Dirty black holes: Entropy as a surface term
- 15 December 1993
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review D
- Vol. 48 (12) , 5697-5705
- https://doi.org/10.1103/physrevd.48.5697
Abstract
It is by now clear that the naive rule for the entropy of a black hole, (entropy)=1/4 (area of event horizon), is violated in many interesting cases. Indeed, several authors have recently conjectured that in general the entropy of a dirty black hole might be given purely in terms of some surface integral over the event horizon of that black hole. A formal proof of this conjecture, using Lorentzian signature techniques, has recently been provided by Wald. This paper performs two functions. First, by extending a previous analysis due to the present author [Phys. Rev. D 48, 583 (1993)] it is possible to provide a rather different proof of this result—a proof based on Euclidean signature techniques.Keywords
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This publication has 10 references indexed in Scilit:
- Black hole entropy is the Noether chargePhysical Review D, 1993
- Dirty black holes: Entropy versus areaPhysical Review D, 1993
- Entropy and action of dilaton black holesPhysical Review D, 1993
- Black hole entropy and higher curvature interactionsPhysical Review Letters, 1993
- Black hole thermodynamics and quantum hairPhysical Review Letters, 1992
- Dirty black holes: Thermodynamics and horizon structurePhysical Review D, 1992
- Higher-derivative gravity, surface terms, and string theoryPhysical Review D, 1987
- Action integrals and partition functions in quantum gravityPhysical Review D, 1977
- Particle creation by black holesCommunications in Mathematical Physics, 1975
- Black Holes and EntropyPhysical Review D, 1973