2017
DOI: 10.1007/jhep09(2017)141
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BPS black holes from massive IIA on S6

Abstract: We present BPS black hole solutions in a four-dimensional 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 AdS 2 × H 2 geometry in the near-horizon region and the domain-wall DW 4 (four-dimensional) description of the D2-brane at the boun… Show more

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Cited by 34 publications
(71 citation statements)
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“…The field theory spectra have been partially determined holographically [28,29], and solutions of various types have been constructed in the gauged supergravity. These include domain-walls [27,30], defects [31] or black holes, both the full asymptotically-AdS geometries [32,33] and their near-horizon regions [34]. These solutions are all in perfect agreement with the corresponding field theory predictions.…”
Section: Motivationmentioning
confidence: 54%
“…The field theory spectra have been partially determined holographically [28,29], and solutions of various types have been constructed in the gauged supergravity. These include domain-walls [27,30], defects [31] or black holes, both the full asymptotically-AdS geometries [32,33] and their near-horizon regions [34]. These solutions are all in perfect agreement with the corresponding field theory predictions.…”
Section: Motivationmentioning
confidence: 54%
“…Thus, not only the black hole considered in [12] uplifts to D = 10, but in fact any other solution of minimal N = 2 supergravity does through those consistent embedding formulae. For example, the SU(3)-invariant, supersymmetric Reissner-Nordström black hole with constant scalars discussed in [75,76] can be more economically regarded as a solution of minimal N = 2 gauged supergravity. Also this black hole uplifts to IIA using the same formulae in [12] and section 4.1 here, as any other solution, supersymmetric or otherwise, of minimal D = 4 N = 2 supergravity does.…”
Section: Discussionmentioning
confidence: 99%
“…Since our line of reasoning did not require the explicit solution beyond the AdS 4 boundary conditions, it should be straightforward to generalize these arguments to theories with charged hypermultiplets where solutions are harder to find [40][41][42][43][44][45] but there are more avenues for embedding such theories into string or M-theory. It would also seem likely that our methods will generalize to asymptotically AdS solutions in other dimensions.…”
Section: Discussionmentioning
confidence: 99%