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Spinor and curvature conventions

Use this page to identify the convention package before moving an index, continuing an action, or importing a curvature coupling. The three-dimensional formulas follow Closset–Dumitrescu–Festuccia–Komargodski, arXiv:1212.3388v3. The four-dimensional Lorentzian spinor matrices follow Bilal, hep-th/0101055v1, with the volume-orientation translation stated below. The Euclidean continuations are the explicitly derived choices used in the linked lessons.

For an introduction, start with three-dimensional spinors or the independent four-dimensional Weyl-spinor lesson. The curvature calculation belongs to the round-sphere geometry lesson.

SettingMetric and coordinate labelsSpinor representation used here
Three-dimensional Euclideanδab\delta_{ab}, a=1,2,3a=1,2,3Two-component lower columns; both partner spinors transform under Spin⁡(3)=SU(2)\operatorname{Spin}(3)=SU(2)
Three-dimensional Lorentzian continuation exampleημν=diag⁡(1,−1,−1)\eta_{\mu\nu}=\operatorname{diag}(1,-1,-1), μ=0,1,2\mu=0,1,2Two-component Dirac column and its Lorentzian adjoint row
Four-dimensional Lorentzianημν=diag⁡(1,−1,−1,−1)\eta_{\mu\nu}=\operatorname{diag}(1,-1,-1,-1), μ=0,1,2,3\mu=0,1,2,3Undotted Weyl column and its dotted conjugate representation
Four-dimensional Euclidean continuationδab\delta_{ab}, a=1,2,3,4a=1,2,3,4Independent chiral sectors of SU(2)L×SU(2)RSU(2)_L\times SU(2)_R

These are kinematic choices. A curved background’s preserved supersymmetries require solving its spinor equations. The parent counts are four real Lorentzian Poincaré supercharges for both 3d N=23d\ \mathcal N=2 and 4d N=14d\ \mathcal N=1. Complexifying their variables does not change that count into eight real Lorentzian generators.

Let the ordinary Pauli matrices be

τ1=(0110),τ2=(0−ii0),τ3=(100−1).\tau_1=\begin{pmatrix}0&1\\1&0\end{pmatrix},\qquad \tau_2=\begin{pmatrix}0&-i\\i&0\end{pmatrix},\qquad \tau_3=\begin{pmatrix}1&0\\0&-1\end{pmatrix}.

Use the following matrices with the indicated index placements:

ObjectThree-dimensional Euclidean packageFour-dimensional Lorentzian package
Vector matrices(γa)αβ=(τ3,−τ1,−τ2)(\gamma^a)_\alpha{}^\beta=(\tau_3,-\tau_1,-\tau_2)σαα˙μ=(I,−τi)\sigma^\mu_{\alpha\dot\alpha}=(I,-\tau_i)
Partner matrixThe same γa\gamma^a acts on either lower-column spinorσˉμα˙α=(I,+τi)\bar\sigma^{\mu\dot\alpha\alpha}=(I,+\tau_i)
Clifford identity{γa,γb}=2δabI\{\gamma^a,\gamma^b\}=2\delta^{ab}Iσμσˉν+σνσˉμ=2ημνI\sigma^\mu\bar\sigma^\nu+\sigma^\nu\bar\sigma^\mu=2\eta^{\mu\nu}I
Orientation-sensitive identityγaγb=δabI+iϵabcγc\gamma^a\gamma^b=\delta^{ab}I+i\epsilon^{abc}\gamma_c, ϵ123=1\epsilon^{123}=1The ordered products use the displayed sigma pair and the Lorentz metric
Undotted scalar contractionψχ=ψαχα\psi\chi=\psi^\alpha\chi_\alphaψχ=ψαχα\psi\chi=\psi^\alpha\chi_\alpha
Other scalar contractionψ~χ=ψ~αχα\widetilde\psi\chi=\widetilde\psi^\alpha\chi_\alpha; no dotted indexψˉχˉ=ψˉα˙χˉα˙\bar\psi\bar\chi=\bar\psi_{\dot\alpha}\bar\chi^{\dot\alpha}

The explicit raising and lowering matrices are the same numerical matrices in these two packages:

(ϵαβ)=(01−10),(ϵαβ)=(0−110)≡C,ψα=ϵαβψβ.(\epsilon^{\alpha\beta})= \begin{pmatrix}0&1\\-1&0\end{pmatrix},\qquad (\epsilon_{\alpha\beta})= \begin{pmatrix}0&-1\\1&0\end{pmatrix}\equiv C, \qquad \psi^\alpha=\epsilon^{\alpha\beta}\psi_\beta .

The four-dimensional dotted tensors have the same entries. Thus ψ1=ψ2\psi^1=\psi_2, ψ2=−ψ1\psi^2=-\psi_1, and ψχ=ψTCχ\psi\chi=\psi^TC\chi for lower undotted columns. Raising an index is a linear contraction, whereas complex conjugation is an antilinear operation.

In four dimensions the barred sigma matrix means

σˉμα˙α=ϵα˙β˙ϵαβσββ˙μ.\bar\sigma^{\mu\dot\alpha\alpha} =\epsilon^{\dot\alpha\dot\beta}\epsilon^{\alpha\beta} \sigma^\mu_{\beta\dot\beta}.

Its bar specifies the other index placement. Entrywise conjugation is a different operation. In particular, the four-dimensional sigma pair connects two chiral index spaces; it cannot be substituted into a three-dimensional identity involving one mixed-index gamma matrix. P, (A.1)–(A.4); Bilal, (2.9)–(2.16).

For spinors of definite Grassmann parity pu,pvp_u,p_v, the three-dimensional contractions obey

uv=−(−1)pupvvu,uγav=(−1)pupvvγau.uv=-(-1)^{p_up_v}vu,\qquad u\gamma^a v=(-1)^{p_up_v}v\gamma^a u.

Consequently an odd ψ\psi has ψψ=−2ψ1ψ2\psi\psi=-2\psi_1\psi_2, while a commuting ζ\zeta has ζζ=0\zeta\zeta=0. The undotted four-dimensional scalar contraction has the same parity rule. Its dotted contraction uses the reversed index placement displayed in the table. Adjoint conjugation reverses the order of odd factors.

For the four-dimensional volume tensor, choose ϵ0123=+1\epsilon_{0123}=+1, hence ϵ0123=−1\epsilon^{0123}=-1 in Lorentzian signature, and ϵ1234=+1\epsilon_{1234}=+1 after Euclidean continuation. Define f~μν=ϵμνρσfρσ/2\widetilde f^{\mu\nu}=\epsilon^{\mu\nu\rho\sigma}f_{\rho\sigma}/2. With the displayed Weyl matrices, the bosonic chiral coefficient is [WαWα]θ2=D2−fμνfμν/2+ifμνf~μν/2[W^\alpha W_\alpha]_{\theta^2}=D^2-f_{\mu\nu}f^{\mu\nu}/2 +if_{\mu\nu}\widetilde f^{\mu\nu}/2. This requires a translation of the upper-epsilon sign printed beside Bilal (4.49): for f03=E,f12=Bf_{03}=E,f_{12}=B, direct matrix multiplication gives D2+E2−B2−2iEBD^2+E^2-B^2-2iEB. Under x0=−ix4x^0=-ix^4 and v0=iv4v_0=iv_4, the dual contraction continues as fLf~L=ifEf~Ef_L\widetilde f_L=i f_E\widetilde f_E. A positive Lorentzian theta coefficient consequently becomes the negative imaginary Euclidean coefficient in the action. The prepotential lesson derives the corresponding scalar and photon coefficients.

In three dimensions,

γ1γ2=(0−110)=iγ3,γ2γ1=−iγ3.\gamma^1\gamma^2 =\begin{pmatrix}0&-1\\1&0\end{pmatrix} =i\gamma^3,\qquad \gamma^2\gamma^1=-i\gamma^3.

The anticommutator vanishes, and γ1γ2γ3=iI\gamma^1\gamma^2\gamma^3=iI fixes the orientation sign. In the four-dimensional Lorentzian package,

σ1σˉ1=(−τ1)(+τ1)=−I,σ0σˉi+σiσˉ0=τi−τi=0.\sigma^1\bar\sigma^1=(-\tau_1)(+\tau_1)=-I, \qquad \sigma^0\bar\sigma^i+\sigma^i\bar\sigma^0=\tau_i-\tau_i=0.

The first result is the spatial metric sign. Multiplying σ1\sigma^1 by itself instead would give +I+I and would be the wrong index contraction for this Clifford identity. The complete derivations and rearrangement identities are in the three-dimensional spinor lesson and four-dimensional Weyl-spinor lesson.

Continuation and normalization dictionaries

Section titled “Continuation and normalization dictionaries”

The following choices include the coordinate order and every spatial factor of ii.

ItemThree-dimensional continuationFour-dimensional continuation
Time rotationt=−iτt=-i\taux0=−ix4x^0=-ix^4
Euclidean coordinate order(xE1,xE2,xE3)=(τ,x,y)(x_E^1,x_E^2,x_E^3)=(\tau,x,y)(xE1,xE2,xE3,xE4)=(x1,x2,x3,x4)(x_E^1,x_E^2,x_E^3,x_E^4)=(x^1,x^2,x^3,x^4)
Lorentzian matricesΓ0=γ1\Gamma^0=\gamma^1, Γ1=iγ2\Gamma^1=i\gamma^2, Γ2=iγ3\Gamma^2=i\gamma^3γLμ=(0σμσˉμ0)\gamma_L^\mu=\begin{pmatrix}0&\sigma^\mu\\\bar\sigma^\mu&0\end{pmatrix}
Euclidean matricesThe γa\gamma^a aboveγE4=γL0\gamma_E^4=\gamma_L^0, γEi=−iγLi\gamma_E^i=-i\gamma_L^i
Continued derivativeΓμ∂μ→iγa∂a\Gamma^\mu\partial_\mu\to i\gamma^a\partial_aγLμ∂μ→iγEa∂a\gamma_L^\mu\partial_\mu\to i\gamma_E^a\partial_a

The four-dimensional Euclidean chiral blocks are therefore

σEa=(iτ1,iτ2,iτ3,I),σˉEa=(−iτ1,−iτ2,−iτ3,I).\sigma_E^a=(i\tau_1,i\tau_2,i\tau_3,I),\qquad \bar\sigma_E^a=(-i\tau_1,-i\tau_2,-i\tau_3,I).

They satisfy the sigma-pair identity with δab\delta^{ab}. The Lorentzian blocks are Bilal’s (2.16); this Euclidean pair is the site’s derived continuation. See the four-dimensional continuation for its independent-chirality test.

In the three-dimensional example, ψˉL=ψL†Γ0\bar\psi_L=\psi_L^\dagger\Gamma^0. Its continued row χE\chi_E is independent of the column ψE\psi_E:

∫d3xL ψˉL(iΓμ∂μ−m)ψL ⟶ i∫d3xE χE(γa∂a+m)ψE.\int d^3x_L\,\bar\psi_L(i\Gamma^\mu\partial_\mu-m)\psi_L \ \longrightarrow\ i\int d^3x_E\,\chi_E(\gamma^a\partial_a+m)\psi_E.

Thus eiSLe^{iS_L} becomes e−SEe^{-S_E} with this prescription. The continuation lesson derives the action and vector-bilinear factors.

To match that lesson’s kinetic normalization to the three-manifold paper’s −iψ~Pγμ∇μψP-i\widetilde\psi_P\gamma^\mu\nabla_\mu\psi_P, use

ψE=ψP,χE=−i ψ~P TC.\psi_E=\psi_P,\qquad \chi_E=-i\,\widetilde\psi_P^{\,T}C.

The extra phase is required by the action coefficient. The contraction-only definition χE=ψ~E TC\chi_E=\widetilde\psi_E^{\,T}C instead gives ψ~E=−iψ~P\widetilde\psi_E=-i\widetilde\psi_P. An action’s interaction coefficients and transformations must be translated along with that field redefinition. Free-action normalization dictionary; P, (6.32).

Distinguish a momentum eigenvalue on a c-number mode from the action of a translation generator on a field. The positive-frequency mode obeys

i∂μe−ip⋅x=pμe−ip⋅x,[Pμ,Φ(x)]=−i∂μΦ(x).i\partial_\mu e^{-ip\cdot x}=p_\mu e^{-ip\cdot x}, \qquad [P_\mu,\Phi(x)]=-i\partial_\mu\Phi(x).

The second equation states the field-adjoint action. Bilal’s superspace differential representation also uses Pμ=−i∂μP_\mu=-i\partial_\mu, as does the site’s three-dimensional component convention. These contexts must be identified before comparing signs; the mode calculation is not a different dimension-dependent choice of physical translation generator. The Lorentzian relation Qˉ=Q†\bar Q=Q^\dagger remains fixed. Bilal, (4.10).

Euclidean partner variables, a Hermitian conjugate, and an integration contour serve different purposes. For example, the three-dimensional antilinear spin map Jψ=Cψ∗\mathcal J\psi=C\psi^* satisfies J2=−1\mathcal J^2=-1, so it does not define a nonzero single-spinor Majorana condition. In four Euclidean dimensions the two chiral sectors transform under independently chosen SU(2)SU(2) factors. Their independence does not supply a bosonic path-integral contour. These statements concern complexified kinematics, before specifying a quantum integration prescription.

Let eae^a be an orthonormal coframe, EaE_a its dual frame, and ∇Eb=ΩabEa\nabla E_b=\Omega^a{}_b E_a. The torsion-free and curvature equations are

dea+Ωab∧eb=0,Rab=dΩab+Ωac∧Ωcb.de^a+\Omega^a{}_b\wedge e^b=0,\qquad \mathcal R^a{}_b=d\Omega^a{}_b+\Omega^a{}_c\wedge\Omega^c{}_b.

The three-manifold paper puts the input frame index first:

ωμab=Ωμba,Rba=12Rμνab dxμ∧dxν.\omega_{\mu a}{}^b=\Omega_\mu{}^b{}_a,\qquad \mathcal R^b{}_a=\frac12R_{\mu\nu a}{}^b\,dx^\mu\wedge dx^\nu.

With Euclidean frame indices lowered, ωμab=−Ωμab\omega_{\mu ab}=-\Omega_{\mu ab}. Its spinor derivative is

∇μψ=(∂μ+14Ωμabγaγb)ψ=(∂μ−i4ωμabϵabcγc)ψ.\nabla_\mu\psi =\left(\partial_\mu+\frac14\Omega_{\mu ab}\gamma^a\gamma^b\right)\psi =\left(\partial_\mu-\frac i4\omega_{\mu ab}\epsilon^{abc}\gamma_c\right)\psi.

These are the same connection in two index arrangements. The source definitions are P, (A.8)–(A.11); their derivation is in covariant spinor derivatives.

For the global oriented sphere frame of radius ℓ\ell,

dea=1ℓϵabceb∧ec,Ωab=1ℓϵabcec,Rab=1ℓ2ea∧eb.de^a=\frac1\ell\epsilon_{abc}e^b\wedge e^c,\qquad \Omega_{ab}=\frac1\ell\epsilon_{abc}e^c,\qquad \mathcal R^a{}_b=\frac1{\ell^2}e^a\wedge e^b.

The compact structure equation sums both orders of b,cb,c; in particular de1=2e2∧e3/ℓde^1=2e^2\wedge e^3/\ell. The source curvature components and trace are

Rcdab=δcbδda−δdbδcaℓ2,Rab=∑c=13Racbc=1−3ℓ2δab.R_{cd a}{}^b =\frac{\delta_c^b\delta_{da}-\delta_d^b\delta_{ca}}{\ell^2}, \qquad R_{ab}=\sum_{c=1}^3R_{ac b}{}^c =\frac{1-3}{\ell^2}\delta_{ab}.

Consequently,

Rab=−2ℓ2δab,R=−6ℓ2.\boxed{R_{ab}=-\frac2{\ell^2}\delta_{ab},\qquad R=-\frac6{\ell^2}.}

This verifies the scalar sign using the declared contraction. A convention that contracts this same commutator tensor with the first two indices reversed gives R+=+6/ℓ2R_+=+6/\ell^2. If RP=−R+R_P=-R_+, an action coefficient must also change sign when translated:

cPRP=c+R+,c+=−cP.c_P R_P=c_+R_+,\qquad c_+=-c_P.

For example, the conformal free-chiral coefficient is −RP/8=+R+/8=3/(4ℓ2)-R_P/8=+R_+/8=3/(4\ell^2). The numerical curvature sign alone is insufficient to translate an action.

The same sphere frame gives ∇a=Ea+iγa/(2ℓ)\nabla_a=E_a+i\gamma_a/(2\ell) on spinors. The rigid background A=V=C=0A=V=C=0, H=−i/ℓH=-i/\ell then admits constant-component solutions of ∇aζ=iγaζ/(2ℓ)\nabla_a\zeta=i\gamma_a\zeta/(2\ell). The sphere solution supplies the complete background and global argument. Curvature by itself does not fix that source choice.

The curvature entries above belong to a three-dimensional sphere and P’s exact trace convention. A four-dimensional source must state its own curvature definition before its couplings are compared. A one-dimensional quantum-mechanics model likewise specifies its time algebra and fermionic variables directly; the spatial Clifford triples here are not a prerequisite for that setting.

In component supersymmetry calculations, keep parameter parity explicit as well. The three-dimensional lessons use commuting labels multiplying odd operations δ\delta; a physical even variation is Δ=ρδ\Delta=\rho\delta with an independent odd parameter ρ\rho. When comparing an odd-parameter component formula, translate the graded and ordinary product rules with the parameters. The matrix and curvature identities in this reference do not change that bookkeeping.