Extended geometry and gauged maximal supergravity

We consider generalized diffeomorphisms on an extended mega-space associated to the U-duality group of gauged maximal supergravity in four dimensions, E_7. Through the bein for the extended metric we derive dynamical (field-dependent) fluxes taking values in the representations allowed by supersymmetry, and obtain their quadratic constraints from gauge consistency conditions. A covariant generalized Ricci tensor is introduced, defined in terms of a connection for the generalized diffeomorphisms. We show that for any torsionless and metric-compatible generalized connection, the Ricci scalar reproduces the scalar potential of gauged maximal supergravity. We comment on how these results extend to other groups and dimensions.

phisms plus gauge transformations of all the gauge fields) look just like diffeomorphisms, and are encoded in a generalized Lie derivative [10]- [13], which gives the differential structure of the space. It allows to define a generalized, metric compatible, and torsion-free connection [10]. Moreover, a generalized Ricci tensor, whose flatness condition reproduces the supergravity equations of motion, and a generalized Ricci scalar, encoding the supergravity Lagrangian [10], can be constructed. For the case of Generalized Complex Geometry, these tensors were worked out in [11], inspired from older double formalism [14]- [16]. More explicit constructions in DFT are presented in [17]- [22].
In this paper, we extend the more explicit DFT constructions to the exceptional case, for d = 6, when the symmetry group is 1 E 7 , following the definitions introduced in [10] for EGG. To be more precise, from the generalized Lie derivative acting on the bein of the generalized metric we define the "dynamical fluxes". These are required to live in certain representations of the duality group. Jacobi-type constraints on these fluxes are obtained from requiring closure of the algebra and gauge invariance. Interestingly enough, for constant fluxes, which correspond to the embedding tensor of N = 8 supergravity [23], the Jacobi-type constraints reduce to the usual quadratic constraints of maximal supergravity. We show that a generalized Levi-Civita connection, related to the fluxes by a torsion free condition, can be constructed allowing to build Riemann and Ricci tensors [10]. When these are defined in the usual way, they turn out to be non-tensorial, and thus one has to resort to generalized versions of them. Covariant definitions of these tensors were introduced in [10,17,19], which interestingly contain undetermined components.
Here, extending the definition of [17] to the exceptional case, we find a covariant (though still not uniquely defined) version of the generalized Ricci tensor. Taking its trace, the undetermined pieces go away, and we show that the generalized Ricci scalar, which coincides with that of [10] when the section condition is imposed, can be written purely in terms of the dynamical fluxes. In the case of constant fluxes, the generalized Ricci scalar is exactly equal to the potential of N = 8 supergravity, provided we identify the generalized metric with the moduli space metric for the N = 8 scalars. Some definitions and results for d < 6 are given in [12], and some more for d = 4, 5 in [24]. Finally, for 1 All throughout the paper when we refer to E 7 , we really mean E 7 (7) . completion we provide a list of complementary results along these lines [25]- [30].
The paper is organized as follows. In Section 2 we set the basic notation and address the definition of generalized diffeomorphisms on a 56 dimensional extended space.
The generalized Lie derivative is introduced and through it the "dynamical fluxes" are defined. In Section 3 we deal with constraints required from closure of the algebra of gauge transformations. We discuss two different solutions to the Jacobi-type constraints.
The so called section condition (also known as strong constraint) and what we call twisted constraints. We mainly deal with these latter constraints. They reproduce the quadratic constraints of maximal N = 8 supergravity and would naturally appear in Scherk-Schwarz like compactifications. A geometrical structure for the extended space is addressed in Section 4 where a generalized covariant derivative and generalized torsion are introduced. A generalized Ricci tensor is defined in Section 5. Interestingly enough it is shown that, under contractions with the generalized metric, the associated Ricci scalar is completely determined in terms of generalized fluxes, and corresponds to the scalar potential of maximal supergravity. Final comments are presented in Section 6. Some notation and useful results are summarized in the Appendices.

Generalized diffeomorphisms and fluxes
Our starting point is the 56-dimensional exceptional generalized tangent space, or extended space, for an extended version of Double Field Theory, where 56 is the dimension of the fundamental representation of E 7 . For toroidal compactifications, such a space was called megatorus [5] 2 . This space encodes all the symmetries of string theory compactified on 6-manifolds, or M-theory compactified on 7-manifolds, namely internal diffeomorphisms and gauge transformations of the NSNS and RR gauge fields (or the 3-form gauge field in M-theory).
The coordinates in the extended space are Y M with M = 1, . . . , 56, and the derivatives 2 Here we do not require the extended space to be a parallelizable manifold (i.e., a torus or a "twisted torus"), except for sections 3.2 and 5.2, and at the very end of section 5, where we compare the generalized Ricci scalar to the potential of N = 8 supergravity.
are noted by ∂ M = ∂/∂Y M and transform in the fundamental representation of E 7 . We postpone to Section 3 the discussion about constraints to be satisfied by them.
We will actually consider an augmented duality group, R + × E 7 , which accounts for a conformal factor [10,11]. This gives an extra degree of freedom in the 4D supergravity whose string theory origin can be traced to the measure of the 6-, 7-dimensional manifold, as well as extra gauge parameters, as we will see.
There is a generalized metric on the extended space H M N , which transforms covariantly under R + × E 7 , and is invariant under SU(8), the maximal compact subgroup of E 7 . It can be written in terms of a generalized bein EĀ M taking values in the quotient so it is natural to define a weighted symplectic metric which raises and lowers indices according to the following convention With this convention, the following relations hold In addition to the symplectic invariant, in R + × E 7 there is also a quartic invariant A generalized diffeomorphisms compatible with this symmetry group is generated by an infinitesimal generalized vector (or gauge parameter) ξ, and is given by the generalized Lie derivative L ξ (or equivalently a generalized gauged transformation δ ξ , which coincide when acting on tensors). Acting on a generalized vector field V , we expect it to be a linear combination of the gauge parameter and its derivatives. A detailed discussion on how to construct generalized diffeomorphisms can be found in Appendix C. Here we simply give its general expression This was first proposed in [10] and we are using the notation of [13] (see also [14,15] in DFT context). The tensor A is fixed by requiring that the gauge transformations preserve the E 7 structure (see (2.3) and (2.7)) and is given by where t α is a generator of E 7 , with α = 1, . . . , 133 an index in the adjoint, and P (adj) is a projection to the adjoint 133 of E 7 . We give its expression in terms of E 7 invariants in (A.1). The coefficient ω corresponds to the R + weight of the object being transformed, which for the bein EĀ M is ω = 1, but forẼĀ M is ω = 0. 3 In the appendices we provide more information about the general structure of generalized diffeomorphisms, showing how the E 7 case arises as a particular example. We also include many useful identities that we will use repeatedly along the paper. The relative coefficient between A and the projector onto the adjoint depends on the group in question.
In Appendix C we explain where this arises from, and why it is 12 for the case of E 7 (7) .
Applying the generalized diffeomorphism (2.8) to the bein, generated by a bein itself, we get where the "generalized dynamical fluxes" FĀBC are defined as In the case when there is a global frame (or in other words when the space is parallelizable), this object is called the Weitzenböck connection. Here, with the exception of sections 3.2, 5.2 and 5.3, we do not a priori require the existence of such a global frame, and as such our expressions should be understood as local. This means in particular that the generalized dynamical fluxes need not be constant (hence the name dynamical), and furthermore they need not even be globally defined. Nevertheless, by an abuse of notation we will still call these fluxes, and we will call Ω in (2.12) the Weitzenböck connection.
Rotating these expressions with the bein we can define the fluxes with curved indices 13) and the corresponding Weitzenböck connection in curved indices (2.14) The Weitzenböck connection (2.14) takes values in the algebra of R + × E 7 (see Appendix B), i.e. it can be written as linear combination of the generators of R + × E 7 15) and is therefore in the 56 × (1 + 133) product. Here, contains the irreducible representations 56 + 912 + 6480. The projectors onto the first two representations in this product is given by (see Appendix C) Equations (2.13) to (2.17) imply that the fluxes are in the 912 and 56 representations only. More precisely and The fluxes F involve therefore a projection onto the 912 given by the gaugings X plus contributions from the gaugings ϑ. In the language of gauged supergravity, they correspond to the gauge group generators, i.e. are contractions of the embedding tensor (which dictates how the gauge group is embedded in the global symmetry group) with the generators of the global symmetry group [23]. For this reason we will sometimes call them "gaugings". The X piece in (2.18) corresponds to the 912 component of the fluxes, and in terms of the Weitzenböck connection and the quartic invariant reads Using the identities (A.5) of the quartic invariant, one can show that X enjoys the properties of the 912 which are the well known conditions satisfied by gaugings in N = 8 maximal supergravity [32].
The D piece (2.20) contains two terms, one belonging to the 56 in 56 × 1, and another belonging to the 56 in 56×133. Notice however, that both terms contain the same degrees of freedom in terms of ϑ and are therefore not independent.
With these results we are able to express the gauge group generators (F A ) B C as in [35] The so-called intertwining tensor (i.e., the symmetric components of the gauge group generators) takes the form 24) and therefore takes values in the E 7 algebra, as expected [35].

Consistency constraints
Closure of the algebra and Leibniz rule of gauge transformations impose a set of Jacobi-type constraints on the vector fields, which are quadratic in derivatives. We first obtain their general expressions, and then show two different set of solutions, commenting on the relevance of each. Defining the closure of the algebra and Leibniz rule can be cast in form is the Exceptional Courant Bracket [8,10], while the ((ξ 1 , ξ 2 )) is given by In the following, it is useful to define the invariant [13] Y Q M R where in the last equality we have used (A.4). The generalized diffeomorphisms (2.8) can be written in terms of this operator as where L ξ V is the ordinary Lie derivative. Therefore, Y can be understood as an object measuring the departure from usual Riemannian geometry.
A first constraint arising form closure of the gauge algebra states that two successive gauge transformations should effectively correspond to a unique gauge transformation.
If the first (second) transformation is parameterized by ξ 1 (ξ 2 ), the parameter of the composed transformation is given by the Exceptional Courant Bracket. Explicitly, this is Using equation (A.6), the closure condition can be written in the form where we have defined Additionally using the Leibniz rule is written as Equations (3.9) and (3.12) imply that any theory invariant under generalized diffeomorphisms will necessarily be a constrained or restricted theory, meaning that the fields and gauge parameters will not be generic, but must necessarily obey these differential conditions. Therefore, these constraints select subset of fields and gauge parameters for which the theory can be consistently defined.
Notice also that, as shown in [13], the Jacobiator can be written as so even if non-vanishing, it generates trivial gauge transformations by virtue of (3.12).
We would now like to explore two different set of solutions to the above constraints, and comment on their relevance for different purposes.

The section condition
In DFT, there exists a so-called section condition, also known as the strong constraint, consisting of the following differential operator that must annihilate all fields and gauge parameters and their products [2] S = η mn ∂ m ∂ n , (3.14) where m, n = 1, ..., 2d span the fundamental of O(d, d). In the strong version of the constraint, each partial derivative acts on a given field. In its weak version, what should vanish is the second order operator acting on a single field. The result of the strong constraint is that the fields and gauge parameters no longer depend of the full set of 2d coordinates, but rather on a d-dimensional section of the space.
The E 7 version of the constraint is given by the following operator [10] and again in its weak version this whole operator should vanish when acting on a single field, while in its strong version each derivative hits a different field.
In SL (8)   hard to see that implies that the fields can only depend on 7 out of the 56 coordinates of the extended space [13]. Indeed, calling these directionsâ = 1, ..., 7, we get that, up to E 7 rotations, ∂â 8 ≡ ∂â, ∂âb = 0, ∂ ab = 0 is the only solution to the constraint. This is precisely how the derivative, which spans a 7-dimensional space for compactifications of M-theory on 7-dimensional manifolds, is embedded in the fundamental representation of E 7 in Exceptional Generalized Geometry [8].
To make contact with DFT, or equivalently with compactifications of type II theories, The different components of the projector onto the adjoint representation are given in (A.14). In particular, the first one of them gives the following constraint The requirements S +m+n = 0, S −m−n = 0 give on one hand that the derivative can only span one of the two copies of the DFT coordinates (call it +, or electric), and on the other hand we get exactly the DFT strong constraint (3.14), which implies that the dependence is only on half of the double coordinates, that we call m = 1, . . . , 6. Using this in the S +m−n − S −m+n constraint, only the last term in (3.17) survives, and one can see that the spinorial derivative can only span a two-dimensional (12-dimensional) subspace in the case of positive (negative) chirality. The former is relevant for compactifications of type IIA, where D-branes have even dimensionality, while the latter applies to type IIB.
The allowed components of the spinorial derivatives are further reduced by the condition S +mα = 0 (where the relevant projector is given in the last line of (A.14)) to a onedimensional (zero-dimensional) space in the case of positive (negative) chirality, defined by the constraint [γ m ] α β ∂ β = 0 5 . In summary, the strong constraint implies that the dependence is on 6 coordinates only 6 ∂ +m = 0 , plus an extra spinorial coordinate for the case of positive chirality, which arises in compactifications of type IIA. This extra coordinate is nothing but the M-theory circle. If one wants to avoid this dependence, an extra constraint should be supplemented to (3.15).
With this information, we can now show that a possibility to solve the constraints (3.9) and (3.12) is to restrict the vector fields to depend only on a 7-dimensional slice of the full mega-space, i.e. constrain them to satisfy the section condition Notice that in (3.9) and (3.12) all the derivatives are contracted with the Y tensor defined in (3.6). When acting on two partial derivatives ∂ Q ∂ R , the last term on the last equality in (3.6) vanishes due to the section condition. The first term vanishes because the section condition restricts the derivatives to lie in an isotropic bundle, i.e. to have zero inner product with respect to the symplectic form. Therefore the section condition implies acting on any two fields, and this in turn guarantees that (3.9) and (3.12) are satisfied.

Twisted constraints
In [4] it was shown that the section condition is sufficient for the gauge consistency of the theory, but not necessary. Rather, in particular setups such as the ones discussed below, it is not hard to see that the constraints (3.9) and (3.12) are weaker than the strong constraint, and this allows for extended configurations not solving the section condition.
These weaker conditions apply when the vector fields are required to take the form with v constant. Note that this is only possible in parallelizable manifolds, so in this section (as well as in section 5.2), where we use these weaker constraints, we restrict to this case (i.e. we demand that the extended space is parallelizable). This definition can be trivially extended to tensors with more indices. This kind of behavior arises naturally in the context of Scherk-Schwarz compactifications, where the bein plays the role of a twist, and the vĀ vectors correspond to fields or gauge parameters in the effective action, and therefore only depend on space-time coordinates (which we are ignoring in this paper, thus v is constant here). We therefore call the constraints obtained in thee setups "twisted constraints". We will show that requiring the vector fields in planar indices to be constant, equations (3.9) and (3.12) admit solutions that do not necessarily satisfy the section condition.
Let us now move to closure (3.9) and the Leibniz rule (3.12). Notice that in the particular case when (3.9) is evaluated on frames, i.e. ξ 1 → EĀ, ξ 2 → EB and ξ 3 → EC and the same for (3.12) Alternatively one can compute ∆ĀBC M using (2.10) directly in terms of FĀBC Then the closure and the Leibniz rule are recovered in the form Notice that if the section condition is imposed the closure and the Leibniz rule are guaranteed as noted above. However if we restrict our vectors to take the form (3.20) a weaker version of the constraints can be considered provided the quadratic constraint (3.23) is imposed to ensure the consistency of the theory. In the particular case in which the fluxes are constant, condition (3.23) becomes which are precisely the quadratic constraints of maximal supergravity, even with local scaling symmetry [35](notice that the trace of this equation implies in turn F AB C ϑ C = 0).
Let us mention that when the fluxes are expressed in planar indices, they should transform as scalars. In fact, we find This actually guarantees that X and ϑ transform as scalars independently. For example, in the case of ϑ we get configurations were found in [34], and it would be interesting to find some here as well.
A few words are in order. The section condition is crucial to make contact with 10 or 11-dimensional supergravity, and therefore puts the extended theory in a safe and controlled place. When relaxed, the connection between this construction and higher dimensional supergravity is less clear and should be understood better. Configurations that satisfy the relaxed constraints but not the section condition lie beyond supergravity compactifications, and are therefore strictly non-geometric (we refer to [34] for a discussion on these issues). Whether they correspond to allowed configurations in the full string or M-theory is a question that remains partially unanswered and worth exploring.

A geometry for the extended space
In this section we discuss the covariant derivative on the extended space, seek for a covariant definition of torsion, and propose a set of conditions that the connection must satisfy. Later in the following section we will define a generalized Ricci tensor, and show that under contractions with the generalized metric, the associated Ricci scalar is completely determined in terms of generalized fluxes, and corresponds to the scalar potential of maximal supergravity.
Having defined the generalized notion of Lie derivative in (2.8), it is natural to look for derivatives that behave covariantly under such transformations. We begin by defining the covariant derivative of a bein E as In addition, one can relate the gaugings to the Weitzenböck connection through projections, as in equation (2.11).
These connections must also transform properly so as to compensate the failure of the usual derivative to transform as a tensor. Given that the covariant derivative is requested to transform covariantly, so must the spin connection. Hence, taking into account (4.2), we see that the Christoffel connection must fail to transform as minus the failure of the Weitzenböck connection where ∆ ξ = δ ξ − L ξ is defined as in an analogous way as in (3.26), and represents the failure of an object to transform as a tensor.

Generalized connections and torsion
We can define the generalized torsion through [11] TĀBC where L ∇ is defined as in (2.8), but with a partial replaced by a covariant derivative.
Using (4.2) we arrive at A torsionless connection requires this to vanish, which amounts to Now, acting on this condition with the projector to the adjoint in the last two indices, we find P (adj) and now plugging this result in (4.6) we find  is ensured if which, as we show below, is a consequence of metric compatibility. The torsionless (4.6) and the trace equations (4.12) imply that the connection takes the form whereΓ belongs to the 6480 of 56 × 133 (which is traceless). This piece remains undetermined here, but a part of it will be fixed by imposing metric compatibility.
We now turn to the analysis of the spin connection W . Using (4.2), (2.15) and (4.13) one can obtain (4.14) From this expression we learn on the one hand that the spin connection takes values in 56 × 133, and on the other that its trace is proportional to the ϑ gaugings (2.13) Knowing that the spin connection belongs to the 56 × 133, we can now act with the projectors to its irreducible representations, and find while the projector to the 6480 just relates it toΓ which is undetermined by the torsionless condition. Finally let us write explicitly the expression for the torsionless condition in terms of W , because it will be useful in the following (4.17)

Generalized metric compatibility
Another condition we can impose to the connections is compatibility with the generalized metric H, equation (2.2). The constraint reads It is instructive to turn to the SU(8) language. When E 7 is broken to SU (8) Another consequence of the metric compatibility is Eq. (4.12). This can be proven taking into account (4.9), the fact that the metric is covanriantly constant (Eq. (4.18)) and the useful formula for the derivative of the determinat Let us also comment on compatibility with E 7 invariants. The compatibility with the symplectic metric is not an additional constraint on the connection, but is automatically satisfied, in fact where we have used (4.13). The same holds for the compatibility with the quartic invariant, since is automatically satisfied using (A.7).
We summarize the properties of the different connections introduced, as well as that of the fluxes, in Table 1.

Generalized Ricci tensor and the scalar potential of gauged maximal supergravity
The Riemann and torsion tensors are usually defined through the relation and We already discussed a generalized version of torsion, arguing that the usual definition is non-covariant under generalized diffeomorphisms (2.8). The same happens to the Riemann tensor and its trace (the Ricci tensor), and then one has to resort to generalized versions of them. We will now split the discussion in two parts. We will begin with the definition of a generalized Ricci tensor, that is covariant under generalized diffeomorphisms that close under the section condition. Then, we will extend the definition of this tensor so that it is also covariant under generalized diffeomorphisms that close under the twisted constraints.

Generalized Ricci tensor and the section condition
In this section we will restrict to diffeomorphisms parameterized by vectors obeying the section condition, defined in Section 3.1.
As we mentioned, under generalized diffeomorphisms (2.8), the generalized Riemann tensor is not covariant. Using the section condition (3.15) (or its variant (3.19)), we find which in the usual case (i.e. in ordinary general relativity where Y = 0) vanishes due to vanishing torsion. Notice that for everything to be consistent here, we must have , and this holds up to terms that vanish under the section condition.
The usual Ricci tensor is defined as 5) and in this case is not symmetric, and fails to transform covariantly as However, note that the vanishing (generalized) torsion condition (4.6) imposes and this allows to rewrite Using this, is it easy to see that the following symmetric object is a covariant extension of the Ricci tensor This is the natural extension of the DFT definition of Ricci tensor introduced in [17,19].
Let us conclude this section by noticing that a definition of the generalized Ricci tensor can be given in terms of covariant derivatives. In fact, after some algebra we find that [10] [∇ M , Namely, the generalized Ricci tensor can be expressed as a commutator of covariant derivatives plus a term proportional to the invariant Y that, as pointed out above, measures in some sense the departure from ordinary Riemannian geometry. Interestingly enough, due to the section condition the operator ∇ A (Y A M B P ∇ B ·) has no second order derivatives. Moreover, when the Ricci is projected to the space of deformations of the generalized metric, its undetermined pieces get projected out [10].

Generalized Ricci tensor and twisted conditions
In this section we assume that all vectors take the form (3.20), and consider diffeomorphisms that close under the twisted constraints of Section 3.2.
The starting point is the failure of the Christoffel connection to transform as a tensor It can be verified that its trace (4.12) transforms properly, provided the twisted constraints In this case, for the Riemann tensor we get So again we find that the usual Riemann tensor (i.e. in ordinary general relativity) is not covariant under the diffeomorphisms that close under the twisted constraints. The same happens for the usual Ricci tensor, because tracing the above expression does not solve the problem However, the Ricci tensor can be generalized into a (symmetric) generalized Ricci tensor by slightly extending the definition (5.9) The last term vanishes if the section condition is imposed, which is not the case here.
This term must therefore be added to define a covariant Ricci tensor. The trace of this term is the analogue of the term added in DFT in [4].
To check the covariance of the generalized Ricci tensor up to twisted constraints, it is instructive to use planar indices. We first write the Riemann tensor in planar indices which is not an assumption in this section. Notice however, that the last two terms can be re-written in an explicitly covariant form We finish this section by giving an explicit expression for a covariant generalized Ricci When tracing this expression and integrating with the measure to obtain an action, the last term gives a total derivative and therefore vanishes. We emphasize that this generalized Ricci tensor was constructed only imposing the twisted constraints, and reduces to (5.9) if the section condition is imposed.

Generalized
Remarkably, this takes the exact same form as the scalar potential of gauged maximal supergravity [32] if we identify the generalized metric with the moduli space matrix M.
Note also that this is true for any torsionless and metric-compatible connection, and the concrete expression of the determined part does not need to be known. In fact, we never needed to solve for the spin connection, but only used the equation that defines it implicitly.
Finally, notice that by definition the Ricci scalar transforms indeed as a scalar under generalized diffeomorphisms can be reached in this way.
We then described the geometry of the extended space, starting from a derivative transforming covariantly under generalized diffeomorphisms, and their corresponding Christoffel and spin connections. These are not uniquely defined, only a subset of its components are, via the torsionless and metric compatibility conditions. We summarized the properties of the different connections in Table 1. The next question is whether a curvature for the extended space can be defined. Since there seems to be no easy way to define a covariant generalized Riemann tensor [11], we considered only the Ricci tensor and scalar, which transform appropriately up to the constraints of the theory. We showed how to meet these conditions in two different ways. In the first one, the Ricci tensor behaves appropriately if the section condition is imposed, and it corresponds to the natural generalization of that introduced in the context of Double Field Theory [17,19] and equals that of [10] in the context of generalized (R + × E 7(7) ) geometry. In the second approach, the section condition is relaxed within the context of Scherk-Schwarz-like compactifications, and we showed that the definition of the Ricci tensor must be further extended so that it is also covariant up to the twisted constraints (3.24). Up to our knowledge, this is the first covariant construction of an extended geometry where the section condition is not imposed.
Finally, we showed that the resulting Ricci scalar matches exactly the scalar potential of gauged maximal supergravity, provided one associates the generalized metric with the moduli scalar matrix, the dynamical fluxes are taken to be the constant gaugings, and the gaugings in the 56 are taken to zero. Although the original expression for the generalized Ricci scalar (5.16) is a function of the spin connection, which contains undetermined pieces, we show that these contributions simply drop out, and therefore any torsionless and metric compatible connection gives the desired Ricci scalar, whatever its undetermined part is.
Let us finally comment on some interesting questions that remain open, and are worth exploring in our point of view. It is known that the section condition implies that this framework is a covariant re-writing of higher-dimensional supergravity compactifications.
In this kind of compactifications only a subset of the gaugings can be reached in the lower dimensional effective action, and thus the space of gauging orbits is split into those that can be obtained (geometric) and those that cannot (non-geometric) [34]. Restricting to Scherk-Schwarz-type backgrounds, this construction does not necessarily use the section condition, and instead uses the twisted conditions, which are in one to one correspondence with the constraints of gauged supergravity. Therefore, any orbit of gaugings can be reached geometrically in this construction, even those that are non-geometric from a supergravity point of view. Recently there has been much progress in moduli-fixing, fluxed induced supersymmetry breaking, de Sitter vacua surveys, etc. in the presence of non-geometric gaugings, and we believe that this framework can shed light on the higher dimensional uplift of these orbits, as background fluxes on the mega-space. For example, recently a one-parameter family of new maximal gauged supergravity with SO(8) gauge group was found [38]. It would be nice to seek for an uplift of these gaugings to the mega-space considered here.
Note added: After our work appeared on the ArXiv the preprint [39], with substantial overlap with our sections 4 and 5, was uploaded.

Acknowledgments
We are very grateful to C. Nuñez for collaboration in the early stages of this project. We and the final useful properties we used in the paper are The maximal compact subgroup of E 7 is SU (8). When E 7 is broken to SU(8), the fundamental 56 and adjoint 133 representations break according to where i, j, · · · = 1, . . . , 8 and the 63 is traceless i i = 0.
The 133 generators of E 7 break into 63 and 70 generators, respectively [35] (t i j ) mn with Cartan-Killing metric The projection to the adjoint in the product 56 × 56 reads B The Weitzenböck connection and the algebra the Weitzenböck connection, defined as is an element of the algebra of G. This can be easily seen by use of the identity A quick computation shows that with

C Representations, projectors and generalized diffeomorphisms
In this Appendix we first present the projectors onto the irreducible representations in the tensor product of the fundamental with the adjoint representation of an arbitrary simple group G, following the appendix of [23]. Related expressions and useful identities can be found in [31]. We will then show how this sheds light in the interpretation of the coefficients appearing in the structure of generalized diffeomorphisms, in terms of group theoretical quantities. and therefore it is useful to construct projectors onto these representations.

C.1 Representations and Projectors
Let us call d Λ = dim(D(Λ)), d = dim(G), and {t α } (α = 1, . . . , d) the generators of G in the D(Λ) representation. Furthermore, let C θ , C Λ be the Casimirs of the adjoint and fundamental representations, respectively. The invariant matrix η αβ = Tr(t α t β ) is used to rise and lower the adjoint indices, and is related to the Cartan-Killing metric κ αβ by Using the definition of the Casimir operator, C Λ 1 d Λ = κ αβ t α t β , we have the following where g ∨ is the dual Coxeter number andĨ Λ is the Dynkin index of the fundamental representation. In the simply laced case we have additionally with r the rank of G. and sum to the identity on D(Λ) × Adj(G). These three projectors can be expressed in terms of three independent objects, namely: where A r r + 1 r + 1 1 2 1 2 (r − 1)(r + 1)(r + 2) with d 1 = dim (D 1 ). Moreover, d 1 is determined to be In where α is some group-dependent constant, and the projector to the adjoint is given in (2.9). Restricted to orthogonal frames EĀ, these transformations must reproduce the embedding tensor components that are compatible with supersymmetry, i.e., the D(Λ) + D 1 components, and project out the remaining representation D 2 . Let us set ω = 0 for the moment, i.e., let us assume that the global symmetry group has no R + component (later we will restore ω). In this case we find As we showed in (B), the Weitzenböck connection Ω takes values in the fundamental times the adjoint of the global symmetry group, so The coefficient α must then be fixed in such a way that the tensor Q M α , N β is a linear combination of the projectors to D(Λ) + D 1 . We find corresponding in particular to α = 12 in E 7 , as stated in equation (2.9).
Let us now see how the coefficient ω can be fixed. A possibility is to demand that the intertwining tensor (i.e. the symmetric part of the gauge group generators takes values in the algebra of the global symmetry group without the R + , as explained in [35]. Here we work out the E 7 case, but the other cases follow analogously. For a generic value of ω, we can compute the general form of the symmetric part of the gauge group generators, which reads We can now use the relation (A.4), together with the fact that the 912 satisfies 16) to show that (C.15) can be written as Here the first term measures the failure of the intertwining tensor to take values in the algebra of E 7 , and in order to cancel it we must take This procedure can be repeated for any other group analogously.
In supersymmetric theories, the representation D 2 is projected out from the embed- introduced in Section 5 gives the scalar potential of maximal supergravity (5.26). To prove this we will use the following assumptions: • The spin connection is torsionless (4.17) From here it is also clear that it belongs to the 56 × 133 representation W AB C = W A α (t α ) B C . This also implies that the trace is given by • The spin connection is generalized metric compatible (4.18) Under these assumptions we will show here that the generalized Ricci scalar equals the scalar potential of maximal supergravity. Let us emphasize that we will not solve equations Note also that this is true for any torsionless and metric-compatible connection, and the concrete expression of the determined part does not need to be known. In fact, we never needed to solve for the spin connection, but only used the equation that defines it implicitly.
Finally, let us mention that the factor 7 in the scalar potential comes form a projection of the spin connection into the space of fluxes (4.16). It is known that it is fixed by supersymmetry [32], so one can wonder where does supersymmetry arise in all this analysis. This factor is actually 1/a 1 in the language of Appendix C, and it is set by supersymmetry in an indirect way. As we explained in Appendix C, the projectors to the irreducible reps of the direct product of the fundamental and the adjoint are normalized to add up to unity. Since supersymmetry projects out some reps through a linear constraint, the remaining are normalized in such a way that they capture information about supersymmetry and this is exactly how this coefficient is obtained here.