The third law of thermodynamics for Kerr black holes

Details The third law of thermodynamics for Kerr black holes The third law of thermodynamics for Kerr black holes

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991mnras.250..300o&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 250, May 15, 1991, p. 300-309.

Statistics

Computation

7

Black Holes (Astronomy), Computational Astrophysics, Stellar Evolution, Stellar Mass Accretion, Thermodynamics, Angular Momentum, Stellar Models

Scientific paper

After using the black hole mass-angular momentum plane to clarify the thermodynamic and evolutionary characteristics of Kerr black holes, the conditions under which the third law of black-hole thermodynamics for such black holes is not violated are derived, taking into account possible accretion processes. It is noted that, in light of these considerations, no Kerr holes are capable of achieving the extreme Kerr state with the absolute zero temperature by accreting finite quantities of both mass and angular momentum.

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