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- W1993942005 abstract "We consider the entropy of a quantum scalar field on a background black hole geometry in asymptotically anti--de Sitter space-time, using the ``brick wall'' approach. In anti--de Sitter space, the theory has no infrared divergences, and all ultraviolet divergences can be absorbed into a renormalization of the coupling constants in the one-loop effective gravitational Lagrangian. We then calculate the finite renormalized entropy for the Schwarzschild--anti-de Sitter and extremal Reissner--Nordstrom--anti-de Sitter black holes, and show that, at least for large black holes, the entropy is entirely accounted for by the one-loop Lagrangian, apart possibly from terms proportional to the logarithm of the event horizon radius. For small black holes, there are indications that non-perturbative quantum gravity effects become important." @default.
- W1993942005 created "2016-06-24" @default.
- W1993942005 creator A5047124264 @default.
- W1993942005 date "2001-03-22" @default.
- W1993942005 modified "2023-09-27" @default.
- W1993942005 title "Renormalized black hole entropy in anti–de Sitter space via the “brick wall” method" @default.
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- W1993942005 doi "https://doi.org/10.1103/physrevd.63.084013" @default.
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