Stability of thermal equilibrium for a radiating black hole in a box

Details Stability of thermal equilibrium for a radiating black hole in a box Stability of thermal equilibrium for a radiating black hole in a box

Jun 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984gregr..16..563p&link_type=abstract

General Relativity and Gravitation (ISSN 0001-7701), vol. 16, June 1984, p. 563-568. Research supported by the University of Alb

Astronomy and Astrophysics

Astronomy

10

Black Holes (Astronomy), Schwarzschild Metric, Thermal Radiation, Thermodynamic Equilibrium, Black Body Radiation, Plancks Constant, Tensor Analysis, Thermal Stability

Scientific paper

The Hawking criterion for the stability of the thermodynamical equilibrium between a Schwarzschild black hole and its own radiation (E rad less than 1/4 M) is refined theoretically by means of Page's expression for the renormalized stress tensor. The numerical procedure whereby the masses of two Schwarzschild black holes m1 and m2 have approximately equal masses is reformulated so that m2 has much greater mass than m1. It is found that the Hawking criterion remains an adequate approximation of stability even for Planck-mass black holes and for box radii comparable with the size of the black hole.

Affiliated with

Also associated with

No associations

Rating

Stability of thermal equilibrium for a radiating black hole in a box 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 Stability of thermal equilibrium for a radiating black hole in a box, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stability of thermal equilibrium for a radiating black hole in a box will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1854384