Thermal stability of radiant black holes

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Latex2e, 13 pages, 2 eps figures. Contribution to the volume to be published by the Indian Association for the Cultivation of

Scientific paper

Beginning with a brief sketch of the derivation of Hawking's theorem of horizon area increase, based on the Raychaudhuri equation, we go on to discuss the issue as to whether generic black holes, undergoing Hawking radiation, can ever remain in stable thermal equilibrium with that radiation. We derive a universal criterion for such a stability, which relates the black hole mass and microcanonical entropy, both of which are well-defined within the context of the Isolated Horizon, and in principle calculable within Loop Quantum Gravity. The criterion is argued to hold even when thermal fluctuations of electric charge are considered, within a {\it grand} canonical ensemble.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Thermal stability of radiant 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 Thermal stability of radiant black holes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Thermal stability of radiant black holes will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-721146

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.