Thermodynamical properties of stationary, axially symmetric non-Kerr black holes.

Details Thermodynamical properties of stationary, axially symmetric non-Kerr black holes. Thermodynamical properties of stationary, axially symmetric non-Kerr black holes.

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993sccha..36.1103z&link_type=abstract

Science in China, Series A, Vol. 36, No. 9, p. 1103 - 1113

Physics

Black Holes: Thermodynamics

Scientific paper

The thermodynamical properties of some stationary, axially symmetric non-Kerr black holes possessing mass with multipole moments are discussed. The rotating angular velocities of this sort of black holes are zero. There exist thermal radiations, and the temperatures on the event horizons are constant. The existence of naked singularities strongly influences the Hawking temperature at the two poles of the black holes, and enables it to vanish or diverge. It shows that the thermodynamical laws forbid this sort of naked singularities to appear, and go so far as to forbid this sort of black holes to form or emerge.

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