A comment on fluctuations and stability limits with application to superheated black holes

Details A comment on fluctuations and stability limits with application to superheated black holes A comment on fluctuations and stability limits with application to superheated black holes

1994-12-13

arxiv.org/abs/gr-qc/9412038v1

Class.Quant.Grav.12:443-448,1995

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

Scientific paper

10.1088/0264-9381/12/2/013

We point out that, contrary to signs of heat capacities, thermodynamic fluctuations are simply and unequivocally related to onset of instabilities that show up near critical points. Fluctuation theory is then applied to \Schw\ \bh s surrounded by radiation. This shows that slowly evolving \bh s along quasi-equilibrium states in cavities greater than $10^6$ Planck length will not evaporate below the critical Hawking limit temperature despite the fact that pure radiation has a much higher entropy. (CQG in press, figure request to okamoto@gprx.miz.nao.ac.jp)

Affiliated with

Also associated with

No associations

Rating

A comment on fluctuations and stability limits with application to superheated black holes 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 A comment on fluctuations and stability limits with application to superheated black holes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A comment on fluctuations and stability limits with application to superheated black holes will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-556207