SAdS black holes and spacetime atoms: a heuristic approach
arXiv:1712.01159 · doi:10.1007/s10714-018-2442-9
Abstract
In this work, both extended phase space and holographic equipartition approaches are employed to develop an exact Van der Waals description of non--rotating SAdS black holes as an ensemble of spacetime atoms. After a possible microscopical interaction model is introduced, statistical mechanics techniques, with certain heuristic gravitational constraints, are used to derive the equation of state and the Bekenstein--Hawking entropy. The procedure is generalized to the charged SAdS black hole and to arbitrary dimensions for the uncharged cases.
arXiv commentAccepted for publication in Gen. Rel. Grav
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