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Paper guide: Appendices C and D, four-dimensional origin

Why does a three-dimensional R-charged field see both a shifted connection and the combination z−rHz-rH? Appendices C and D of Supersymmetric Field Theories on Three-Manifolds, version 3 answer this by reducing a four-dimensional construction. The calculation is particularly useful for finding missing signs: a single four-dimensional derivative must account for both terms.

Read the four-dimensional new minimal background and twisted dimensional reduction first. Those lessons derive the background equation and complete reduction. This guide supplies a reading order, separates the paper’s overlapping notation, and changes one geometric assumption to test the argument’s limits.

The parent theory has four-dimensional N=1\mathcal N=1 supersymmetry, or four real Poincaré generators. Its three-dimensional description has N=2\mathcal N=2, also four real generators. Euclidean spinors of opposite chirality are independent complex fields; their complex solution count does not add physical supercharges. The construction does not specify a dynamical gauge group or rank. A chosen background can preserve fewer generators.

Read the background before the component table

Section titled “Read the background before the component table”

Start with (C.1), not the long transformation table. A rigid background consists of a metric, an R connection and a conserved auxiliary vector. Its sources are fixed, and its gravitino variation must vanish. They are not required to solve gravitational equations of motion. A conserved continuous R-symmetry admitting the appropriate current multiplet is an input. Festuccia–Seiberg, section 2 and section 6

Then read Appendix D in three passes: geometry in D.1, spinor equations in D.2, and multiplets in D.3. The following map covers all numbered equations. Site equation labels identify the relevant calculation inside the linked teaching home.

Paper landmarkQuestion it answersCanonical calculation
(C.1)Which fixed sources preserve a spinor?New minimal equations, (B02.4)–(B02.5).
(C.2)–(C.3)What transforms, and which algebra closes?Twisted reduction, (B03.12)–(B03.15); read the component dictionary before applying the table.
(D.1)–(D.2)Which direction is removed, and how are dotted indices identified?Twisted reduction, (B03.4) and its frame discussion.
(D.3)–(D.7)How do the metric, frame and horizontal components reduce?Twisted reduction, (B03.1)–(B03.2), (B03.5).
(D.8)–(D.11)Where do central charge, spin rotations and curvature terms come from?Twisted reduction, (B03.3), (B03.6), and the curvature check following (B03.14).
(D.12)–(D.16)Which source identification avoids an extra spinor projection?Reduction source dictionary, (B03.7)–(B03.9).
(D.17)–(D.18)Which three-dimensional fields and derivatives enter the transformations?Twisted reduction, (B03.12)–(B03.14).
(D.19)How does translation along the fiber become a central transformation?Twisted reduction, (B03.15).

The source’s (D.14) is a sufficient choice that makes the vertical equation an identity in the spinor. It is not a classification of every background preserving one selected spinor. Also, the reduction retains spinors independent of the fiber coordinate in the stated frame. A fiber-dependent four-dimensional solution is not automatically retained.

The transformations in (C.3) and (D.19) are odd operations labeled by commuting spinors, as in the teaching lessons. Their bracket is an anticommutator. Multiplying by external odd parameters gives ordinary even variations with a correspondingly translated commutator; one must not change the bracket while keeping its parameter signs unchanged.

Write four-dimensional background sources as A,V\mathcal A,\mathcal V, and the three-dimensional ones as A,V,H,CA,V,H,C. Write the vector component of a general matter multiplet as BM\mathcal B_M; it is not the background R connection. Denote the multiplet’s bottom scalar by XX.

Printed symbol and contextMeaning here
AM,VMA_M,V_M in (C.1)Background AM,VM\mathcal A_M,\mathcal V_M.
C,AM,DC,A_M,D in the multiplet of (C.2)Matter components X,BM,DX,\mathcal B_M,\mathcal D.
cμ,vμ,aμc_\mu,v_\mu,a_\mu in D.1–D.2Backgrounds Cμ,Vμ,AμC_\mu,V_\mu,A_\mu.
aμ,σ,D(3)a_\mu,\sigma,D^{(3)} in D.3Matter components bμ=Bμ−CμByb_\mu=\mathcal B_\mu-C_\mu\mathcal B_y, σ=By\sigma=\mathcal B_y, D=D−HσD=\mathcal D-H\sigma.
Dμ(3)D_\mu^{(3)} acting on a component of R-charge qq∇μ−iq(Aμ−Vμ/2)−izCμ\nabla_\mu-iq(A_\mu-V_\mu/2)-izC_\mu.

The paper also uses a different one-index sigma package from the positive Euclidean blocks in the four-dimensional lesson: σP=−is\sigma_P=-is, σ~P=−is~\widetilde\sigma_P=-i\widetilde s. Consequently its two-index matrices equal minus the site’s Σ,Σ~\Sigma,\widetilde\Sigma. Its input-first frame connection equals minus the ordinary Cartan connection, so the two signs cancel in the spin derivative. Use the dotted-column conversion in the reduction lesson as well; replacing a dotted index by an undotted one without that conversion loses signs in (D.17).

The reduction direction is frame direction 22 in the four-dimensional ordering (x1,y,x2,x3)(x^1,y,x^2,x^3). Keep this ordering when using epsilon tensors. Curvature has the paper’s sign, negative on a round sphere. Euclidean bilinears such as VμVμV_\mu V^\mu contain no complex conjugation.

Finally, the four-dimensional two-form potential is distinct from the metric connection CC. The four-dimensional lesson uses VM=εMNPQ∂NBPQ/2\mathcal V^M=\varepsilon^{MNPQ}\partial_N B_{PQ}/2; Festuccia–Seiberg print coefficient 1/41/4. Equal V\mathcal V therefore requires BFS=2BB_{\rm FS}=2B in these conventions. Neither this normalization nor the local reduction assigns a compact two-form charge lattice.

Take the paper’s unit-fiber metric and write its source dictionary as one-forms:

ds42=gμνdxμdxν+θ2,θ=dy+C,A=A−12V+Hθ,V=12V+Hθ,V=−i∗3dC.(PC09.1)\begin{gathered} ds_4^2=g_{\mu\nu}dx^\mu dx^\nu+\theta^2,\qquad \theta=dy+C,\\ \mathcal A=A-\frac12V+H\theta,\qquad \mathcal V=\frac12V+H\theta,\qquad V=-i*_3dC. \end{gathered} \tag{PC09.1}

The horizontal vector is Eμ=∂μ−Cμ∂yE_\mu=\partial_\mu-C_\mu\partial_y. Thus A(Eμ)=Aμ−Vμ/2\mathcal A(E_\mu)=A_\mu-V_\mu/2, whereas the coordinate component is Aμ=Aμ−Vμ/2+HCμ\mathcal A_\mu=A_\mu-V_\mu/2+HC_\mu. This distinction is compressed into (D.16) by the preceding vector-reduction rules.

For a scalar component of R-charge qq, let Φ(x,y)=eizyϕ(x)\Phi(x,y)=e^{izy}\phi(x) and DM=∂M−iqAM\mathscr D_M=\partial_M-iq\mathcal A_M. Direct subtraction gives

e−izyDyΦ=i(z−qH)ϕ,e−izy(Dμ−CμDy)Φ=[∂μ−iq(Aμ−Vμ/2+HCμ)−iCμ(z−qH)]ϕ=[∂μ−iq(Aμ−Vμ/2)−izCμ]ϕ.(PC09.2)\begin{aligned} e^{-izy}\mathscr D_y\Phi&=i(z-qH)\phi,\\ e^{-izy}(\mathscr D_\mu-C_\mu\mathscr D_y)\Phi &=\left[\partial_\mu-iq(A_\mu-V_\mu/2+HC_\mu) -iC_\mu(z-qH)\right]\phi\\ &=\left[\partial_\mu-iq(A_\mu-V_\mu/2)-izC_\mu\right]\phi . \end{aligned} \tag{PC09.2}

The HCμHC_\mu terms cancel. Using the coordinate component as a horizontal one would retain a spurious term. For the bottom field, q=rq=r, and the vertical line supplies precisely the combination z−rHz-rH in (D.17) and (D.19). For spinors, (D.9) adds the frame-rotation terms; the scalar calculation is not a substitute for them.

Here coordinates have length units, [Aμ]=[Vμ]=[H]=[z]=1[A_\mu]=[V_\mu]=[H]=[z]=1, [Cμ]=0[C_\mu]=0, and qq is dimensionless. This also distinguishes CC from an ordinarily normalized compact gauge connection: if yy has period 2πRf2\pi R_f, a periodic scalar has z=n/Rfz=n/R_f and couples with integer nn to C/RfC/R_f.

The connection in (PC09.2) governs matter transformations. The linearized current coupling uses j(R)μ(Aμ−3Vμ/2)j^{(R)\mu}(A_\mu-3V_\mu/2) in (2.10). These are different statements about the same sources. One cannot replace the matter connection by the current-source combination.

Use the local supersymmetric example already solved in the reduction lesson: flat base coordinates, real nonzero β\beta of dimension one, and

C=βx1dx2,V=−iβ dx3,H=β,A=−3iβ2dx3.(PC09.3)C=\beta x^1dx^2,\qquad V=-i\beta\,dx^3,\qquad H=\beta,\qquad A=-\frac{3i\beta}{2}dx^3 . \tag{PC09.3}

It has one fiber-invariant solution in each spinor sector. For a scalar of charge rr and fiber momentum zz, the four-dimensional source is A=−iβ dx3+β dy+β2x1dx2\mathcal A=-i\beta\,dx^3+\beta\,dy+\beta^2x^1dx^2. Therefore D2=∂2−irβ2x1\mathscr D_2=\partial_2-ir\beta^2x^1 and Dy=i(z−rβ)\mathscr D_y=i(z-r\beta) on the mode. Subtracting βx1Dy\beta x^1\mathscr D_y gives D2(3)=∂2−izβx1D_2^{(3)}=\partial_2-iz\beta x^1. Likewise D3(3)=∂3−rβD_3^{(3)}=\partial_3-r\beta. The R contribution cancels from the first expression, but remains in the second. The latter is a real shift produced by an imaginary Euclidean source, not a unitary momentum shift. No positive action or integration contour follows from this algebra alone.

The formal source construction does not by itself establish a quantum compactification or a real global uplift. Appendix D ends D.2 by allowing complexification of the three-dimensional graviphoton after reduction; a real four-dimensional metric initially gives real CC. Circle periods, spin structure, source holonomy and patching must still be specified globally. The retained fields and labels must have compatible boundary conditions.

There is a separate local limitation worth calculating. Replace the metric, solely as a geometric test, by

ds42=gμνdxμdxν+ρ(x)2θ2,ρ>0.(PC09.4)ds_4^2=g_{\mu\nu}dx^\mu dx^\nu+\rho(x)^2\theta^2,\qquad \rho>0. \tag{PC09.4}

The dimensionless function ρ\rho changes the proper fiber radius. The triangular coframe now gives G=ρg\sqrt G=\rho\sqrt g. For a yy-independent vector U=UμEμ+W∂y\mathcal U=U^\mu E_\mu+W\partial_y, the coordinate divergence is

∇M(4)UM=1ρg∂μ(ρg Uμ)=∇μ(3)Uμ+Uμ∂μlog⁡ρ.(PC09.5)\nabla_M^{(4)}\mathcal U^M =\frac1{\rho\sqrt g}\partial_\mu(\rho\sqrt g\,U^\mu) =\nabla_\mu^{(3)}U^\mu+U^\mu\partial_\mu\log\rho . \tag{PC09.5}

Consequently, keeping Uμ=Vμ/2U^\mu=V^\mu/2 with ∇μVμ=0\nabla_\mu V^\mu=0 no longer guarantees conservation. On the flat base of (PC09.3), choose ρ=eκx3\rho=e^{\kappa x^3}, with real κ\kappa of dimension one. The proposed conserved source would instead have divergence −iβκ/2-i\beta\kappa/2. It already fails a defining condition of Appendix C.

This diagnoses a failed reuse of (D.14), not a no-go theorem for varying-radius supersymmetric reductions. The spin connection changes too. A consistent extension would have to revisit both sources and spinor equations. The last exit calculation checks the changed measure independently using a scalar probe.

1. Which R-charge belongs in the derivative?

Section titled “1. Which R-charge belongs in the derivative?”

In (C.2), the bottom field has charge rr and ζ,ζ~\zeta,\widetilde\zeta have charges +1,−1+1,-1. Infer the charges of χ,χ~,M,M~\chi,\widetilde\chi,M,\widetilde M. All components have fiber dependence eizye^{izy}. Find the vertical scalar derivatives of X,M,M~X,M,\widetilde M, and specialize their differences to H=−i/ℓH=-i/\ell.

Hint 1

The variation preserves total R-charge. First use the two terms in δX\delta X, then δχ=ζM+⋯\delta\chi=\zeta M+\cdots.

Hint 2

The supersymmetry labels have zero fiber momentum. Central charge remains zz even when R-charge changes.

Solution

Charge conservation gives R(χ)=r−1R(\chi)=r-1, R(χ~)=r+1R(\widetilde\chi)=r+1, R(M)=r−2R(M)=r-2, R(M~)=r+2R(\widetilde M)=r+2. Equation (PC09.2) gives vertical coefficients i(z−rH)i(z-rH), i[z−(r−2)H]i[z-(r-2)H], and i[z−(r+2)H]i[z-(r+2)H]. Relative to the bottom coefficient, the last two differ by +2iH+2iH and −2iH-2iH, hence +2/ℓ+2/\ell and −2/ℓ-2/\ell on the stated sphere background.

The same symbol Dμ(3)D_\mu^{(3)} in the transformation table acts with each operand’s charge. Using the bottom charge on every component breaks R covariance. These derivative shifts are not independent mass-shell assertions.

2. Translate the auxiliary and its curvature coefficient

Section titled “2. Translate the auxiliary and its curvature coefficient”

Use the unit-fiber dictionary to reduce R−6VMVM\mathcal R-6\mathcal V_M\mathcal V^M in (C.2), where R\mathcal R is the paper’s four-dimensional Ricci scalar. Evaluate it on (PC09.3). Also find δD\delta D in terms of δD,δσ\delta\mathcal D,\delta\sigma at fixed HH. Does setting D=0D=0 follow from the field definition?

Hint 1

Equation (D.11) gives R=R3−V2/2\mathcal R=R_3-V^2/2. The horizontal and vertical parts of V\mathcal V in (PC09.1) are orthogonal.

Hint 2

Keep V2V^2 bilinear. In the worked example it equals −β2-\beta^2, not +β2+\beta^2.

Solution

Since V2=V2/4+H2\mathcal V^2=V^2/4+H^2,

R−6V2=R3−12V2−6(14V2+H2)=R3−2V2−6H2.\mathcal R-6\mathcal V^2 =R_3-\frac12V^2-6\left(\frac14V^2+H^2\right) =R_3-2V^2-6H^2.

For (PC09.3), R=β2/2\mathcal R=\beta^2/2 and V2=3β2/4\mathcal V^2=3\beta^2/4, so both forms give −4β2-4\beta^2. This checks the coefficient in (D.17), including its continuation convention.

At fixed HH, δD=δD−Hδσ\delta D=\delta\mathcal D-H\delta\sigma. This second term is essential when reducing the transformation of the auxiliary. Defining D=D−HσD=\mathcal D-H\sigma is an invertible field redefinition. Setting D=0D=0 is an additional field restriction, equivalent to D=Hσ\mathcal D=H\sigma; whether it solves an equation of motion requires an action. No such equation was used in the reduction.

In (PC09.4), take a flat base with one nonconstant coordinate xx, set C=0C=0, and let ρ=eκx\rho=e^{\kappa x}. A neutral scalar has fiber dependence einy/Rfe^{iny/R_f} and momentum kf=n/Rfk_f=n/R_f. Per unit transverse volume and per coordinate fiber length, its norm and kinetic form are

N=∫Rρ∣ϕ∣2dx,E=∫Rρ(∣ϕ′∣2+kf2ρ−2∣ϕ∣2)dx.N=\int_{\mathbb R}\rho|\phi|^2dx,\qquad E=\int_{\mathbb R}\rho\left(|\phi'|^2+k_f^2\rho^{-2}|\phi|^2\right)dx.

Set ϕ=ρ−1/2ψ\phi=\rho^{-1/2}\psi. Derive the operator acting on ψ\psi and evaluate E/NE/N for ψ=(a/π)1/4e−a(x−x0)2/2+ipx\psi=(a/\pi)^{1/4}e^{-a(x-x_0)^2/2+ipx}, with a>0a>0 and real p,x0,κp,x_0,\kappa.

Hint 1

Expand ∣ψ′−κψ/2∣2|\psi'-\kappa\psi/2|^2. Its cross term is a derivative of ∣ψ∣2|\psi|^2.

Hint 2

The normalized Gaussian has variance 1/(2a)1/(2a) and ⟨e−2κx⟩=e−2κx0+κ2/a\langle e^{-2\kappa x}\rangle=e^{-2\kappa x_0+\kappa^2/a}.

Solution

The norm becomes ∫∣ψ∣2dx\int|\psi|^2dx. Decay removes the boundary term −κ∣ψ∣2/2-\kappa|\psi|^2/2 from the energy. Thus the unitarily transformed operator and this normalized probe’s energy are

L^=−∂x2+κ24+kf2e−2κx,EN=a2+p2+κ24+kf2e−2κx0+κ2/a.\widehat L=-\partial_x^2+\frac{\kappa^2}{4} +k_f^2e^{-2\kappa x},\qquad \frac EN=\frac a2+p^2+\frac{\kappa^2}{4} +k_f^2e^{-2\kappa x_0+\kappa^2/a}.

The original weighted operator is −ρ−1∂x(ρ∂x)+kf2ρ−2-\rho^{-1}\partial_x(\rho\partial_x)+k_f^2\rho^{-2}. Its first derivative is exactly what the rescaling removes. At κ=0\kappa=0 the result reduces to the ordinary Gaussian gradient energy plus kf2k_f^2. Direct integration of the original weighted form gives the same answer for nonzero κ\kappa: in a fixed length unit, (a,x0,p,κ,n,Rf)=(1.3,0.4,0.7,0.6,2,1.7)(a,x_0,p,\kappa,n,R_f)=(1.3,0.4,0.7,0.6,2,1.7) gives E/N=2.35970996983615E/N=2.35970996983615 in inverse-square length units.

This is a Rayleigh expectation, not an asserted eigenvalue or a supersymmetric determinant. It demonstrates independently why retaining the unit-fiber measure would change the reduced theory.

Return to (D.17) with the charges, horizontal components and auxiliary shift written beside it. Then (D.19) should have a concrete interpretation: the retained four-dimensional translation splits into a three-dimensional covariant motion and a fiber-charge transformation. The canonical reduction lesson derives that algebra; global compactification and quantum matching require additional data beyond these local equations.