Non-semisimple gauging of a magical N = 4 supergravity in three dimensions

We construct a new N = 4 non-semisimple gauged supergravity in three dimensions with E6(2)/SU(6) × SU(2) scalar manifold and SO(4) ⋉ T6 gauge group. Depending on the values of the gauge coupling constants, the theory admits both the maximally supersymmetric AdS3 vacuum preserving SO(4) gauge symmetry and half-supersymmetric domain walls with unbroken SO(4) symmetry. We give all scalar masses at the supersymmetric AdS3 critical point corresponding to an N = (4, 0) superconformal field theory (SCFT) in two dimensions. The scalar potential also admits two flat directions corresponding to marginal deformations that preserve full supersymmetry and conformal symmetry. This SO(4) ⋉ T6 gauged supergravity is expected to arise from a dimensional reduction on a three-sphere of the minimal N = (1, 0) supergravity in six dimensions coupled to three tensor and four vector multiplets.


Introduction
Gauged supergravities in various dimensions play an important role in many aspects of string/M theory in particular the AdS/CFT correspondence [1]. Unlike higher dimensional analogues, gauged supergravity in three dimensions has a much richer structure due to the duality between vectors and scalars. Since three-dimensional supergravity fields are topological, the propagating bosonic degrees of freedom of the matter-coupled supergravity can be described entirely in terms of scalar fields. The resulting theory is a supersymmetric non-linear sigma model coupled to supergravity. All of these theories with different numbers (N ) of supersymmetries have been classified in [2]. For N > 4, scalar fields must be described by a symmetric space of the form G/H in which G and H are global and local symmetries, respectively. The latter is the maximal compact subgroup of G and takes the form SO(N ) × H ′ with SO(N ) being the R-symmetry group.
Gauged supergravity can be constructed by introducing gauge vector fields via Chern-Simons (CS) terms which are topological in nature. This CS formulation makes the connection to usual Yang-Mills (YM) gauged supergravities, in which gauge fields appear via YM kinetic terms, obscure. Furthermore, since conventional dimensional reductions result in YM gauged supergravities, the embedding of these CS gauged supergravities in higher dimensions is then a non-trivial task. However, it has been shown that CS gauged supergravity with a non-semisimple gauge group G 0 ⋉ T dimG 0 is on-shell equivalent to YM JHEP12(2015)153 gauged supergravity with G 0 gauge group [3]. The T dimG 0 factor is a nilpotent translational group transforming in the adjoint representation of a semisimple group G 0 . Therefore, at least some of these particular gauge groups might have higher dimensional origins in terms of known dimensional reductions. Since the embedding in higher dimensions is necessary for interpreting three-dimensional solutions in string/M-theory context, CS gauged supergravities with non-semisimple gauge groups are of particular interest in the AdS/CFT correspondence.
Until now, a number of works considering CS gauged supergravity with non-semisimple gauge groups and their application in the AdS/CFT correspondence have appeared [4][5][6][7][8][9][10][11][12]. All of these gauged supergravities are expected to arise from dimensional reductions of higher dimensional theories, and explicit reduction ansatze for obtaining three-dimensional gauged supergravities from a three-sphere reduction, both the full S 3 reduction and SU (2) group manifold reduction, have been constructed in [13][14][15][16]. Furthermore, a number of N = 2 gauged supergravities with abelian gauge groups have also been obtained from wrapped branes in type IIB and M-theory [17][18][19].
In this paper, we construct new N = 4 gauged supergravity with E 6(2) /SU(6) × SU(2) scalar manifold and SO(4) ⋉ T 6 gauge group. According to the result of [3], the resulting gauged supergravity is equivalent to SO(4) YM gauged supergravity. A number of possible semisimple gaugings of this theory have already been classified in [8]. In the present work, we will study possible non-semisimple gauge groups and also classify supersymmetric vacua of the gauged supergravity both maximally supersymmetric and half-supersymmetric with the full SO(4) symmetry unbroken. These would be useful in AdS 3 /CFT 2 correspondence.
The theory considered here is one of the magical supergravities in three dimensions, see [20][21][22] for higher dimensional magical supergravities. In [8], another SO(4) ⋉ T 6 gauged magical supergravity with F 4(4) /USp(6) × SU(2) scalar manifold has been studied. This theory is expected to arise from an S 3 reduction of N = (1, 0) supergravity in six dimensions coupled to two vector and two tensor multiplets. In the present case, we expect the new SO(4) ⋉ T 6 gauged theory with E 6(2) /SU(6) × SU(2) scalar manifold to arise from an S 3 reduction of this N = (1, 0) supergravity coupled to four vector and three tensor multiplets. Both of these six-dimensional supergravities are also magical supergravities, and the possible gaugings have been systematically considered in [23] using the embedding tensor formalism.
The paper is organized as follow. In section 2, we review N = 4 three-dimensional gauged supergravity with symmetric scalar target spaces. We mainly focus on a specific case of exceptional coset E 6(2) /SU(6) × SU(2). In section 3, the embedding tensor of SO(4) ⋉ T 6 is given. We then study the resulting scalar potential for the SO(4) singlet scalars and identify some of their possible supersymmetric vacua. We end the paper by giving some conclusions and comments on a possible higher dimensional origin of the gauged supergravity constructed here in section 4. Two appendices with some useful formulae are also included.

JHEP12(2015)153
2 N = 4 gauged supergravity in three dimensions with E 6(2) /SU(6) × SU(2) scalar manifold Three dimensional matter-coupled supergravity is given by a nonlinear sigma model coupled to supergravity. Scalar fields will be denoted by φ i , i = 1, . . . , d with d being the dimension of the scalar target space. Throughout this paper, we will work in the SO(N ) covariant formulation of [24]. Coupling the non-linear sigma model to N extended supergravity requires N −1 almost complex structures, denoted by f P i j , P = 2, . . . N , on the target space of the sigma model. The R-symmetry in three dimensions is given by SO(N ) under which scalars transform in a spinor representation. The tensor f IJ , I, J = 1, . . . N , generating SO(N ) R-symmetry in this spinor representation, can be constructed from f P via For N = 4 theory, the scalar target space must be a quaternionic manifold. Special to N = 4 supersymmetry, there exists a tensor J = 1 6 ǫ P QR f P f Q f R that commutes with the almost complex structures and is covariantly constant. This implies the product structure of the target space. Therefore, a general N = 4 matter-coupled supergravity admits a scalar manifold of the form M = M − × M + with a total dimension d = d + + d − . The full SO(4) ∼ SO(3) − × SO(3) + R-symmetry will split into each factor of the full target space. In this paper, we are however only interested in the so-called degenerate case with only one factor of M present. For definiteness, we will consider a non-vanishing M + by setting d − = 0. Furthermore, we will restrict ourselves to only a symmetric target space of the form G/H although this is not in general a requirement from N = 4 supersymmetry.
The symmetric target space of the form G/H has a global symmetry G and a local symmetry H given by its maximal compact subgroup. In general, the local symmetry H contains the SO(N ) R-symmetry and takes the form H = SO(N ) × H ′ . But, for the N = 4 theory, we have the compact group H ± = SO(3) ± × H ′ ± ∼ SU(2) ± × H ′ ± for each subspace M ± . In the present case, the scalar target space is given by E 6(2) /SU(6) × SU(2) of dimension 40.

JHEP12(2015)153
The metric on the target space g ij can be computed from the vielbein e A i by the usual relation g ij = e A i e B j δ AB . Here, indices A, B = 1, . . . 40 can be considered as "flat" target space indices.
Gaugings are implemented by a symmetric and gauge invariant tensor called the embedding tensor Θ MN [25,26]. A viable gauging consistent with supersymmetry is characterized by the embedding tensor that satisfies two consistency conditions. The first condition, called the quadratic constraint, requires that the gauge group is a proper subgroup of the global symmetry G. This constraint is explicitly given by where f KL M are the G-structure constants. Furthermore, supersymmetry requires that the T-tensor defined by the image of the embedding tensor under a map V satisfies the constraint The T-tensor transforms under the local H symmetry with the index A = {IJ, α, A}. The above constraint implies that the ⊞ representation of SO(N ) is absent from the T IJ,KL component of the T-tensor. Therefore, we can equivalently write this constraint as In the case of symmetric target spaces, the condition (2.7) can be expressed as a consistency condition on the embedding tensor which lives in a symmetric product of the adjoint representation of G. It turns out that under the decomposition of this product into irreducible representations of G, there is a unique representation of G, called R 0 , which gives rise to the SO(N ) representation ⊞ under the branching G → SO(N ). Therefore, in this case, the constraint (2.7) can be written in a G-covariant way by In the case of G = E 6(2) , the representation R 0 is given by 2430 [24]. In addition, for symmetric spaces in the form of a coset space, the map V will be an isomorphism, and its components are given by the relation Various components of the T-tensor can be straightforwardly computed from the embedding tensor by using the definition (2.5) and the map V from (2.9). Combinations of these T-tensor components are used to construct the A 1 , A 2 and A 3 tensors which will appear as fermion mass-like terms and the scalar potential in the gauged Lagrangian. They

JHEP12(2015)153
are defined by where D i is the covariant derivative with respect to φ i . In terms of these tensors, the scalar potential can be written as As a final ingredient, we give the supersymmetry transformations of the gravitini ψ I µ and the spinor fields χ iI , involving only bosonic fields, where the covariant derivative of ǫ I is given by The covariant derivative on scalars φ i is defined by with X N i being the Killing vectors associated to the isometries of G/H. Note that there are only d physical χ i fields in consistent with d scalar fields φ i as required by supersymmetry. In order to work with the SO(N ) covariant formulation of [24], in which the explicit dependence on f P is absent, the χ i fields have been written in terms of the constrained fields χ iI satisfying We finally note here that, for maximally symmetric vacua, the unbroken supersymmetry corresponds to Killing spinors ǫ I satisfying the relation This relation can be derived by solving the BPS conditions δψ I µ = 0 and δχ iI = 0 at constant scalars, see the relevant detail in [24].

JHEP12(2015)153
3 N = 4, SO(4) ⋉ T 6 gauged supergravity and some supersymmetric vacua We first give an explicit construction of the E 6(2) /SU(6) × SU(2) coset space. Generators of the compact H = SU(6) × SU(2) subgroup and the 40 non-compact generators are given in appendix A. We first describe the embedding of SO(4) ⋉ T 6 gauge group in the global symmetry group E 6(2) . In order to do this, we will decompose E 6(2) into its maximal subgroup SO(6, 4) × U(1) generated byXîĵ andX given explicitly in appendix A. The full gauge group SO(4) ⋉ T 6 can be embedded in SO(6, 4) as follow.
The semisimple part SO(4) is given by a diagonal subgroup of SO(4) × SO(4) ⊂ SO(6) × SO(4) which is in turn the maximal compact subgroup of SO (6,4). This SO(4) is accordingly generated by The other combinationX ab −X a+6,b+6 together with a suitable set of non-compact generators will give rise to the translational generators T 6 transforming as an adjoint representation of the above mentioned SO(4). All of the T 6 generators also commute with each other. In order to identify the appropriate non-compact generators constituting T 6 , we decompose the Y A generators under the SO(4) part of the gauge group. Under SU(6)×SU(2), the 40 generators Y A transform as (20,2). Under SU (6) From now on, we will neglect all the U(1) charges since they will not play any important role in the following analysis. We now decompose SU(4) ∼ SO ( where we have denoted the SO(4) ∼ SU(2) × SU(2) representations by (2j 1 + 1, 2j 2 + 1) with j 1 , j 2 corresponding to the spins of the two SU(2)'s. The last two representations in (3.3) are the adjoint representation of SO(4) diag . These will be part of the gauge generators T 6 . Explicitly, we find that these generators are given by t ab =X ab −X a+6,b+6 +X a,b+6 +X a+6,b , a, b = 1, . . . , 4 .

JHEP12(2015)153
The non-vanishing components of the embedding tensor corresponding to the full gauge group are denoted by Θ ab and Θ bb with a and b associated to the J ab and t ab parts, respectively [3]. It turns out that the embedding tensor satisfying the linear and quadratic constraints given in (2.4) and (2.8) is given by where both Θ ab ab,cd and Θ bb ab,cd are given by ǫ abcd . This is much similar to the N = 8 and N = 4 theories studied in [6] and [8]. It should be noted that supersymmetry allows for two independent coupling constants.

Maximally supersymmetric vacua with SO(4) symmetry
We now consider some vacua of the N = 4 gauged supergravity constructed previously. From equation (3.3), we see that there are three scalars which are singlets under SO(4). These singlets correspond to the following non-compact generatorŝ The coset representative L can be parametrized by By using the formulae in section 2 and appendix B, we obtain the scalar potential for (Φ 1 , Φ 2 , Φ 3 ) given by From this potential, it can be readily verified that the SO(4) ⋉ T 6 gauged supergravity admits a maximally supersymmetric AdS 3 critical point. By shifting the values of scalar fields at the vacuum, we can bring the critical point to L = I 27×27 at which Φ 1 = Φ 2 = Φ 3 = 0. This can also be achieved by setting g 2 = g 1 = g. The cosmological constant at the critical point is given by V 0 = −1024g 2 . In our convention, the AdS 3 radius is given by where we have taken g > 0 for definiteness. It can be checked by using the supersymmetry transformations (2.14) and (2.15) or the relation (2.19) that this critical point preserves the full eight supercharges corresponding to N = (4, 0) superconformal symmetry in the dual two-dimensional SCFT. This gives supersymmetric Minkowski vacua in three dimensions with V 0 = 0.

Half-supersymmetric domain walls
We now move to half-supersymmetric vacuum solutions. To find these solutions, we set up the corresponding BPS equations from the supersymmetry transformations (2.14) and (2.15). The three-dimensional metric is taken to be the standard domain wall ansatz With the projection γ r ǫ I = −ǫ I corresponding to N = (4, 0) supersymmetry in two dimensions, equations δχ iI = 0 and δψ I µ = 0 for µ = 0, 1 give 17) where ′ denotes the r-derivative. All of these equations satisfy the second-order field equations. Some details of this verification is given in appendix C. We first consider the case Φ 1 = Φ 2 = 0. It can be readily seen that the first two equations are identically satisfied. We are left with two equations For g 2 = 0, the Φ ′ 3 equation has a critical point at Φ 3 = 1 2 ln g 2 g 1 while the A ′ equation gives A = 32g 2 1 g 2 r + C. This is the maximally supersymmetric AdS 3 critical point identified previously.
Equations (3.18) and (3.19) can be solved explicitly with the corresponding solution It should be noted that the integration constants C 2 and C 1 can be removed by shifting the coordinate r and rescaling the x 0 and x 1 coordinates, respectively. The solution interpolates between N = 4AdS 3 critical point at r → ∞ to a half-supersymmetric domain wall at a finite value of r. At large |Φ 3 |, we find with C being a constant. We have set g 2 = g 1 for simplicity. The metric at r ∼ C 32g 1 becomes ds 2 = (C − 32g 1 r) −2 dx 2 1,1 + dr 2 (3.22) which takes the form of a domain wall. However, the scalar potential becomes unbounded when Φ 3 → −∞. The singularity of the above metric is then unphysical by the criterion of [27]. Therefore, the holographic interpretation of the solution as an RG flow between an N = (4, 0) SCFT and an N = (4, 0) non-conformal field theory in two dimensions cannot be given at least in the three-dimensional framework. It would be interesting to further investigate the singularity in the context of higher dimensions in which this solution is embedded. Note also that since the operator dual to Φ 3 is irrelevant, we would expect the N = (4, 0) SCFT to appear in the IR. There is another simple exact solution to equations (3.14), (3.15), (3.16) and (3.17) namely

JHEP12(2015)153
This solution corresponds to a marginal deformation of the supersymmetric AdS 3 critical point. We now move to another type of domain walls which is a half-supersymmetric vacuum of the theory without any limit with enhanced supersymmetry. Recall that supersymmetry allows for two independent gauge couplings g 1 and g 2 , by setting g 2 = 0, we also have a consistent gauged supergravity. In this case, the resulting gauged supergravity possesses a half-supersymmetric domain wall vacuum. We will present a simple solution of this type. With Φ 1 = Φ 2 = g 2 = 0, the BPS equations become which admit a solution with an integration constant C ′ . This solution gives a domain wall metric For Φ 2 = 0 which satisfies equation (3.15), a more general solution can be found by treating Φ 1 as an independent variable. After combing equations (3.16) and (3.17) with (3.14), we can solve for Φ 3 and A as functions of Φ 1 . The result is then substituted in equation (3.14) to find the solution for Φ 1 (r). The resulting solution is given by In the above equations, we have neglected additive integration constants in Φ 1 (r) and A(Φ 1 ) solutions. Apart from these solutions, we are not able to completely solve the BPS equations with all scalars non-vanishing in an analytic form. We will however give a partial result on this solution since it might be useful for further investigation. It turns out that combining equations (3.14) and (3.15) gives an equation for Φ 2 as a function of Φ 1 with a solution If all of the integration constants are set to zero, a simple solution for Φ 3 can also be found With these relations, equation (3.17) would in principle give a solution for A(Φ 1 ) while equation (3.14) would give a solution for Φ 1 (r). We have not succeeded in obtaining an analytic form for these solutions.

Conclusions
In this paper, we have constructed N = 4 gauged supergravity in three dimensions with SO(4)⋉T 6 gauge group and E 6(2) /SU(6)×SU(2) scalar manifold. We have studied some of the maximally supersymmetric and half-supersymmetric vacua of this gauged supergravity. The N = 4AdS 3 critical point with SO(4) symmetry corresponds to an N = (4, 0) SCFT in two dimensions. We have given the full scalar mass spectrum at this critical point which might be useful for other holographic applications. In addition, some half-supersymmetric domain wall solutions have also been explicitly given in an analytic form. According to the DW/QFT correspondence [28], we expect these solutions to be dual to N = (4, 0) non-conformal field theories in two dimensions. We have also identified two flat directions of the scalar potential corresponding to exactly marginal deformations of the N = (4, 0) SCFT that preserve all supersymmetries and SO(4) symmetry. Remarkably, these flat directions are not Goldstone bosons. This is in contrast to the four-dimensional N = 4 gauged supergravity studied in [29]. In that case, all flat directions correspond to Goldstone bosons. It would be interesting to identify the N = (4, 0) SCFT and two-dimensional non-conformal field theories dual to the vacua identified here. Further investigations of the scalar potential in other scalar sectors invariant under smaller residual gauge symmetry could be useful for the study of other deformations of the dual N = (4, 0) SCFT in particular relevant deformations given by scalars in (1,3), (2,2) and (3,3) representations.
Due to the equivalence between the gauged supergravity constructed here and the Yang-Mills gauged supergravity with SO(4) gauge group, it is possible that this theory might be obtained from higher dimensions. The ungauged N = 4 supergravity with E 6(2) /SU(6) × SU(2) scalar manifold can be obtained from a reduction on a 3-torus (T 3 ) of the minimal supergravity in six dimensions coupled to three tensor and four vector multiplets. The three tensor multiplets consist of three scalars parametrized by the SO(3, 1)/SO(3) coset manifold. After dimensional reduction and dualization of the vector fields coming from the six-dimensional metric and the (anti) self-dual tensor fields, the resulting three-dimensional supergravity consists of 40 scalars as required by the dimension of E 6(2) /SU(6) × SU(2) coset manifold.
We then expect that the SO(4) ⋉ T 6 gauged supergravity constructed here should arise from a dimensional reduction of this six-dimensional supergravity on a 3-shpere (S 3 ). Along the line of this uplifting, it could be useful to compute vector and fermion masses and match with the AdS 3 × S 3 spectrum of N = (1, 0) six-dimensional supergravity carried JHEP12(2015)153 out in [32]. It should also be remarked here that, when coupled to hypermultiplets with hyper-scalars described by M − manifold, the six-dimensional supergravity could give rise to three-dimensional gauged supergravity with two scalar target manifolds M + × M − . It would be interesting to construct an explicit reduction ansatz similar to the recent result in [16]. The result will be very useful in uplifting the three-dimensional solutions to higher dimensions. We leave this issue and related ones for future works.

JHEP12(2015)153 B Essential formulae
For a general symmetric space of the form G/H with G and H = SO(N ) × H ′ being the global and local symmetry groups, the G algebra is given by C αβ is an invariant tensor of H ′ , and h α AB are antisymmetric tensors that commute with f IJ AB . Using the above algebra, we find that components of f IJ tensor written in flat coset space indices are given by In term of the coset representative, various components of the V map can be computed by using the relations From these relations, the tensors A IJ 1 , A IJ 2i and the scalar potential can be straightforwardly computed.

C Field equations for SO(4) singlet scalars and the metric
In this appendix, we explicitly verify that the BPS equations given in (3.14), (3.15), (3.16), and (3.17) indeed satisfy the corresponding second-order field equations. With only scalar fields and the metric, the Lagrangian of the gauged supergravity read, in our convention, where the scalar potential is given in (3.9). The scalar kinetic term is written in term of the coset vielbein e A i as It should be noted that, with the relation g ij = e A i e A j , the scalar kinetic term is the same as that given in [24] − 1 2 P A µ P Aµ = −

JHEP12(2015)153
In the present case, the coset vielbein can be computed from (2.3) For completeness, we will explicitly give the result here Einstein's equation coming from the above Lagrangian is given by The resulting equations are quite complicated, so we refrain from giving their explicit form here. It can however be verified that all of these equations are satisfied by the BPS equations (3.14), (3.15), (3.16), and (3.17).
Open Access. This article is distributed under the terms of the Creative Commons Attribution License (CC-BY 4.0), which permits any use, distribution and reproduction in any medium, provided the original author(s) and source are credited.