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Microscopic origin of the Bekenstein-Hawking entropy of supersymmetric AdS$_{\bf 5}$ black holes

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arxiv 1810.11442 v4 pith:3QYNR7DX submitted 2018-10-26 hep-th

Alejandro Cabo-Bizet , Davide Cassani , Dario Martelli , Sameer Murthy This is my paper · ORCID
classification hep-th
keywords blackentropysupersymmetricconstraintholebekenstein-hawkingchemicalcomplexified
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

We present a holographic derivation of the entropy of supersymmetric asymptotically AdS$_5$ black holes. We define a BPS limit of black hole thermodynamics by first focussing on a supersymmetric family of complexified solutions and then reaching extremality. We show that in this limit the black hole entropy is the Legendre transform of the on-shell gravitational action with respect to three chemical potentials subject to a constraint. This constraint follows from supersymmetry and regularity in the Euclidean bulk geometry. Further, we calculate, using localization, the exact partition function of the dual $\mathcal{N}=1$ SCFT on a twisted $S^1\times S^3$ with complexified chemical potentials obeying this constraint. This defines a generalization of the supersymmetric Casimir energy, whose Legendre transform at large $N$ exactly reproduces the Bekenstein-Hawking entropy of the black hole.

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