We consider asymptotically anti-de Sitter black holes in d-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(d−2)+1 spacetime dimensions, where the
energy-momentum dispersion relation for the constituents of the fluid is
assumed to be ϵ=κpα. We examine implications of this
result for entropy bounds and the holographic hypothesis.Comment: Minor changes to match published version. 9 Pages, Revte