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Black Holes with Scalar Hair and Asymptotics in N=8 Supergravity

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arxiv hep-th/0404261 v3 pith:BXMSLOYY submitted 2004-04-30 hep-th gr-qc

classification hep-thgr-qc
keywords blackboundaryconditionsholeholesscalarads-invariantasymptotic
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

We consider N=8 gauged supergravity in D=4 and D=5. We show one can weaken the boundary conditions on the metric and on all scalars with $m^2 <-{(D-1)^2 \over 4}+1$, while preserving the asymptotic anti-de Sitter (AdS) symmetries. Each scalar admits a one-parameter family of AdS-invariant boundary conditions for which the metric falls off slower than usual. The generators of the asymptotic symmetries are finite, but generically acquire a contribution from the scalars. For a large class of boundary conditions we numerically find a one-parameter family of black holes with scalar hair. These solutions exist above a certain critical mass and are disconnected from the Schwarschild-AdS black hole, which is a solution for all boundary conditions. We show the Schwarschild-AdS black hole has larger entropy than a hairy black hole of the same mass. The hairy black holes lift to inhomogeneous black brane solutions in ten or eleven dimensions. We briefly discuss how generalized AdS-invariant boundary conditions can be incorporated in the AdS/CFT correspondence.

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Cited by 3 Pith papers

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