Entropy of self-gravitating radiation systems and the entropy of black holes

Details Entropy of self-gravitating radiation systems and the entropy of black holes Entropy of self-gravitating radiation systems and the entropy of black holes

Dec 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994phrvd..50.7385w&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 50, Issue 12, 15 December 1994, pp.7385-7388

Mathematics

Dynamical Systems

10

Quantum Aspects Of Black Holes, Evaporation, Thermodynamics, Other Topics In Statistical Physics, Thermodynamics, And Nonlinear Dynamical Systems

Scientific paper

The entropy of a self-gravitating radiation system (SGRS) confined to a spherical box is calculated by using the equation of state of radiation near the black-hole horizon, which was derived by Li and Liu. Compared with the result given by Sorkin, Wald, and Zhang, there is no divergence problem with the result of this paper. Furthermore, the upper bound on the entropy of SGRS's is exactly equal to the corresponding black-hole entropy. In this way, an explanation for the origin of black-hole entropy is provided.

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