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Changing a metric probes the stress tensor. A supersymmetric change of geometry also changes the sources that accompany the metric. Those additional changes can make a current correlator the most direct way to compute the response. We will follow one complete background and derive the coefficient, including the subtraction needed when two current insertions coincide.

Prepare with the current two-point normalization, squashed spheres and their full background data, and the physical R-symmetry selected by F-maximization. The first supplies the flat correlator; the second supplies the supersymmetric family. Here we compute what its partition-function curvature measures.

Work with a unitary three-dimensional N=2\mathcal N=2 SCFT and its superconformal R-multiplet. Its Lorentzian superconformal algebra has four real Poincaré and four real conformal supercharges. The background below is the four-rigid-supercharge family of P, section 5.2; this specifies preserved curved generators, not a new count for the parent theory. No gauge group or rank is needed.

Fix the theory at its conformal point, set additional flavor masses to zero, and hold the physical R-current fixed as the geometry changes. Write

F(b)=−log⁡Z(b),⟨jμ(R)(x)jν(R)(0)⟩=τRR16π2(δμν∂2−∂μ∂ν)1x2.(O08.1)F(b)=-\log Z(b),\qquad \langle j_\mu^{(R)}(x)j_\nu^{(R)}(0)\rangle =\frac{\tau_{RR}}{16\pi^2} (\delta_{\mu\nu}\partial^2-\partial_\mu\partial_\nu)\frac1{x^2}. \tag{O08.1}

The second equation fixes the charge and coefficient convention. It first holds at separated points; a distributional extension is needed to integrate it. For a nonzero physical current, unitarity gives τRR>0\tau_{RR}>0. Take the continuous logarithm near the round background. Its real part is −log⁡∣Z∣-\log|Z| and does not depend on a logarithm branch.

The prescription is the conformal, supersymmetric source prescription of P: power divergences are removed consistently with its Ward identities, while allowed finite background Chern–Simons terms retain their prescribed global meaning. We do not add arbitrary finite terms with new mass scales. This restriction matters when we take a real part.

Set the round radius to one, so all coordinates below are dimensionless. Let g0g_0 be the round metric and v0v_0 the unit Hopf one-form, with the orientation chosen so that dv0=2∗0v0dv_0=2*_0v_0. Introduce

h=b+b−12,d=b−b−1,b>0,h2−1=d24.h=\frac{b+b^{-1}}2,\qquad d=b-b^{-1},\qquad b>0, \qquad h^2-1=\frac{d^2}{4}.

The full background of P (5.11), (8.4)–(8.5) can be written

gb=g0+(h2−1)v0⊗v0,vb=hv0,A=V=dhv0,C=id2v0,H=ih.(O08.2)g_b=g_0+(h^2-1)v_0\otimes v_0,\qquad v_b=h v_0, \qquad A=V=dhv_0,\qquad C=\frac{id}{2}v_0,\qquad H=ih. \tag{O08.2}

Here vbv_b has unit norm in gbg_b. The field AA is the background R-connection; V,H,CV,H,C are its rigid-supergravity companions, with V=−i∗bdCV=-i*_b dC. They are fixed sources, not dynamical gauge fields. Indeed ∗bdv0=2hv0*_b dv_0=2h v_0 verifies that dual relation. The metric and A,VA,V are real, while C,HC,H are imaginary. Restoring radius ℓ\ell multiplies the metric by ℓ2\ell^2, replaces HH by ih/ℓih/\ell and CC by iℓdv0/2i\ell d v_0/2, and leaves the displayed connection one-forms A,VA,V unchanged. Their orthonormal components have mass dimension one.

This family has H=+iH=+i at b=1b=1. Earlier round-sphere examples used the other Killing-spinor branch, H=−i/ℓH=-i/\ell. We use the source’s positive branch throughout this calculation; retaining the old value of HH while varying (O08.2) would not specify this family. Its round metric still has the paper’s scalar curvature R=−6R=-6.

For b=1+ϵb=1+\epsilon,

h=1+ϵ22+O(ϵ3),d=2ϵ−ϵ2+O(ϵ3),gb=g0+ϵ2v0⊗v0+O(ϵ3).h=1+\frac{\epsilon^2}{2}+O(\epsilon^3),\quad d=2\epsilon-\epsilon^2+O(\epsilon^3),\quad g_b=g_0+\epsilon^2v_0\otimes v_0+O(\epsilon^3).

Thus the metric and HH have no first derivative. The actual first-order source is

A−32V=−ϵv0+O(ϵ2),C=iϵv0+O(ϵ2),S′(1)=∫S3 ⁣g0 v0μ(ij(Z)μ−j(R)μ).(O08.3)A-\frac32V=-\epsilon v_0+O(\epsilon^2),\qquad C=i\epsilon v_0+O(\epsilon^2),\qquad S'(1)=\int_{S^3}\!\sqrt{g_0}\,v_{0\mu} \bigl(ij^{(Z)\mu}-j^{(R)\mu}\bigr). \tag{O08.3}

The source for the R-current is A−3V/2A-3V/2, not the matter covariant derivative’s connection A−V/2A-V/2. The operator j(Z)j^{(Z)} belongs to the R-multiplet. In the SCFT with its superconformal improvement it is redundant: its separated-point correlators vanish. Its contact terms must still be considered. These are precisely the source identifications in P (8.6)–(8.8).

Turn a derivative into an integrated correlator

Section titled “Turn a derivative into an integrated correlator”

Differentiating the path integral with its complete action gives

F′=⟨S′⟩,F′′=⟨S′′⟩−⟨S′S′⟩c.(O08.4)F'=\langle S'\rangle,\qquad F''=\langle S''\rangle-\langle S'S'\rangle_c. \tag{O08.4}

The second term has a minus sign because the weight is e−Se^{-S}. The first term includes the second-order source variation and terms from differentiating the action twice, often called seagull terms. Omitting it before specifying the regulator can change the answer.

Conformal mapping from the flat vacuum makes the noncontact one-point functions vanish on the round sphere. Accordingly Re⁡F′(1)=0\operatorname{Re}F'(1)=0, and the noncontact part of ⟨S′′⟩\langle S''\rangle vanishes in this prescription. Removing redundant separated insertions leaves

Re⁡F′′(1)=−Iren,I=∫ ⁣d3xg0(x)∫ ⁣d3yg0(y) v0μ(x)v0ν(y)⟨j(R)μ(x)j(R)ν(y)⟩.(O08.5)\operatorname{Re}F''(1)=-\mathcal I_{\rm ren},\qquad \mathcal I=\int\!d^3x\sqrt{g_0(x)}\int\!d^3y\sqrt{g_0(y)}\, v_{0\mu}(x)v_{0\nu}(y) \langle j^{(R)\mu}(x)j^{(R)\nu}(y)\rangle. \tag{O08.5}

The subscript means that the coincident singularity is treated with the Ward-preserving prescription, not that an ordinary positive integral has been assigned a finite value by declaration. We now compute it.

Use stereographic coordinates x=(x1,x2,x3)x=(x^1,x^2,x^3), ρ=∣x∣\rho=|x| and Ω=2/(1+ρ2)\Omega=2/(1+\rho^2), so g0=Ω2δg_0=\Omega^2\delta. The required Hopf form is

v0=Ω2[−x2dx1+x1dx2+1−ρ22dx3+x3(x1dx1+x2dx2+x3dx3)].(O08.6)v_0=\Omega^2\left[ -x^2dx^1+x^1dx^2+\frac{1-\rho^2}{2}dx^3 +x^3(x^1dx^1+x^2dx^2+x^3dx^3)\right]. \tag{O08.6}

It obeys g0−1(v0,v0)=1g_0^{-1}(v_0,v_0)=1, and at the origin v0=2dx3v_0=2dx^3. The subgroup of round isometries preserving this Hopf form acts transitively. We may therefore fix y=0y=0 and multiply by Vol⁡(S3)=2π2\operatorname{Vol}(S^3)=2\pi^2.

For contravariant coordinate components the current’s Weyl factor is Ω−3\Omega^{-3}. Thus the flat correlator in (O08.1) gives

⟨jμ(x)jν(0)⟩S3=τRR4π2Ω(x)3Ω(0)3δμνρ2−2xμxνρ6.(O08.7)\langle j^\mu(x)j^\nu(0)\rangle_{S^3} =\frac{\tau_{RR}}{4\pi^2\Omega(x)^3\Omega(0)^3} \frac{\delta^{\mu\nu}\rho^2-2x^\mu x^\nu}{\rho^6}. \tag{O08.7}

This is P (8.9), with chordal distance s(x,0)=Ω(x)Ω(0) ρs(x,0)=\sqrt{\Omega(x)\Omega(0)}\,\rho. Coordinate products here use δ\delta; physical tensor norms use g0g_0.

To do the contraction explicitly, note that v0μxμ=Ωx3v_{0\mu}x^\mu=\Omega x^3 and v03=Ω2[(1−ρ2)/2+(x3)2]v_{03}=\Omega^2[(1-\rho^2)/2+(x^3)^2]. Its angular average uses ⟨(x3)2⟩=ρ2/3\langle(x^3)^2\rangle=\rho^2/3. Excluding ρ<ε\rho<\varepsilon then reduces the full integral to

Iε=πτRR3∫ε∞1−3ρ2ρ2(1+ρ2)2 dρ=πτRR3[1ε+2ε1+ε2+3arctan⁡ε−3π2].(O08.8)\mathcal I_\varepsilon =\frac{\pi\tau_{RR}}3\int_\varepsilon^\infty \frac{1-3\rho^2}{\rho^2(1+\rho^2)^2}\,d\rho =\frac{\pi\tau_{RR}}3 \left[\frac1\varepsilon+\frac{2\varepsilon}{1+\varepsilon^2} +3\arctan\varepsilon-\frac{3\pi}{2}\right]. \tag{O08.8}

For example, the integrand decomposes as ρ−2−(1+ρ2)−1−4(1+ρ2)−2\rho^{-2}-(1+\rho^2)^{-1}-4(1+\rho^2)^{-2}, which checks the antiderivative and its sign. The divergence is local: it comes entirely from coincident insertions.

A hard exclusion does not preserve the current Ward identity by itself. Its restoring contact term removes πτRR/(3ε)\pi\tau_{RR}/(3\varepsilon). A finite real source-mass term cannot then be chosen freely: it would violate background gauge invariance, and a finite Maxwell term would introduce a new scale. The supersymmetric treatment of this kind of power divergence and its seagull is explained in FM (3.8) and footnote 9, the prescription cited by P’s footnote 13. We obtain

Iren=lim⁡ε→0(Iε−πτRR3ε)=−π22τRR,τRR=2π2d2Re⁡Fdb2∣b=1.(O08.9)\mathcal I_{\rm ren}= \lim_{\varepsilon\to0}\left(\mathcal I_\varepsilon- \frac{\pi\tau_{RR}}{3\varepsilon}\right) =-\frac{\pi^2}{2}\tau_{RR},\qquad \boxed{\displaystyle \tau_{RR}=\frac{2}{\pi^2} \left.\frac{d^2\operatorname{Re}F}{db^2}\right|_{b=1}}. \tag{O08.9}

The sign change after subtraction is consistent with unitarity. It is the renormalized distribution, not the unregulated cutoff integrand, which enters the response.

As a separate check, conformally map the whole integral to flat space and use the transverse distribution derived in the current lesson. With v^(p)=∫eip⋅xv(x)d3x\widehat v(p)=\int e^{ip\cdot x}v(x)d^3x, n=p/∣p∣n=p/|p| and PT=1−nnTP_T=1-nn^{\mathsf T}, differentiating the transform (1+ρ2)−2^=π2e−∣p∣\widehat{(1+\rho^2)^{-2}}=\pi^2e^{-|p|} gives

PTv^0=4π2e−∣p∣[e3−n3n+i(e3×n)],∫d3p(2π)3∣p∣ ∣PTv^0∣2=4π2.P_T\widehat v_0=4\pi^2e^{-|p|} \left[e_3-n_3n+i(e_3\mathbin{\times}n)\right],\qquad \int\frac{d^3p}{(2\pi)^3}|p|\,|P_T\widehat v_0|^2=4\pi^2.

The last equality uses ∫dΩn(1−n32)=8π/3\int d\Omega_n(1-n_3^2)=8\pi/3 and ∫0∞p3e−2pdp=3/8\int_0^\infty p^3e^{-2p}dp=3/8. The conserved Fourier kernel is −τRR∣p∣PT/8-\tau_{RR}|p|P_T/8, so it independently gives Iren=−π2τRR/2\mathcal I_{\rm ren}=-\pi^2\tau_{RR}/2 without a hard exclusion. The integral is convergent at both momentum endpoints.

Explain the real part and the limits of the statement

Section titled “Explain the real part and the limits of the statement”

Local terms in the background fields encode contact terms in the R-multiplet. P’s analysis after (8.10) establishes that their allowed finite contributions on this complete family are imaginary. The real second derivative therefore isolates the separated coefficient. This is an input about supersymmetry, the source prescription and reality conditions, not a claim that every real response on every background is independent of local terms.

The result has no residual radius: FF, bb and τRR\tau_{RR} are dimensionless, and restoring ℓ\ell cancels between volumes, current factors and normalized sources. It is exact at the round point, with no large-rank or weak-coupling approximation. Localization is a possible way to compute FF; the response derivation itself used current correlators.

F-maximization selects the physical R-current before this measurement, subject to its usual accidental-symmetry qualifications. It does not say that bb should maximize FF. Here Re⁡F′′(1)>0\operatorname{Re}F''(1)>0: the round point is a local minimum along this particular background direction. Changing a trial R-current, turning on an extra flavor source, or varying only the metric changes the problem.

The remaining practical question is how to obtain the same coefficient by differentiating an actual localized determinant. The free-chiral calculation provides that next test; the result above explains which observable such a differentiation must reproduce.

Set u=log⁡bu=\log b, so h=cosh⁡uh=\cosh u. Express the leading real response in uu and in h−1h-1. Is dh2Re⁡Fd_h^2\operatorname{Re}F at h=1h=1 the coefficient in (O08.9)? Explain why the metric alone does not distinguish the two signs of uu.

Hint 1

For a regular reparameterization, use the chain rule and Re⁡F′(1)=0\operatorname{Re}F'(1)=0. Here db/du=1db/du=1 at u=0u=0.

Hint 2

The metric depends on h2−1h^2-1, whereas A,V,CA,V,C also depend on d=2sinh⁡ud=2\sinh u. The map from uu to hh has zero first derivative at the round point.

Solution

Writing F0=Re⁡F(1)F_0=\operatorname{Re}F(1), (O08.9) gives

Re⁡F(eu)=F0+π2τRR4u2+O(u3),h−1=u22+O(u4).\operatorname{Re}F(e^u)=F_0+\frac{\pi^2\tau_{RR}}4u^2+O(u^3), \qquad h-1=\frac{u^2}{2}+O(u^4).

Hence along either local branch Re⁡F=F0+(π2τRR/2)(h−1)+O((h−1)3/2)\operatorname{Re}F=F_0+(\pi^2\tau_{RR}/2)(h-1)+O((h-1)^{3/2}). The one-sided first derivative with respect to hh has the stated coefficient. The second derivative with respect to hh is not fixed by the round-point theorem and need not even be finite without further information about higher terms. We have not assumed an exact evenness of the full answer in uu.

The metric and HH are the same at uu and −u-u, but the three one-form sources reverse sign. Thus hh labels the metric but is not a regular signed parameter for the complete background near u=0u=0. For a regular parameter tt with b(0)=1b(0)=1, the measurable Hessian instead transforms as ∂t2Re⁡F∣0=[b′(0)]2π2τRR/2\partial_t^2\operatorname{Re}F|_0=[b'(0)]^2\pi^2\tau_{RR}/2.

2. Check the subtraction with physical distance

Section titled “2. Check the subtraction with physical distance”

Replace the coordinate exclusion in (O08.8) by a geodesic ball of radius δ\delta on the unit sphere. Show that ε=tan⁡(δ/2)\varepsilon=\tan(\delta/2), find the divergent term, and verify that the finite answer is unchanged. Estimate the leading error after subtraction at small δ\delta.

Hint 1

Along a radial line the proper length element is 2 dρ/(1+ρ2)2\,d\rho/(1+\rho^2).

Hint 2

Use 2ε/(1+ε2)=sin⁡δ2\varepsilon/(1+\varepsilon^2)=\sin\delta and arctan⁡ε=δ/2\arctan\varepsilon=\delta/2. Expand cot⁡(δ/2)\cot(\delta/2) before extracting a constant.

Solution

The radial integral gives δ=2arctan⁡ε\delta=2\arctan\varepsilon, so

Iδ=πτRR3[cot⁡δ2+sin⁡δ+3δ2−3π2].\mathcal I_\delta=\frac{\pi\tau_{RR}}3 \left[\cot\frac\delta2+\sin\delta+\frac{3\delta}{2} -\frac{3\pi}{2}\right].

The required divergence is 2πτRR/(3δ)2\pi\tau_{RR}/(3\delta). Since cot⁡(δ/2)=2/δ−δ/6+O(δ3)\cot(\delta/2)=2/\delta-\delta/6+O(\delta^3),

Iδ−2πτRR3δ=−π2τRR2+7πτRR9δ+O(δ3).\mathcal I_\delta-\frac{2\pi\tau_{RR}}{3\delta} =-\frac{\pi^2\tau_{RR}}2+\frac{7\pi\tau_{RR}}9\delta+O(\delta^3).

The finite coefficient agrees. Halving a sufficiently small cutoff halves the leading residual; the unsubtracted integral does not converge. Restoring a radius ℓ\ell replaces δ\delta by physical distance divided by ℓ\ell, so the finite response remains dimensionless. This checks a controlled change of cutoff, not permission to add arbitrary finite counterterms.

3. Diagnose a different subtraction prescription

Section titled “3. Diagnose a different subtraction prescription”

A calculation adds ΔF=c(4M)−1∫g fμνfμν\Delta F=c(4M)^{-1}\int\sqrt g\, f_{\mu\nu}f^{\mu\nu}, where a=A−3V/2a=A-3V/2, f=daf=da, cc is real and dimensionless, and MM is a fixed positive mass. Find its effect on the round second derivative at radius ℓ\ell. Can taking a real part remove it? Is this a counterexample to (O08.9)?

Hint 1

At first order a=−ϵv0a=-\epsilon v_0, while dv0=2∗0v0dv_0=2*_0v_0 on the unit sphere. Metric corrections start at order ϵ2\epsilon^2 and multiply an already quadratic field strength.

Hint 2

The norm of a two-form is ∣f∣2=fμνfμν/2|f|^2=f_{\mu\nu}f^{\mu\nu}/2. Restoring the radius gives two inverse metrics and one volume factor.

Solution

The unit-radius form has ∣dv0∣2=4|dv_0|^2=4, hence fμνfμν=8ϵ2+O(ϵ3)f_{\mu\nu}f^{\mu\nu}=8\epsilon^2+O(\epsilon^3). The volume is 2π22\pi^2, and the radius dependence is ℓ3−4=ℓ−1\ell^{3-4}=\ell^{-1}. Therefore

ΔF=4π2cMℓϵ2+O(ϵ3),Δ ⁣[∂b2Re⁡F]b=1=8π2cMℓ.\Delta F=\frac{4\pi^2c}{M\ell}\epsilon^2+O(\epsilon^3),\qquad \Delta\!\left[\partial_b^2\operatorname{Re}F\right]_{b=1} =\frac{8\pi^2c}{M\ell}.

This change is real, so taking a real part does not remove it. The new mass scale and the chosen Maxwell subtraction lie outside the conformal supersymmetric prescription in the theorem; the displayed term alone is not asserted to be its supersymmetric completion. It is a diagnostic of a changed source functional, not a contradiction. Its radius dependence also exposes the difference from the dimensionless universal coefficient. Finite imaginary contact contributions within the prescribed family require a different analysis and do not change (O08.9).

Reproduce the free-chiral response now calculates this curvature directly from the matter spectrum. Follow the fixed R-charge through the changing eigenvalues, then compare a convergent integral with a carefully subtracted spectral sum.