Gravitational entropy: Beyond the black hole

P. C.W. Davies, L. H. Ford, D. N. Page

Research output: Contribution to journalArticle

35 Scopus citations

Abstract

We attempt to establish the existence of gravitational entropy for a thin spherical shell of matter as a function of radius by examining the modifications to the thermodynamics of a black hole at the center of such a shell. We show that the shell has the effect of depressing the temperature of the hole, but that small exchanges of energy between the hole and its environment at the same temperature remain isentropic in the presence of the shell. The model is generalized to include de Sitter horizons too, and we find that the shell can be positioned so that a back flow of radiation takes place from the de Sitter horizon into the hole, thus enabling the hole-plus-shell system to be used as a device for mining the Universe. In all cases our results are consistent with simple arguments indicating that there is no gravitational entropy associated with spherical shells which have not collapsed into black holes.

Original languageEnglish (US)
Pages (from-to)1700-1707
Number of pages8
JournalPhysical Review D
Volume34
Issue number6
DOIs
StatePublished - Jan 1 1986
Externally publishedYes

ASJC Scopus subject areas

  • Nuclear and High Energy Physics
  • Physics and Astronomy (miscellaneous)

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