ)W(\phi). An Abelian factor may have a rigid Fayet–Iliopoulos parameter ξa\xi^a. The algebraic part of the Lagrangian is

Laux=Fi∗Fi+WiFi+W‾iˉF∗iˉ+12DaDa−Da ⁣[gaϕ†Taϕ+ξa],\begin{aligned} \mathcal L_{\rm aux} ={}&F_i^*F^i+W_iF^i+\overline W_{\bar i}F^{*\bar i}\\ &+\frac12D^aD^a -D^a\!\left[g_a\phi^\dagger T^a\phi+\xi^a\right], \end{aligned}

where Wi=∂W/∂ϕiW_i=\partial W/\partial\phi^i and ξa\xi^a is allowed only for an admissible Abelian factor. This is the site convention Pa=gaμa+ξa\mathcal P_a=g_a\mu_a+\xi_a and Da=PaD^a=\mathcal P_a for a canonical gauge kinetic term. Completing squares gives

Fi=−W‾iˉ,Da=gaϕ†Taϕ+ξa,F^i=-\overline W_{\bar i}, \qquad D^a=g_a\phi^\dagger T^a\phi+\xi^a,

and

V(ϕ,ϕˉ)=∑i∣Fi∣2+12∑a(Da)2≥0.V(\phi,\bar\phi) =\sum_i|F^i|^2+\frac12\sum_a(D^a)^2\geq0.

For a noncanonical Kähler potential, the first term is WiKijˉW‾jˉW_iK^{i\bar j}\overline W_{\bar j}; positivity requires a positive Kähler metric. In either case a Lorentz-invariant field configuration is supersymmetric precisely when the inhomogeneous parts of all fermion transformations vanish, which here requires

Fi=0,Da=0,F^i=0, \qquad D^a=0,

because derivative and field-strength terms in the fermion variations vanish on that configuration. The auxiliary fields themselves are not transformation laws. Therefore incompatible FF- and DD-flatness equations prove that no supersymmetric configuration exists in the stated field domain. They do not yet prove that the potential has a stationary, stable, or normalizable vacuum.

The operator algebra gives the same criterion without weak coupling. If the global supercharges are well defined and surface terms vanish,

⟨Ω∣H∣Ω⟩=14∑α=12(∥Qα∣Ω⟩∥2+∥Qα†∣Ω⟩∥2).\langle\Omega|H|\Omega\rangle =\frac14\sum_{\alpha=1}^{2} \left( \lVert Q_\alpha|\Omega\rangle\rVert^2 +\lVert Q_\alpha^\dagger|\Omega\rangle\rVert^2 \right).

The normalization follows from {Qα,Qˉα˙}=2σαα˙μPμ\{Q_\alpha,\bar Q_{\dot\alpha}\}=2\sigma^\mu_{\alpha\dot\alpha}P_\mu. Thus a normalizable zero-energy ground state is supersymmetric, while a ground state of strictly positive energy breaks supersymmetry. For an infinite homogeneous system, both sides are understood through energy density and smeared local charges before the thermodynamic limit. Weinberg 2000, §§29.1–29.2, pp. 248–263 develops both the algebraic and current forms of this statement.

At a constant vacuum, the inhomogeneous parts of the fermion transformations are, in these conventions,

δψi=2 ϵFi,δλa=iϵDa.\delta\psi^i=\sqrt2\,\epsilon F^i, \qquad \delta\lambda^a=i\epsilon D^a.

Define the breaking scale by the vacuum energy density,

f2≡Vvac=Fi∗Fi+12DaDa.f^2\equiv V_{\rm vac} =F_i^*F^i+\frac12D^aD^a.

If f≠0f\neq0, the normalized fermionic direction

G=1f(Fi∗ψi−i2Daλa)G =\frac{1}{f} \left(F_i^*\psi^i-\frac{i}{\sqrt2}D^a\lambda^a\right)

shifts as δG=2f ϵ+derivative terms\delta G=\sqrt2f\,\epsilon+\text{derivative terms}. Orthogonal fermion combinations have no constant shift. This identifies the goldstino without diagonalizing a mass matrix; it also shows how F- and D-term order parameters mix.

The shift must be compatible with a zero eigenvalue of the fermion mass matrix at a stationary point. Keep the phase fixed by the gauge Yukawa interaction −i2ga(ϕ†Ta)iψiλa+h.c.-i\sqrt2g_a(\phi^\dagger T^a)_i\psi^i\lambda^a+\text{h.c.} rather than hiding it in an unspecified redefinition. In the basis (ψi,λa)(\psi^i,\lambda^a),

MF=(Wiji2ga(ϕ†Ta)ii2gb(ϕ†Tb)j0).\mathcal M_F= \begin{pmatrix} W_{ij} & i\sqrt2g_a(\phi^\dagger T^a)_i\\ i\sqrt2g_b(\phi^\dagger T^b)_j & 0 \end{pmatrix}.

Differentiating the potential gives

0=∂iV=−WijFj+gaDa(ϕ†Ta)i.0=\partial_iV =-W_{ij}F^j+g_aD^a(\phi^\dagger T^a)_i.

Gauge invariance, Wi(Taϕ)i=0W_i(T^a\phi)^i=0, gives the conjugate relation (ϕ†Ta)iFi=0(\phi^\dagger T^a)_iF^i=0. Consequently,

MF(FjiDa/2)=0.\mathcal M_F \begin{pmatrix}F^j\\iD^a/\sqrt2\end{pmatrix}=0.

The complex-conjugate coefficients of this null vector give the field GG displayed above. Equivalently, after the explicit rephasing λ~a=iλa\widetilde\lambda^a=i\lambda^a, the off-diagonal entries are real, the null vector is (Fj,−Da/2)(F^j,-D^a/\sqrt2), and G=(Fi∗ψi−Daλ~a/2)/fG=(F_i^*\psi^i-D^a\widetilde\lambda^a/\sqrt2)/f. The zero mode is a consequence of stationarity plus gauge invariance, not merely of V>0V>0 at an arbitrary field point. In a pure Wess–Zumino model this collapses to WijFj=0W_{ij}F^j=0. A nonzero F-term therefore supplies an exact tree-level massless fermion at every stationary point, even when the scalar Hessian later reveals a saddle. Weinberg 2000, §27.5, pp. 146–148; §29.2, pp. 263–264 gives the corresponding component zero-mode check.

With a curved Kähler metric, ordinary derivatives are replaced by Kähler-covariant ones and the normalized direction uses the metric. With field-dependent gauge kinetic functions, gaugino masses and additional mixing enter, but the full stationary mass matrix still annihilates the supersymmetry-variation direction when the action is exactly supersymmetric.

The massless fermion is not only a tree-level accident. Let SαμS^\mu_\alpha be a conserved supercurrent whose charge generates supersymmetry. Spontaneous breaking means that some local operator has a nonzero vacuum variation, equivalently that the charge does not annihilate the vacuum. Schematically, with the overall factor of ii and improvement contact terms fixed by the time-ordering convention, the supercurrent Ward identity contains

∂μ⟨0∣T Sαμ(x)Sˉβ˙ν(0)∣0⟩=2σαβ˙ρ⟨0∣Tρν∣0⟩ δ4(x)+contact terms.\partial_\mu \langle0|T\,S^\mu_\alpha(x)\bar S^\nu_{\dot\beta}(0)|0\rangle =2\sigma^\rho_{\alpha\dot\beta} \langle0|T_\rho{}^\nu|0\rangle\,\delta^4(x) +\text{contact terms}.

For a homogeneous Lorentz-invariant vacuum, ⟨Tρν⟩=Vvacδρν\langle T_\rho{}^\nu\rangle=V_{\rm vac}\delta_\rho{}^\nu. A nonzero right-hand side cannot be reproduced by a correlator analytic at zero momentum, so the Ward identity requires a massless singularity. Lorentz covariance permits

⟨0∣Sαμ(0)∣G(p)⟩=i2f (σμuˉ(p))αup to improvement and phase conventions.\langle0|S^\mu_\alpha(0)|G(p)\rangle =i\sqrt2f\,(\sigma^\mu\bar u(p))_\alpha \quad\text{up to improvement and phase conventions}.

Insertion into the spectral representation produces a 1/p21/p^2 pole with residue fixed by f2f^2. Interactions may rotate an elementary combination into a composite one, but cannot gap the goldstino while global supersymmetry remains exact and spontaneously broken. This is the fermionic Goldstone theorem first formulated in current-algebra language by Salam and Strathdee 1974, pp. 465–467; a component derivation and normalization check appear in Weinberg 2000, §29.2, pp. 256–263.

The improvement ambiguity Sμ↦Sμ+∂νB[νμ]S^\mu\mapsto S^\mu+\partial_\nu B^{[\nu\mu]} changes contact terms and the representative current, not the conserved charge or the physical pole when surface terms vanish. If a boundary supports flux, however, the improvement term can change the charge and the boundary degrees of freedom must be included.

The decision flow below assembles these statements in their logical order and then tests them in the exact classical O’Raifeartaigh and Fayet–Iliopoulos model families. Follow the failure exit whenever stationarity, physical stability, normalizability, or the conserved charge has not been established.

From auxiliary order parameters to the Goldstino — print equivalent

This reflow preserves the figure’s hypothesis gate, exact identities, and benchmark branches at readable print size.

1. Full ground-state gate

Assume an exact rigid four-dimensional N=1 theory with positive kinetic metrics, a stationary and physically stable Lorentz-invariant ground state, a normalizable state, and a well-defined conserved supercharge with no unaccounted boundary or central terms.

Only under that gate, f² ≡ Vvac = Σi|Fi|² + ½Σa(Da)², and f > 0 is equivalent to spontaneous supersymmetry breaking. A merely local or metastable stationary state does not by itself pass the full ground-state theorem.

2. Goldstino and current pole

Stationarity plus gauge invariance gives MF(Fj, iDa/√2)T = 0. The normalized field is G = [Fi*ψi − iDaλa/√2]/f, up to phase conventions.

Its inhomogeneous shift produces ⟨0|Sμα|G(p)⟩ = i√2f(σμū)α, up to improvements and phase, and hence a massless 1/p² supercurrent pole. At an arbitrary nonstationary field point, nonzero F or D does not imply this null vector.

3. Exact O’Raifeartaigh branches

For W = fX + ½hXφ₁² + mφ₁φ₂ and y = hf/m²: when 0 < y ≤ 1, φ₁ = φ₂ = 0 with X arbitrary, Vmin = f², and (FX, F₁, F₂) = (−f, 0, 0). When y > 1, define Δ = hf − m² and r² = 2Δ/h²; then φ₁ = ±ir, φ₂ = −(hX/m)φ₁, Vmin = f² − Δ²/h², and (FX, F₁, F₂) = (−m²/h, 0, −mφ₁*). The two branches meet at y = 1.

4. Exact Fayet–Iliopoulos branches

For the anomaly-free U(1) pair with W = mΦ₊Φ₋ and D = g(|φ₊|² − |φ₋|²) + ξ: when gξ < m², the origin is the unbroken-gauge minimum, Vmin = ξ²/2, and D = ξ. When gξ > m², φ₊ = 0 and |φ₋|² = ξ/g − m²/g²; the U(1) is Higgsed, Vmin = m²ξ/g − m⁴/(2g²), D = m²/g, and F₊ = −mφ₋*. The descriptions meet at gξ = m².

Boundary of the conclusion

These cards verify exact classical stationary data, not the full ground-state gate. The noncompact O’Raifeartaigh X direction still requires quantum lifting and a normalizable vacuum. A constant FI term also has current-multiplet and supergravity consistency conditions outside this rigid benchmark.

For a proposed weakly coupled vacuum, perform the following checks in order.

  1. Specify the field domain. Include gauge identifications, singular loci, and allowed behavior at infinity.
  2. Solve auxiliary equations. Show whether Fi=Da=0F_i=D^a=0 can be satisfied anywhere, including runaway limits.
  3. Find stationary points. Solve ∂V=0\partial V=0; do not infer one from incompatible flatness equations.
  4. Remove redundancies and test stability. Quotient gauge orbits, separate Goldstone directions, and diagonalize the physical scalar Hessian.
  5. Identify the goldstino. Compute (Fi,iDa/2)(F^i,iD^a/\sqrt2) in the declared gaugino convention and verify that the full fermion mass matrix has this null vector.
  6. State global status. Distinguish a global vacuum, a local minimum with a specified lower endpoint, a saddle, and a runaway.
  7. Name the regime. Record loop expansion parameters, cutoff, and whether the theory is rigid or coupled to gravity.

The first two steps diagnose supersymmetric configurations; all seven are needed for a controlled vacuum claim.

Explicit breaking. If the Lagrangian contains nonsupersymmetric terms, the supercurrent is not conserved and no exactly massless goldstino is required. A spurion can keep bookkeeping supersymmetric, but freezing its F-component is still explicit breaking in the visible theory.

Supergravity. Local supersymmetry gauges the current. The goldstino becomes the longitudinal helicity-1/21/2 component of a massive gravitino, and the scalar potential contains negative terms proportional to the superpotential. Neither V=∑∣F∣2+D2/2V=\sum|F|^2+D^2/2 nor a physical massless goldstino survives unchanged.

Boundaries and central charges. Boundaries, defects, or extended objects can add surface or central terms to the superalgebra. A positive energy may then saturate a BPS bound rather than signal complete breaking. One must test the preserved linear combinations of supercharges.

No vacuum. A potential whose infimum occurs only at infinite field distance may have arbitrarily small energy without a normalizable ground state. “No finite solution of F=0F=0” and “spontaneous breaking in a vacuum” are different conclusions.

Index information. A nonzero well-defined Witten index obstructs breaking, but a zero index is compatible with either a broken vacuum or paired supersymmetric vacua. The index cannot replace the local and global analysis above.

Evaluating VV at a convenient point. Positive VV diagnoses breaking only if the point is a physical state of interest, normally a stationary vacuum. At a generic point it is simply potential energy.

Calling every massless fermion a goldstino. The goldstino is selected by the inhomogeneous supersymmetry transformation and the supercurrent residue. An accidental zero eigenvalue with zero current overlap is not enough.

Ignoring gauge directions in the Hessian. A zero scalar eigenvalue tangent to a gauge orbit is not a pseudomodulus, and a negative eigenvalue in a gauge-fixed but unphysical direction is not a tachyon. Test the quadratic form on gauge-invariant fluctuations.

1. The chiral null vector. For canonical chiral fields with V=WiW‾iV=W_i\overline W_i, show that every stationary point with some Fi≠0F^i\neq0 has a massless Weyl fermion at tree level.

Solution

Since Fi=−W‾iF^i=-\overline W_i,

0=∂iV=WijW‾j=−WijFj.0=\partial_iV=W_{ij}\overline W_j=-W_{ij}F^j.

The chiral-fermion mass matrix is WijW_{ij}, so FjF^j is a nonzero null vector. The corresponding normalized fermion is G=Fi∗ψi/(Fj∗Fj)1/2G=F_i^*\psi^i/(F_j^*F^j)^{1/2}. This proves a massless fermion at a stationary point; it says nothing about scalar stability.

2. Mixed breaking. Suppose ∣F∣2=3D2/2|F|^2=3D^2/2 for one chiral and one Abelian vector multiplet. What fraction of the normalized goldstino norm lies in the gaugino?

Solution

The norm is f2=∣F∣2+D2/2=2D2f^2=|F|^2+D^2/2=2D^2. The gaugino contribution is D2/2D^2/2, so its fraction is (D2/2)/(2D2)=1/4(D^2/2)/(2D^2)=1/4. The remaining 3/43/4 lies in the chiral fermion.

3. Diagnose the claim. A potential has no finite solution of Fi=0F_i=0, but along ϕ=t\phi=t one finds V(t)→0V(t)\to0 as t→∞t\to\infty. Is supersymmetry spontaneously broken?

Solution

Not enough information is given. There is no finite supersymmetric configuration, but the infimum is zero at infinite field distance. One must determine whether a normalizable ground state exists, whether the limit is a physical vacuum, and whether the global charges are defined. The appropriate conclusion is a supersymmetric runaway or no vacuum, not automatically spontaneous breaking in a stable state.

  • Salam, A., and J. Strathdee. “On Goldstone Fermions.” Physics Letters B 49 (1974): 465–467. DOI.
  • Weinberg, S. The Quantum Theory of Fields, Volume III: Supersymmetry. Cambridge: Cambridge University Press, 2000, §§29.1–29.2. DOI.

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