Thermodynamic stability of Kerr black holes

Details Thermodynamic stability of Kerr black holes Thermodynamic stability of Kerr black holes

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993phrvd..47.2234k&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 47, Issue 6, 15 March 1993, pp.2234-2241

Physics

35

Classical General Relativity, Thermodynamics, Relativity And Gravitation, Black Holes

Scientific paper

Isolated Kerr black holes are thermodynamically stable with respect to axisymmetric perturbations. Holes in a heat bath may be stable with large enough angular momentum. Isolated or not, at a fixed angular velocity divided by the temperature they are all unstable. The stability of the ``inner horizons'' has also been considered. Isolated inner horizons are stable. With different constraints, they are either stable or unstable. The analysis concerns pure black holes. Thermal radiation around black holes is treated as one of their possible circumstances. The effects of back reaction on the metric and nonconstancy of temperature in a heat bath have been neglected.

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