77 research outputs found

    On new maximal supergravity and its BPS domain-walls

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    We revise the SU(3)-invariant sector of N=8\mathcal{N}=8 supergravity with dyonic SO(8) gaugings. By using the embedding tensor formalism, analytic expressions for the scalar potential, superpotential(s) and fermion mass terms are obtained as a function of the electromagnetic phase ω\omega and the scalars in the theory. Equipped with these results, we explore non-supersymmetric AdS critical points at ω≠0\omega \neq 0 for which perturbative stability could not be analysed before. The ω\omega-dependent superpotential is then used to derive first-order flow equations and obtain new BPS domain-wall solutions at ω≠0\omega \neq 0. We numerically look at steepest-descent paths motivated by the (conjectured) RG flows.Comment: 40 pages (30 pages + appendices), 3 tables, 6 figures. v2: References added and discussion in section 4.2 clarified. v3: References added, published version. v4: Fixed typo

    BPS black hole horizons from massive IIA

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    The maximal four-dimensional supergravity with a dyonic ISO(7) gauging that arises from the reduction of massive IIA on a six-sphere has recently been shown to accommodate static BPS black holes with hyperbolic horizons. When restricted to the N=2 subsector that retains one vector multiplet and the universal hypermultiplet, the attractor mechanism was shown to fix both the vector charges and the scalar fields at the horizon to a unique configuration in terms of the gauging parameters. In order to assess the (non-)uniqueness of BPS black hole horizons from massive IIA, we extend the study of the attractor mechanism to other N=2 subsectors including additional matter multiplets. We note that, while extending the hypermultiplet sector does not modify the set of solutions to the attractor equations, the inclusion of additional vector multiplets results in new hyperbolic/spherical horizons containing free parameters. The model with three vector multiplets and the universal hypermultiplet, which is the massive IIA analogue of the STU-model from M-theory, may play a relevant role in massive IIA holography.Comment: 18 pages, 2 figures. v2: typos fixed, notation and presentation improved, references added. v3: published versio

    Hypermultiplet gaugings and supersymmetric solutions from 11D and massive IIA supergravity on H(p,q)^{(p,q)} spaces

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    Supersymmetric  AdS4 \,\textrm{AdS}_{4}\,,  AdS2×Σ2 \,\textrm{AdS}_{2} \times \Sigma_{2}\, and asymptotically AdS4_{4} black hole solutions are studied in the context of non-minimal  N=2 \,\mathcal{N}=2\, supergravity models involving three vector multiplets (STU-model) and Abelian gaugings of the universal hypermultiplet moduli space. Such models correspond to consistent subsectors of the  SO(p,q) \,\textrm{SO}(p,q)\, and  ISO(p,q) \,\textrm{ISO}(p,q)\, gauged maximal supergravities that arise from the reduction of 11D and massive IIA supergravity on  H(p,q) \,\textrm{H}^{(p,q)}\, spaces down to four dimensions. A unified description of all the models is provided in terms of a square-root prepotential and the gauging of a duality-hidden symmetry pair of the universal hypermultiplet. Some aspects of M-theory and massive IIA holography are mentioned in passing.Comment: 10 pages, 3 tables. v2: Published version. v3: minor edits, added clarification

    CSOc_c superpotentials

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    Motivated by their application to holographic RG flows and hairy black holes in Einstein-scalar systems, we present a collection of superpotentials driving the dynamics of N=2\mathcal{N}=2 and N=1\mathcal{N}=1 four-dimensional supergravities. These theories arise as consistent truncations of the electric/magnetic families of CSO(p,q,r)c\textrm{CSO}(p,q,r)_{c} maximal supergravities, with p+q+r=8{p+q+r=8}, discovered by Dall'Agata et al. The N=2\mathcal{N}=2 and N=1\mathcal{N}=1 truncations describe SU(3)\textrm{SU}(3) and Z2×SO(3)\mathbb{Z}_{2} \times \textrm{SO}(3) invariant sectors, respectively, and contain AdS4_4 solutions preserving N=1,2,3,4\mathcal{N}=1,2,3,4 supersymmetry within the full theories, as well as various gauge symmetries. Realisations in terms of non-geometric type IIB as well as geometric massive type IIA backgrounds are also discussed. The aim of this note is to provide easy to handle superpotentials that facilitate the study of gravitational and gauge aspects of the CSO(p,q,r)c\textrm{CSO}(p,q,r)_{c} maximal supergravities avoiding the technicalities required in their construction.Comment: 10 pages, 1 table. v2: Published versio

    Dyonic ISO(7) supergravity and the duality hierarchy

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    Motivated by its well defined higher dimensional origin, a detailed study of D=4D=4 N=8\mathcal{N}=8 supergravity with a dyonically gauged ISO(7)=SO(7)⋉R7\textrm{ISO}(7) = \textrm{SO}(7) \ltimes \mathbb{R}^7 gauge group is performed. We write down the Lagrangian and describe the tensor and duality hierarchies, focusing on an interesting subsector with closed field equations and supersymmetry transformations. We then truncate the N=8\mathcal{N}=8 theory to some smaller sectors with N=2\mathcal{N}=2 and N=1\mathcal{N}=1 supersymmetry and SU(3), G2\textrm{G}_2 and SO(4) bosonic symmetry. Canonical and superpotential formulations for these sectors are given, and their vacuum structure and spectra is analysed. Unlike the purely electric ISO(7) gauging, the dyonic gauging displays a rich structure of vacua, all of them AdS. We recover all previously known ones and find a new N=1\mathcal{N}=1 vacuum with SU(3) symmetry and various non-supersymmetric vacua, all of them stable within the full N=8\mathcal{N}=8 theory.Comment: 52 pages, 4 tables. v2: Section 2.4 on critical points added. v3: Version published in JHE

    BPS black holes from massive IIA on S6^6

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    We present BPS black hole solutions in a four-dimensional N=2\mathcal{N}=2 supergravity with an abelian dyonic gauging of the universal hypermultiplet moduli space. This supergravity arises as the SU(3)-invariant subsector in the reduction of massive IIA supergravity on a six-sphere. The solutions are supported by non-constant scalar, vector and tensor fields and interpolate between a unique AdS2 × H2\textrm{AdS}_{2} \,\times\, \textrm{H}^2 geometry in the near-horizon region and the domain-wall DW4_{4} (four-dimensional) description of the D2-brane at the boundary. Some special solutions with charged AdS4_{4} or non-relativistic scaling behaviours in the ultraviolet are also presented.Comment: 20 pages, 4 figures and 1 appendix. v2: New appendix, comments and references added, published versio

    A second look at gauged supergravities from fluxes in M-theory

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    We investigate reductions of M-theory beyond twisted tori by allowing the presence of KK6 monopoles (KKO6-planes) compatible with N=4 supersymmetry in four dimensions. The presence of KKO6-planes proves crucial to achieve full moduli stabilisation as they generate new universal moduli powers in the scalar potential. The resulting gauged supergravities turn out to be compatible with a weak G2 holonomy at N=1 as well as at some non-supersymmetric AdS4 vacua. The M-theory flux vacua we present here cannot be obtained from ordinary type IIA orientifold reductions including background fluxes, D6-branes (O6-planes) and/or KK5 (KKO5) sources. However, from a four-dimensional point of view, they still admit a description in terms of so-called non-geometric fluxes. In this sense we provide the M-theory interpretation for such non-geometric type IIA flux vacua.Comment: 46 pages. Published version. Minor changes, references adde

    KK-monopoles and G-structures in M-theory/type IIA reductions

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    We argue that M-theory/massive IIA backgrounds including KK-monopoles are suitably described in the language of G-structures and their intrinsic torsion. To this end, we study classes of minimal supergravity models that admit an interpretation as twisted reductions in which the twist parameters are not restricted to satisfy the Jacobi constraints ω ω=0\omega\, \omega=0 required by an ordinary Scherk-Schwarz reduction. We first derive the correspondence between four-dimensional data and torsion classes of the internal space and, then, check the one-to-one correspondence between higher-dimensional and four-dimensional equations of motion. Remarkably, the whole construction holds regardless of the Jacobi constraints, thus shedding light upon the string/M-theory interpretation of (smeared) KK-monopoles.Comment: 38 pages, 1 figure, 1 table; v2: refs added, published versio
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