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Background fields

A background field is a prescribed source held fixed while the matter fields fluctuate. “Auxiliary” instead means that a field has an algebraic equation of motion in a particular action. A background field can descend from an auxiliary field of supergravity without being integrated out in the rigid matter theory.

For the derivations, use the source construction and the background-field lesson. This page provides the compact definitions and the translation between the original three-manifold paper and its sequel.

VariableIn the rigid matter theoryWhat equation is relevant?
Metric and bosonic gravity sourcesPrescribedBackground-preservation conditions if supersymmetry is wanted
Background gravitiniSet to zero on a bosonic backgroundTheir supersymmetry variations must also vanish
Matter scalar and fermionDynamicalMatter field equations; these need not hold for an off-shell symmetry check
Matter auxiliary field, such as FΦF_\PhiPart of the off-shell matter variablesIt may be eliminated with its own algebraic equation, changing how closure is expressed
Flavor connectionPrescribed when used as an external probeIts full source multiplet must preserve the desired supercharge
Dynamical gauge connectionIntegrated overGauge-field equations and gauge redundancy

The source is not allowed to follow each fluctuating matter configuration. Fixing a source u=u0u=u_0 and imposing its would-be equation u=−λxu=-\lambda x are different operations. The Gaussian comparison calculates their different effects.

This distinction applies in one-dimensional quantum mechanics as well as in three- and four-dimensional field theory. It does not identify their supergravity multiplets. In four dimensions, for example, the old-minimal formulation uses a scalar pair and a vector, while the new-minimal formulation with R-symmetry uses an R-connection and a conserved dual vector. These are different source systems with different gravitino equations. Festuccia–Seiberg, sections 2 and 6, explains the two four-dimensional constructions; do not transfer the three-dimensional coefficients below by changing the index range.

This table uses three-dimensional N=2\mathcal N=2 supergravity sources for a theory with a continuous R-symmetry. The parent theory has four real Lorentzian Poincaré supercharges. In Euclidean signature the two spinor families are independent. The table specifies the sources, not the number of supercharges preserved by a particular background.

Use length coordinates, [∂μ]=1[\partial_\mu]=1, and a real positive-definite metric. Dimensions are engineering mass dimensions of components. Fix ϵ123=1/g\epsilon^{123}=1/\sqrt g in an oriented chart.

FieldDimensionDefinition or role
gμνg_{\mu\nu}00Metric and Levi-Civita spin connection
AμA_\mu11Original paper’s R-gauge potential
CμC_\mu00Potential coupled to the central-charge current
VμV^\mu11−iϵμνρ∂νCρ-i\epsilon^{\mu\nu\rho}\partial_\nu C_\rho
BμνB_{\mu\nu}00Two-form potential, B=12Bμνdxμ∧dxνB=\frac12B_{\mu\nu}dx^\mu\wedge dx^\nu
HH11i2ϵμνρ∂μBνρ\frac i2\epsilon^{\mu\nu\rho}\partial_\mu B_{\nu\rho}

The invariant identities are

V♭=−i∗dC,H=i∗dB,∇μVμ=0.V^\flat=-i*dC,\qquad H=i*dB,\qquad \nabla_\mu V^\mu=0.

Here ∗* is the metric Hodge dual and V♭=VμdxμV^\flat=V_\mu dx^\mu. The divergence follows from the definition; it is not a gravitational equation of motion. A,C,B,V,HA,C,B,V,H can be complex in the Euclidean construction, while the original paper keeps the gauge parameters for AA and CC real. Potentials can require patches. In particular, nonzero ∫H volg\int H\,\mathrm{vol}_g on a closed three-manifold rules out a single smooth global BB.

For a matter component XX of R-charge rXr_X and central-charge eigenvalue zXz_X, define

aμmat=Aμ−12Vμ,Aμ(R)=Aμ−32Vμ.a_\mu^{\mathrm{mat}}=A_\mu-\frac12V_\mu,\qquad A_\mu^{(R)}=A_\mu-\frac32V_\mu.
ExpressionWhere it appears
∇μ−isAμ\nabla_\mu-isA_\muOriginal paper’s spinor equation; s=+1s=+1 for ζ\zeta, s=−1s=-1 for ζ~\widetilde\zeta
∇μ−irXaμmat−izXCμ\nabla_\mu-ir_Xa_\mu^{\mathrm{mat}}-iz_XC_\muThe matter derivative defined in the original paper’s (6.6)
jRμAμ(R)j_R^\mu A_\mu^{(R)}The linear R-current source coupling, also the sequel’s choice of connection symbol

The component charge matters: a chiral scalar of charge rr has a fermion of charge r−1r-1 and an auxiliary of charge r−2r-2. The central charge zXz_X has dimension one; rXr_X is dimensionless. All terms in the matter derivative therefore have dimension one.

At first order around flat space, with gμν=δμν+2hμνg_{\mu\nu}=\delta_{\mu\nu}+2h_{\mu\nu}, the bosonic source coupling is

ΔL=−Tμνhμν+jRμAμ(R)+jZμCμ+JZH.\Delta\mathcal L=-T^{\mu\nu}h_{\mu\nu} +j_R^\mu A_\mu^{(R)}+j_Z^\mu C_\mu+J_ZH.

jZμj_Z^\mu is the central-charge current and JZJ_Z its scalar source partner. This is the original paper’s (7.1). The sequel’s (1.18) instead writes the metric term as −12ΔgμνTμν-\frac12\Delta g_{\mu\nu}T^{\mu\nu}, the same term because Δgμν=2hμν\Delta g_{\mu\nu}=2h_{\mu\nu}.

All three connection combinations acquire dλRd\lambda_R under A↦A+dλRA\mapsto A+d\lambda_R, since VV is invariant. Gauge covariance alone cannot tell you which one belongs in a given formula.

Translate the sequel without losing a vector term

Section titled “Translate the sequel without losing a vector term”

The sequel, The Geometry of Supersymmetric Partition Functions, explicitly defines A(R)=A−32VA^{(R)}=A-\frac32V in Appendix A, equation (A.1). Therefore

A=A(R)+32V,amat=A(R)+V,A=A^{(R)}+\frac32V,\qquad a^{\mathrm{mat}}=A^{(R)}+V,

and the original matter derivative becomes

DμX=[∇μ−irXAμ(R)−irXVμ−izXCμ]X.D_\mu X= \left[\nabla_\mu-ir_XA_\mu^{(R)}-ir_XV_\mu-iz_XC_\mu\right]X.

The extra −irXVμ-ir_XV_\mu remains. For a quick numerical coefficient check, take rX=2r_X=2, zX=0z_X=0, A1=0A_1=0, V1=vV_1=v and X=eipx1X=e^{ipx^1} in a flat local frame. Then A1(R)=−3v/2A_1^{(R)}=-3v/2 and a1mat=−v/2a_1^{\mathrm{mat}}=-v/2. The original expression gives D1X=i(p+v)XD_1X=i(p+v)X. The translated expression gives [ip+3iv−2iv]X[ip+3iv-2iv]X, the same result. Omitting the extra vector term would give i(p+3v)Xi(p+3v)X.

The spinor equations also change appearance. Starting from the original equations and substituting for AA, one obtains

(∇μ−isAμ(R))εs=−H2γμεs+is2Vμεs−s2ϵμνρVνγρεs.(\nabla_\mu-isA_\mu^{(R)})\varepsilon_s =-\frac H2\gamma_\mu\varepsilon_s +\frac{is}{2}V_\mu\varepsilon_s -\frac s2\epsilon_{\mu\nu\rho}V^\nu\gamma^\rho\varepsilon_s.

Here ε+=ζ\varepsilon_+=\zeta and ε−=ζ~\varepsilon_-=\widetilde\zeta. The change from −isVμ-isV_\mu in the original right-hand side to +isVμ/2+isV_\mu/2 is exactly the connection shift. This agrees with the sequel’s equations (1.19)–(1.20); it is the same background equation in different variables.

Identify its dimension, signature, source conventions, and chosen R-symmetry. State which variables are prescribed and which are integrated over. Then specify local fields and global information such as the spin structure, gauge period, holonomies, and potential patches. Vanishing source fermions are not enough: their variations select the preserved spinors. The Killing spinor lesson provides both the local test and a global circle example.