Statistical mechanical origin of the entropy of a rotating, charged black hole

Details Statistical mechanical origin of the entropy of a rotating, charged black hole Statistical mechanical origin of the entropy of a rotating, charged black hole

May 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985phrvl..54.2171z&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 54, May 20, 1985, p. 2171-2175.

Physics

Condensed Matter

Statistical Mechanics

135

Black Holes (Astronomy), Entropy, Rotating Bodies, Statistical Mechanics, Asymptotic Properties, Quantum Mechanics, Schwarzschild Metric, Space-Time Functions

Scientific paper

The entropy of a rotating charged black hole is argued to be the logarithm of the number of quantum mechanically distinct ways in which the hole could have been produced, and the logarithm of the number of configurations that the hole's atmosphere could assume in the presence of its background noise of acceleration radiation. A space-time horizon evolution diagram is included, in which the horizon initially grows due to accretion, then shrinks due to evaporation, and then grows again. As a side product, a proof of the generalized second law of thermodynamics is obtained.

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