D'Auria-Fre formulation of supergravity




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The D’Auria-Fré formalism (D’Auria-Fré-Regge 80, D’Auria-Fré 80, Castellani-D’Auria-Fré 91) is a natural “superspace” formulation of supergravity in general dimensions, including type II supergravity and heterotic supergravity in dimension 10 as well as notably 11-dimensional supergravity.

This proceeds in generalization of how Einstein gravity in first order formulation of gravity is equivalently the Cartan geometry for the inclusion of the Lorentz group inside the Poincare group: a field configuration of the field of gravity is equivalently a Cartan connection for this subgroup inclusion.

Accordingly, low dimensional supergravity without extended supersymmetry is equivalently the super-Cartan geometry of the inclusion of the spin group into the super Poincaré group.

What D’Auria-Fré implicitly observe (not in this homotopy theoretic language though, that was developed in Sati-Schreiber-Stasheff 08, Fiorenza-Schreiber-Stasheff 10, Fiorenza-Sati-Schreiber 13) is that for higher supergravity with extended supersymmetry such as 11-dimensional supergravity with its M-theory super Lie algebra symmetry, the description of the fields is in the higher differential geometry version of Cartan geometry, namely higher Cartan geometry, where the super Poincare Lie algebra is replaced by one of its exceptional super Lie n-algebra extensions (those that also control the brane scan), such as notably the supergravity Lie 3-algebra and the supergravity Lie 6-algebra. This is the refinement of super-Cartan geometry to higher Cartan geometry.

geometric contextgauge groupstabilizer subgrouplocal model spacelocal geometryglobal geometrydifferential cohomologyfirst order formulation of gravity
differential geometryLie group/algebraic group GGsubgroup (monomorphism) HGH \hookrightarrow Gquotient (“coset space”) G/HG/HKlein geometryCartan geometryCartan connection
examplesEuclidean group Iso(d)Iso(d)rotation group O(d)O(d)Cartesian space d\mathbb{R}^dEuclidean geometryRiemannian geometryaffine connectionEuclidean gravity
Poincaré group Iso(d1,1)Iso(d-1,1)Lorentz group O(d1,1)O(d-1,1)Minkowski spacetime d1,1\mathbb{R}^{d-1,1}Lorentzian geometrypseudo-Riemannian geometryspin connectionEinstein gravity
anti de Sitter group O(d1,2)O(d-1,2)O(d1,1)O(d-1,1)anti de Sitter spacetime AdS dAdS^dAdS gravity
de Sitter group O(d,1)O(d,1)O(d1,1)O(d-1,1)de Sitter spacetime dS ddS^ddeSitter gravity
linear algebraic groupparabolic subgroup/Borel subgroupflag varietyparabolic geometry
conformal group O(d,t+1)O(d,t+1)conformal parabolic subgroupMöbius space S d,tS^{d,t}conformal geometryconformal connectionconformal gravity
supergeometrysuper Lie group GGsubgroup (monomorphism) HGH \hookrightarrow Gquotient (“coset space”) G/HG/Hsuper Klein geometrysuper Cartan geometryCartan superconnection
examplessuper Poincaré groupspin groupsuper Minkowski spacetime d1,1|N\mathbb{R}^{d-1,1\vert N}Lorentzian supergeometrysupergeometrysuperconnectionsupergravity
super anti de Sitter groupsuper anti de Sitter spacetime
higher differential geometrysmooth 2-group GG2-monomorphism HGH \to Ghomotopy quotient G//HG//HKlein 2-geometryCartan 2-geometry
cohesive ∞-group∞-monomorphism (i.e. any homomorphism) HGH \to Ghomotopy quotient G//HG//H of ∞-actionhigher Klein geometryhigher Cartan geometryhigher Cartan connection
examplesextended super Minkowski spacetimeextended supergeometryhigher supergravity: type II, heterotic, 11d

For more background on principal ∞-connections see also at ∞-Chern-Weil theory introduction.


Around 1981 D’Auria and Fré noticed, in GeSuGra, that the intricacies of various supergravity classical field theories have a strikingly powerful reformulation in terms of super semifree differential graded-commutative algebras.

They defined various such super dg-algebras W(𝔤)W(\mathfrak{g}) and showed (paraphrasing somewhat) that

  • the field content, field strengths, covariant derivatives and Bianchi identities are all neatly encoded in terms of dg-algebra homomorphism Ω (X)W(𝔤):ϕ\Omega^\bullet(X) \leftarrow W(\mathfrak{g}) : \phi;

  • the action functionals of supergravity theories on such ϕ\phi may be constructed as images under ϕ\phi of certain elements in W(𝔤)W(\mathfrak{g}) subject to natural conditions.

Their algorithm was considerably more powerful than earlier more pedestrian methods for construction such action functionals. The textbook CastellaniDAuriaFre on supergravity and string theory from the perspective of this formalism gives a comprehensive description of this approach.

We observe here that the D’Auria-Fre-formalism is ∞-Chern-Simons theory for ∞-Lie algebra-valued forms with values in super ∞-Lie algebras such as the supergravity Lie 3-algebra and the supergravity Lie 6-algebra.

The pivotal concept that allows to pass between this interpretation and the original formulation is the concept of ∞-Lie algebroid with its various incarnations:


(Incarnations of \infty-Lie algebroids)

A (super) ∞-Lie algebroid

Notably the semifree dga upon which D’Auria-Fré base their description is the Chevalley-Eilenberg algebra of the supergravity Lie 3-algebra, which is an ∞-Lie algebra that is a higher central extension

0b 2𝔲(1)𝔰𝔲𝔤𝔯𝔞(10,1)𝔰𝔦𝔰𝔬(10,1)0 0 \to b^2 \mathfrak{u}(1) \to \mathfrak{sugra}(10,1) \to \mathfrak{siso}(10,1) \to 0

of a super Poincare Lie algebra 𝔰𝔦𝔰𝔬(10,1)\mathfrak{siso}(10,1) in the way the String Lie 2-algebra 𝔰𝔱𝔯𝔦𝔫𝔤(n)\mathfrak{string}(n) is a higher central extension of the special orthogonal Lie algebra 𝔰𝔬(n)\mathfrak{so}(n).

A super connection on an ∞-bundle with values in 𝔰𝔲𝔤𝔯𝔞(10,1)\mathfrak{sugra}(10,1) on a supermanifold XX is locally given by ∞-Lie algebroid valued differential forms consisting of

  • a 11\mathbb{R}^{11}-valued 1-form ee – the vielbein

  • a 𝔰𝔬(10,1)\mathfrak{so}(10,1)-valued 1-form ω\omega – the spin connection

  • a spin-representation valued 1-form ψ\psi – the spinor

  • a 3-form CC .

These are identified with the fields of 11-dimensional supergravity, respectively:

By realizing this data as components of a Lie 3-algebra valued connection (more or less explicitly), the D’Auria-Fré-formalism achieves some conceptual simplication of

Higher gauge theory reinterpretation

Originally D’Auria and Fré referred to commutative semifree dgas as Cartan integrable systems. Later the term free differential algebra, abbreviated FDA was used instead and became popular. Nowadays much of the literature that studies commutative semifree dgas in supergravity refers to them as “FDA”s. One speaks of the FDA approach to supergravity .

But strictly speaking “free differential algebra” is a misnomer: genuinely free differential algebras are pretty boring objects. Crucially it is only the underlying graded commutative algebra which is required to be free as a graded commutative algebra in that it is a Grassmann algebra 𝔤 *\wedge^\bullet \mathfrak{g}^* on a graded vector space 𝔤 *\mathfrak{g}^*. The differential on that is in general not free, hence the more precise term semifree dga .

In fact, when 𝔤\mathfrak{g} is concentrated in non-positive degree (so that 𝔤 *\wedge^\bullet \mathfrak{g}^* is concentrated in non-negative degree) the differential on 𝔤 *\wedge^\bullet \mathfrak{g}^{*} encodes all the structure of an ∞-Lie algebroid on 𝔤\mathfrak{g}. If 𝔤\mathfrak{g} is concentrated in negative degree the differential encodes the structure of an ∞-Lie algebra on 𝔤\mathfrak{g}. This interpretation of semifree dgas in Lie theory is the key to our general abstract reformulation of the D’Auria-Fré-formalism.

Already D’Auria and Fré themselves, and afterwards other authors, have tried to better understand the intrinsic conceptual meaning of their dg-algebra formalism that happened to be so useful in supergravity:

the idea arose and then became pupular in the “FDA”-literature that the D’Auria-Fré-formalism should be about a concept called soft group manifolds. This is motivated from the observation that by means of the dg-algebra formulation the fields in supergravity arrange themselves into systems of differential forms that satisfy equations structurally similar to the Maurer-Cartan forms of left-invariant differential forms on a Lie groupexcept that where the ordinary Maurer-Cartan form has vanishing curvature (= field strength) these equations for supergravity fields have a possibly non-vanishing field strength. These generalized Maurer-Cartan equations are suggested in the “FDA”-literature to describe generalized or “softened” group manifolds.

However, even when the field strengths do vanish the remaining collection of differential forms does not constrain the base manifold to be a group. Rather, if the field strengths vanish we have a natural interpretation of the remaining differential form data as being flat ∞-Lie algebroid valued differential forms, given by a morphism

A:TX𝔤 A : T X \to \mathfrak{g}

from the tangent Lie algebroid of the base manifold XX to the ∞-Lie algebra 𝔤\mathfrak{g} encoded by the semifree dga in question. In fact, applying the functor from ∞-Lie algebroids to dg-algebras given by forming Chevalley-Eilenberg algebras, the above morphism turns into a dg-algebra morphism

Ω (X)CE(𝔤):A \Omega^\bullet(X) \leftarrow CE(\mathfrak{g}) : A

to the deRham dg-algebra of XX (which we denote by the same letter, AA, in a convenient abuse of notation).

Since CE(𝔤)CE(\mathfrak{g}) is semifree, this is a map of graded vector spaces

Ω (X)𝔤 *:A \Omega^\bullet(X) \leftarrow \mathfrak{g}^* : A

together with a constraint that the morphism respects the differentials on CE(𝔤)CE(\mathfrak{g}) and on Ω (X)\Omega^\bullet(X). Such a morphism of graded vector spaces in canonically identified with a 𝔤\mathfrak{g}-valued differential form (recall that 𝔤\mathfrak{g} is a graded vector space)

ωΩ (X,𝔤) \omega \in \Omega^\bullet(X,\mathfrak{g})

and the aforementioned constraint is precisely the Maurer-Cartan-like equation that is known from left-invariant 1-forms on a Lie group. In fact, for GG a Lie group with Lie algebra 𝔤\mathfrak{g} there is a canonical morphism

Ω (G)CE(𝔤) \Omega^\bullet(G) \leftarrow CE(\mathfrak{g})

whose image is precisely the left-invariant 1-forms on the Lie group GG and whose respect for the differentials is precisely the ordinary Maurer-Cartan equation.

To see the role of group manifolds for more general morphisms

Ω (X)CE(𝔤):A \Omega^\bullet(X) \leftarrow CE(\mathfrak{g}) : A

one has to apply Lie integration of the ∞-Lie algebroid morphism TX𝔤T X \to \mathfrak{g} to a morphism of ∞-Lie groupoids

Π(X)BG \Pi(X) \to \mathbf{B}G

where Π(X)\Pi(X) is the path ∞-groupoid and where BG\mathbf{B}G is the delooping of Lie in-group GG that integrates the Lie n-algebra 𝔤\mathfrak{g}. Such morphisms are the integrated version of flat ∞-Lie algebroid valued differential forms.

The ∞-Chern-Weil theory of connections on ∞-bundles is about

  1. the generalization of such flat form data to ∞-Lie algebroid valued differential forms with curvature.

  2. the generalization from globally defined differential form data – which are connections on trivial principal ∞-bundles – to connections on arbitrary principal ∞-bundles.

The D’Auria-Fré-formalism – after this re-interpretation – is about the first of these points. So as an immediate gain of our reformlation of D’Auria-Fré-formalism in terms of connections on ∞-bundless we obtain, using the second of these points, a natural proposal for a formulation of supergravity field configurations that are possibly globally topologically nontrivial. Physicists speak of instanton solutions.

In fact, the ∞-Lie theory-reformulation exhibits the D’Auria-Fré-formalism as being secretly the realization of supergravity as a higher gauge theory.

It realizes supergravity as an example for a nonabelian higher gauge theory in that a supergravity field configuration is not realizable as a cocycle in ordinary differential cohomology as in ordinary abelian higher gauge theory (see there) but as a nonabelian connection on an ∞-bundle.


The supergravity Lie nn-algebras

We have a sequence of ∞-Lie algebra extensions

supergravity Lie 6-algebra\to supergravity Lie 3-algebra \to super Poincare Lie algebra

𝔰𝔲𝔤𝔯𝔞 6𝔰𝔲𝔤𝔯𝔞 3𝔰𝔦𝔰𝔬(10,1). \mathfrak{sugra}_6 \to \mathfrak{sugra}_3 \to \mathfrak{siso}(10,1) \,.

Super Lorentzian spacetime manifolds

The base space XX on which a supergravity field is a super Lie nn-algebra valued connection on an ∞-bundle is a supermanifold.

In particular, for constructing the action functional of supergravity we want XX to locally look like super Minkowski space.

Field configuration and field strength

A local field configuration on a supermanifold XX in the classical field theory is a morphism

TX(A,F A)inn(𝔰𝔲𝔤𝔯𝔞(𝔤)) T X \stackrel{(A, F_A)}{\to} inn(\mathfrak{sugra}(\mathfrak{g}))

from the tangent Lie algebroid to the inner-derivation Lie 4-algebra inn(𝔰𝔲𝔤𝔯𝔞(10,1))inn(\mathfrak{sugra}(10,1)), defined as the formal dual of the Weil algebra of 𝔰𝔲𝔤𝔯𝔞\mathfrak{sugra}). So dually this is a morhism of dg-algebras from the Weil algebra W(𝔰𝔲𝔤𝔯𝔞(10,1))W(\mathfrak{sugra}(10,1)) to the deRham dg-algebra Ω (X)\Omega^\bullet(X) of XX:

Ω (X)W(𝔰𝔲𝔤𝔯𝔞(10,1)):(A,F A). \Omega^\bullet(X) \leftarrow W(\mathfrak{sugra}(10,1)) : (A,F_A) \,.

This is ∞-Lie algebroid valued differential form data with ∞-Lie algebroid valued curvature that is explicitly given by:

  • connection forms / field configuration

  • curvature forms / field strengths

    • T=dE+ΩE+Γ(Ψ¯Ψ)Ω 2(X, 10,1)T = d E + \Omega \cdot E + \Gamma(\bar \Psi \wedge \Psi) \in \Omega^2(X,\mathbb{R}^{10,1}) - the torsion

    • R=dΩ+[ΩΩ]Ω 2(X,𝔰𝔬(10,1))R = d \Omega + [\Omega \wedge \Omega] \in \Omega^2(X, \mathfrak{so}(10,1)) - the Riemann curvature

    • ρ=dΨ+(ΩΨ)Ω 2(X,S)\rho = d \Psi + (\Omega \wedge \Psi) \in \Omega^2(X, S) – the covariant derivative of the spinor

    • G=dC+μ 4(ψ,E)Ω 4(X)G = d C + \mu_4(\psi, E) \in \Omega^4(X) – the 4-form field strength

Gauge transformations

A gauge transformation of a field configuration

ϕ:TXinn(𝔤 \phi : T X \to inn(\mathfrak{g}

is a diagram

Ω (X×Δ 1) vert A vert CE(𝔞) gaugetransformation Ω (X×Δ 1) A W(𝔞) field Ω (X) F A inv(𝔤) gaugeinvariantobservable \array{ \Omega^\bullet(X \times \Delta^{1})_{vert} &\stackrel{A_{vert}}{\leftarrow}& CE(\mathfrak{a}) &&& gauge\;transformation \\ \uparrow && \uparrow \\ \Omega^\bullet(X \times \Delta^{1}) &\stackrel{A}{\leftarrow}& W(\mathfrak{a}) &&& field \\ \uparrow && \uparrow \\ \Omega^\bullet(X) &\stackrel{\langle F_A\rangle}{\leftarrow}& inv(\mathfrak{g}) &&& gauge\;invariant\;observable }

Given a 1-morphism in exp(𝔤)(X)\exp(\mathfrak{g})(X), represented by 𝔤\mathfrak{g}-valued forms

Ω (U×Δ 1)W(𝔤):A \Omega^\bullet(U \times \Delta^1) \leftarrow W(\mathfrak{g}) : A

consider the unique decomposition

A=A U+(A vertλdt), A = A_U + ( A_{vert} \coloneqq \lambda \wedge d t) \; \; \,,

with A UA_U the horizonal differential form component and t:Δ 1=[0,1]t : \Delta^1 = [0,1] \to \mathbb{R} the canonical coordinate.

We call λ\lambda the gauge parameter . This is a function on Δ 1\Delta^1 with values in 0-forms on UU for 𝔤\mathfrak{g} an ordinary Lie algebra, plus 1-forms on UU for 𝔤\mathfrak{g} a Lie 2-algebra, plus 2-forms for a Lie 3-algebra, and so forth.

We describe now how this enccodes a gauge transformation

A 0(s=1)λA U(s=1). A_0(s=1) \stackrel{\lambda}{\to} A_U(s = 1) \,.

The condition that all curvature characteristic forms descend to UU in that AA completes to a diagram

Ω (U×Δ k) A W(𝔞) Ω (U) F A inv(𝔤) \array{ \Omega^\bullet(U \times \Delta^k) &\stackrel{A}{\leftarrow}& W(\mathfrak{a}) \\ \uparrow && \uparrow \\ \Omega^\bullet(U) &\stackrel{\langle F_A\rangle}{\leftarrow}& inv(\mathfrak{g}) }

is solved by requiring all components

Ω (U×Δ 1)AW(𝔤)r a 1𝔤 *F A a \Omega^\bullet(U \times \Delta^1) \stackrel{A}{\leftarrow} W(\mathfrak{g}) \stackrel{r^a}{\leftarrow} \wedge^1 \mathfrak{g}^* F_A^a

of the curvature forms to vanish when evaluated on the vector field s\partial_s along s\partial_s.

By the nature of the Weil algebra we have

ddsA U=d Uλ+[λA]+[λAA]++(F A)( s,), \frac{d}{d s} A_U = d_U \lambda + [\lambda \wedge A] + [\lambda \wedge A \wedge A] + \cdots + (F_A)(\partial_s, \cdots) \,,

so that this condition is a system of ordinary differential equations of the form

ddsA U=d Uλ+[λA]+[λAA]+, \frac{d}{d s} A_U = d_U \lambda + [\lambda \wedge A] + [\lambda \wedge A \wedge A] + \cdots \,,

where the sum is over all higher brackets of the ∞-Lie algebra 𝔤\mathfrak{g}.


Define the covariant derivative of the gauge parameter to be

λdλ+[Aλ]+[AAλ]+. \nabla \lambda \coloneqq d \lambda + [A \wedge \lambda] + [A \wedge A \wedge \lambda] + \cdots \,.

In this notation we have

  • the general identity

    (1)ddsA U=λ+(F A) s \frac{d}{d s} A_U = \nabla \lambda + (F_A)_s
  • the horizontality constraint or second Ehresmann condition

    (2)ddsA U=λ. \frac{d}{d s} A_U = \nabla \lambda \,.

This is known as the equation for infinitesimal gauge transformations of an \infty-Lie algebra valued form.


By Lie integration we have that A vertA_{vert} – and hence λ\lambda – defines an element exp(λ)\exp(\lambda) in the ∞-Lie group that integrates 𝔤\mathfrak{g}.

The unique solution A U(s=1)A_U(s = 1) of the above differential equation at s=1s = 1 for the initial values A U(s=0)A_U(s = 0) we may think of as the result of acting on A U(0)A_U(0) with the gauge transformatin exp(λ)\exp(\lambda).


In the formulation here the fields of supergravity are modeled by super differential forms on a supermanifold X˜\tilde X, and this very fact serves to make local supersymmetry manifest, i.e.serves to model geometry by higher supergeometric higher Cartan geometry.

But the actual fields of supergravity are supposed to be fields on actual spacetime XX (an ordinary smooth manifold) XX˜X \hookrightarrow \tilde X. Hence one is to impose a constraint that ensures that the super differential forms used on X˜\tilde X are uniquely determined by their restriction to ordinary differential forms on XX. This constraint is called rheonomy (Castellani-D’Auria-Fré 91, vol 2, section III.3.3), alluding to the idea that the constrains allow to “flow” the field data from spacetime XX to the super spacetime X˜\tilde X.

The idea here is analogous (Castellani-D’Auria-Fré 91, vol 2, p. 660, Fré-Grassi 08, p. 4) to how the Cauchy-Riemann equations impose the constraint for a function on the complex plane \mathbb{C} to be a holomorphic function and hence to be already fixed by its values on the real line \mathbb{R} \hookrightarrow \mathbb{C}.

In (Castellani-D’Auria-Fré, vol 2, section III.3.3) this idea is formalized by the constraint that for the given super-L L_\infty-algebra connection as above, those components of the curvature forms which carry fermionic indices must be linear combinations of the components carrying no fermionic indices. (See also at L-∞ algebra valued differential forms – integration of transformation.)

This rheonomy constraint is equivalent to what elsewhere is called “superspace constraints”, see (AFFFTT 98, below (3.12)).

See also at rheonomy modality.


Field equations of motion

A Chern-Simons element W(𝔤)W(b n1)csW(\mathfrak{g}) \leftarrow W(b^{n-1} \mathbb{R}) cs of an ∞-Lie algebra defines an ∞-Chern-Simons theory action functional on the space of 𝔤\mathfrak{g}-∞-Lie algebra-valued differential forms.

The major statement/claim is that all the supergravity equations of motion specify just precisely those super-L L_\infty-connections – satisfying their Bianchi identities– which are rheonomic.

Cosmo-cocycle equations

We discuss how actional functionals for supergravity theories are special cases of this.

In first-order formulation of gravity where the field of gravity is encoded in a vielbein EE and a spin connection Ω\Omega, the Einstein-Hilbert action takes the Palatini form

:(e,ω) XR a 1a 2E a 3E a dϵ a 1a d+, \mathcal{L} : (e,\omega) \mapsto \int_X R^{a_1 a_2} \wedge E^{a_3} \wedge \cdots \wedge E^{a_d} \epsilon_{a_1 \cdots a_d} + \cdots \,,

where R ab=dΩ ab+Ω acΩ c bR^{a b} = \mathbf{d} \Omega^{a b} + \Omega^{a c}\wedge \Omega_c{}^b are the components of the curvature of Ω\Omega and

ϵ a 1a n=sgn(a 1,,a n) \epsilon_{a_1 \cdots a_n} = sgn(a_1, \cdots, a_n)

is the signature of the index-permutation.

If EE and Ω\Omega are components of an ∞-Lie algebroid-valued form Ω (X)W(𝔤):A\Omega^\bullet(X) \leftarrow W(\mathfrak{g}) : A then such a Palatini term is of the form as may appear in a Chern-Simons element

Ω (X)AW(𝔤)csW(b n1):cs(A) \Omega^\bullet(X) \stackrel{A}{\leftarrow} W(\mathfrak{g}) \stackrel{cs}{\leftarrow} W(b^{n-1}\mathbb{R}) : cs(A)

on W(𝔤)W(\mathfrak{g}). We now discuss, following D’Auria-Fré, how the action functionals of supergravity are related to ∞-Chern-Simons theory for Chern-Simons elements on certain super \infty-Lie algebroids.

We discuss a system of equations that characterizes a necessary condition on Chern-Simons elements in the Weil algebra W(𝔤)W(\mathfrak{g}). This condition is called the cosmo-cocycle condition in (DAuriaFre).

To do so, we work in a basis {t a}\{t^a\} of 𝔤 *\mathfrak{g}^*. Let {r a}\{r^a\} be the corresponding shifted basis of 𝔤 *[1]\mathfrak{g}^*[1]. Write {1nC a b 0b n}\{\frac{1}{n}C^a{}_{b_0 \cdots b_n}\} for the structure constants in this basis, so that the differential in the Weil algebra acts as

d W:t a n1nC a b 0b nt b 0t b n+r a. d_W : t^a \mapsto \sum_{n \in \mathbb{N}} \frac{1}{n} C^a{}_{b_0 \cdots b_n} t^{b_0} \wedge \cdots \wedge t^{b_n} + r^a \,.

Write a general element in W(𝔤)W(\mathfrak{g}) as

csλ+r aν a+r ar bν ab++r a 1r a dν a 1a 2, cs \coloneqq \lambda + r^a \wedge \nu_a + r^a \wedge r^b \wedge \nu_{a b} + \cdots + r^{a_1} \wedge \cdots \wedge r^{a_d} \nu_{a_1 \cdots a_2} \,,

where λ,ν a,ν ab,CE(𝔤)\lambda, \nu_a, \nu_{a b}, \cdots \in CE(\mathfrak{g}).


The condition that d W(𝔤)(cs)d_{W(\mathfrak{g})} (cs) has no terms linear in the curvatures r ar^a is equivalent to the system of equations

ι t aλ+ν a ι t aλ+d Wν a+(1) |t a|C c ab 1b nt b 1t b nν c =0, \begin{aligned} \iota_{t_a} \lambda + \nabla \nu_a & \coloneqq \iota_{t_a} \lambda + d_W \nu_a + (-1)^{|t_a|} C^c{}_{a b_1 \cdots b_n} t^{b^1} \wedge \cdots t^{b^n} \wedge \nu_c \\ & = 0 \end{aligned} \,,

for all t a𝔤t_a \in \mathfrak{g}.

In DAuriaFre p. 9 this system of equations is called the cosmo-cocycle condition .


This follows straightforwardly from the definition of the Weil algebra-differential d W(𝔤)d_{W(\mathfrak{g})}:

We have d W(𝔤)=d CE(𝔤)+dd_{W(\mathfrak{g})} = d_{CE(\mathfrak{g})} + \mathbf{d}, where d:t ar a\mathbf{d} : t^a \mapsto r^a. So

d W(𝔤)λ=d CE(𝔤)λ+dλ=d CE(𝔤)λ+ ar aι t aλ. d_{W(\mathfrak{g})} \lambda = d_{CE(\mathfrak{g})} \lambda + \mathbf{d} \lambda = d_{CE(\mathfrak{g})} \lambda + \sum_a r^a \wedge \iota_{t_a} \lambda \,.

Here the first term contains no curvatures, while the second is precisely linear in the curvatures.

Moreover, by the Bianchi identity we have

d W(𝔤)r a= nC a b 0b nr b 0t b 1t b n. d_{W(\mathfrak{g})} r^a = \sum_n C^a{}_{b_0 \cdots b_n} r^{b_0} \wedge t^{b_1} \wedge \cdots \wedge t^{b_n} \,.

Therefore the condition that all terms in d Wcsd_{W} cs that are linear in r ar^a in vanish is

r aι t aλ+(1) |t a|r ad CE(𝔤)ν a+r a nC c ab 1b nt b 1t b nν c =r a(ι t aλ+d CE(𝔤)ν a+(1) |t a| nC c ab 1b nt b 1t b nν c) =0. \begin{aligned} & r^a \wedge \iota_{t_a} \lambda + (-1)^{|t_a|} r^a d_{CE(\mathfrak{g})}\nu_a + r^a \wedge \sum_n C^c{}_{a b_1 \cdots b_n} t^{b_1} \wedge t^{b_n} \wedge \nu_c \\ & = r^a( \iota_{t_a} \lambda + d_{CE(\mathfrak{g})}\nu_a + (-1)^{|t_a|} \sum_n C^c{}_{a b_1 \cdots b_n} t^{b_1}\wedge \cdots \wedge t^{b_n} \wedge \nu_c ) \\ & = 0 \end{aligned} \,.

For comparison with DAuriaFre notice the following:

  • there all elements t at_a happen to be in even degree. Therefore the extra sign (1) |t a|(-1)^{|t_a|} that we display does not appear.

  • the term that we write d CE(𝔤)ν ad_{CE(\mathfrak{g})} \nu_a is there equivalently expressed as

    d W(𝔤)ν a,atr a=0 d_{W(\mathfrak{g})} \nu_a \;,\;\;\; at\; r^a = 0

    (equation (2.21)).


Minimal 4-dimensional N=2N=2 supergravity


5-Dimensional Supergravity


1111-Dimensional Supergravity

Let 𝔤=𝔰𝔲𝔤𝔯𝔞 6\mathfrak{g} = \mathfrak{sugra}_6 be the supergravity Lie 6-algebra.

The Weil algebra:

d Wc=12ψ¯Γ abψe ae b+r c d_{W} c = \frac{1}{2} \bar \psi \wedge \Gamma^{a b} \psi \wedge e_a \wedge e_b + r^c


The Bianchi identity

d Wr c=ψ¯Γ abρe ae bψ¯Γ abψθ ae b d_W r^c = \bar \psi \wedge \Gamma^{a b} \rho \wedge e_a \wedge e_b - \bar \psi \wedge \Gamma^{a b} \psi \wedge \theta_a \wedge e_b

The element that gives the action is

11 =19R a 1a 2e a 3e a 11ϵ a 1a 11 + + + + + +840r cψ¯Γ abψe ae bc + +14ψ¯Γ a 1a 2ψψ¯Γ a 3a 4ψe a 5e a 11ϵ a 1a 11 +1415ψ¯Γ a 1a 2ψψ¯Γ a 3a 4ψe a 1e a 4C 840r cr cc \begin{aligned} \ell_{11} &= -\frac{1}{9} R^{a_1 a_2} \wedge e^{a_3} \wedge \cdots \wedge e^{a_{11}} \epsilon_{a_1 \cdots a_{11}} \\ & + \cdots \\ & + \cdots \\ & + \cdots \\ & + \cdots \\ & + \cdots \\ & + 840 r^c \wedge \bar \psi \Gamma^{a b} \psi \wedge e_a \wedge e_b \wedge c \\ & + \cdots \\ & + \frac{1}{4}\bar \psi\wedge \Gamma^{a_1 a_2} \psi \wedge \bar \psi \Gamma^{a_3 a_4} \psi \wedge e^{a_5} \wedge \cdots \wedge e^{a_{11}} \epsilon_{a_1 \cdots a_{11}} \\ & + - 14 \cdot 15 \bar \psi \wedge \Gamma^{a_1 a_2} \psi \wedge \bar \psi \Gamma^{a_3 a_4} \psi \wedge e_{a_1} \wedge \cdots \wedge e_{a_4} \wedge C \\ & -840 r^c \wedge r^c \wedge c \end{aligned}

This is DAuriaFre, page 26.

The first term gives the Palatini action for gravity.

The last terms is the Chern-Simons term for the the supergravity C-field.

The second but last two terms are the cocycle Λ\Lambda.


The term λ\lambda appearing here (the two terms containing no curvature) are d CEd_{CE}-exact: there is a modification of this element by a d Wd_W-exact term for which the cocycles vanish, λ=0\lambda = 0 (DAuriaFre, page 27 and CastellaniDAuriaFre (III.8.136)). It follows that in particular λ\lambda is d CEd_{CE}-closed. So with the above discussion of the “cosmo-cocycle”-condition the results given in DAuriaFre imply that d W 11d_{W} \ell_{11} has no 0-ary and no unary terms in the curvatures.

We find that the d Wd_W-differential of this Lagrangian term is

d W 11 =r cr cr c R a 1a 2θ a 3e a 11ϵ a 1a 11 + +840{σ(r cψ¯Γ abψe ae bc)+(d W(r cr c))c=0} +840r cr cψ¯Γ abψe ae bi48r cσ(ψ¯Γ a 1a 5ψe a 1e a 5) +. \begin{aligned} d_{W} \ell_{11} & = r^c \wedge r^c \wedge r^c \\ & - R^{a_1 a_2} \wedge \theta^{a_3} \wedge \cdots \wedge e^{a_{11}} \epsilon_{a_1 \cdots a_{11}} \\ & + \cdots \\ & + 840 \{ \sigma(r^c \wedge \bar \psi \Gamma^{a b} \psi \wedge e_a \wedge e_b \wedge c ) + (d_{W}(r^c \wedge r^c)) \wedge c = 0 \} \\ & + 840 r^c \wedge r^c \wedge \bar \psi \Gamma_{a b} \psi\wedge e_a \wedge e_b - i 48 r^c \wedge \sigma(\bar \psi \wedge \Gamma^{a_1 \cdots a_5} \psi \wedge e_{a_1} \wedge \cdots \wedge e_{a_5}) \\ & + \cdots \end{aligned} \,.

This fails to sit in the shifted generators by the terms coming from the translation algebra. For the degree-3 element cc however it does produce the expected term r cr cr cr^c \wedge r^c \wedge r^c.


The formulation of supergravity of supermanifolds and the relevance of the Bianchi identities originates in

  • R. Grimm, Julius Wess, Bruno Zumino, A complete solution of the Bianchi identities in superspace with supergravity constraints, Nuclear Phys. B152 (1979), 255–265.

  • Julius WessBruno Zumino, Superspace formulation of supergravity, Phys. Lett. B66 (1977), 361–364.

The use in this context of super L-∞ algebras in their formal dual incarnation semifree super-graded commutative dg-algebras was suggested originally in

  • Peter van Nieuwenhuizen, Free Graded Differential Superalgebras, in Istanbul 1982, Proceedings, Group Theoretical Methods In Physics, 228-247 and CERN Geneva - TH. 3499 (spire)

The original articles that introduced specifically the D’Auria-Fré-formalism are

The standard textbook monograph on supergravity in general and this formalism is particular is

Review includes

Discussion of gauged supergravity in this way is in

The interpretation of the D’Auria-Fré-formulation as identifying supergravity fields as ∞-Lie algebra valued differential forms is in

The Lie integration of that to genuine principal ∞-connections is in

The super L-∞ algebras that govern the construction are interpreted in the higher gauge theory of an ∞-Wess-Zumino-Witten theory description of the Green-Schwarz sigma-model-type pp-branes in

Apart from that the first vague mention of the observation that the “FDA”-formalism for supergravity is about higher categorical Lie algebras (as far as I am aware, would be grateful for further references) is page 2 of

An attempt at a comprehensive discussion of the formalism in the context of cohesive (∞,1)-topos-theory for smooth super ∞-groupoids is in the last section of

To compare D’Auria-Fre with our language here, notice the following points in their book

  • The statement that a supergravity field is a morphisms ϕ:TXinn(𝔤)\phi : T X \to inn(\mathfrak{g}) or dually a morphism Ω (X)W(𝔤):ϕ\Omega^\bullet(X) \leftarrow W(\mathfrak{g}) : \phi out of the Weil algebra of the supergravity Lie 3-algebra or similar is implicit in (I.3.122)(I.3.122) (but it is evident, comparing with the formulas at Weil algebra) – notice that these authors call ϕ\phi here a “soft form”.

  • What we identify as gauge transformations and shifts by the characterization of curvature forms on the cylinder object U×Δ 1|pU \times \Delta^{1|p} is their equation (I.3.36).

Here are some more references:

  • Pietro Fré, M-theory FDA, twisted tori and Chevalley cohomology (arXiv)

  • Pietro Fré; and Pietro Antonio Grassi, Pure spinors, free differential algebras, and the supermembrane (arXiv)

  • Pietro Fré; and Pietro Antonio Grassi, Free differential algebras, rheonomy, and pure spinors (arXiv)

Discussion in this formalism of the Green-Schwarz action functional for the M2-brane sigma-model with a target space 11-dimensional supergravity background is in

Last revised on February 13, 2018 at 02:03:30. See the history of this page for a list of all contributions to it.