Abstract

We consider asymptotically anti-de Sitter black holes in dd-spacetime dimensions in the thermodynamically stable regime. We show that the Bekenstein-Hawking entropy and its leading order corrections due to thermal fluctuations can be reproduced by a weakly interacting fluid of bosons and fermions (`dual gas') in Δ=α(d2)+1\Delta=\alpha(d-2)+1 spacetime dimensions, where the energy-momentum dispersion relation for the constituents of the fluid is assumed to be ϵ=κpα\epsilon = \kappa p^\alpha. We examine implications of this result for entropy bounds and the holographic hypothesis.Comment: Minor changes to match published version. 9 Pages, Revte

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    Last time updated on 01/04/2019