Extreme State of a Charged Black Hole in a Grand Canonical Ensemble

Details Extreme State of a Charged Black Hole in a Grand Canonical Ensemble Extreme State of a Charged Black Hole in a Grand Canonical Ensemble

Mar 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996phrvl..76.2211z&link_type=abstract

Physical Review Letters, Volume 76, Issue 13, March 25, 1996, pp.2211-2213

Physics

42

Scientific paper

It is shown that a charged black hole in a cavity can approach the extreme state at finite temperature. In so doing, its surface area tends to that of a cavity but the proper distance L between a horizon and the boundary tends to a finite value. The arguments in the favor of zero entropy based on infinite L become inapplicable and the entropy equals the Bekenstein-Hawking one.

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