Investigation on the origin of black-hole entropy

Details Investigation on the origin of black-hole entropy Investigation on the origin of black-hole entropy

May 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996phrvd..53.5705w&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 53, Issue 10, 15 May 1996, pp.5705-5707

Physics

3

Quantum Aspects Of Black Holes, Evaporation, Thermodynamics

Scientific paper

The entropy bound of a self-gravitating radiation system (SGRS) confined to a spherical box with a central black hole is calculated by using the modified equation of state of radiation near the black-hole horizon, which was derived by Li and Liu. A reasonable mode of the gravitational collapse of a SGRS is given, and the collapsing process is proved to be an entropy-increasing process, throughout which the upper bound on the entropy of the whole system is equal to the entropy of the final black hole with the same mass as the system. In this way, a possible explanation for the origin of black-hole entropy is provided, which is an extension of this author's previous work.

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