Stability of thermal equilibrium for a radiating black hole in a box.
Abstract
The Hawking criterion for the stability of thermodynamical equilibrium between a Schwarzschild black hole and its own radiation is refined by the use of Page's expression for the renormalized stress-energy tensor.
- Publication:
-
General Relativity and Gravitation
- Pub Date:
- June 1984
- DOI:
- 10.1007/BF00769629
- Bibcode:
- 1984GReGr..16..563P
- Keywords:
-
- Black Holes (Astronomy);
- Schwarzschild Metric;
- Thermal Radiation;
- Thermodynamic Equilibrium;
- Black Body Radiation;
- Plancks Constant;
- Tensor Analysis;
- Thermal Stability;
- Astrophysics;
- Black Holes:Thermal Radiation