Entropy of self-gravitating radiation systems and gravitational collapse

Details Entropy of self-gravitating radiation systems and gravitational collapse Entropy of self-gravitating radiation systems and gravitational collapse

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996cha%26a..20..267w&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 20, Issue 3, p. 267-272.

Astronomy and Astrophysics

Astrophysics

Scientific paper

The entropy of a self-gravitating and radiating system confined to a spherical box (for two cases with and without a central black hole) is calculated using the equation of state of radiation near the black hole horizon, derived by Li Li-xin and Liu Liao. Unlike the result of Sorkin et al., the present result contains no divergence difficulties and the upper bound on the total entropy in the case with a central black hole is equal to the entropy of a black hole having the same mass. The following scenario is considered reasonable: a central black hole forms first, it then grows until all the radiation and matter falls into the black hole. The entropy of the system at any stage of the collapse is always less than the entropy of the final black hole, thus providing an explanation of the origin of the black hole entropy.

Affiliated with

Also associated with

No associations

Rating

Entropy of self-gravitating radiation systems and gravitational collapse does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Entropy of self-gravitating radiation systems and gravitational collapse, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Entropy of self-gravitating radiation systems and gravitational collapse will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1154343