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Thermodynamics of charged anti-de Sitter black holes in canonical ensemble

P. Mitra
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Abstract

As in the grand canonical treatment of Reissner - Nordström black holes in anti-de Sitter spacetime, the canonical ensemble formulation also shows that non-extremal black holes tend to have lower action than extremal ones. However, some small non-extremal black holes have higher action, leading to the possibility of transitions between non-extremal and extremal black holes.

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P. Mitra. 1999-12-16. Thermodynamics of charged anti-de Sitter black holes in canonical ensemble. https://doi.org/10.1016/s0370-2693(99)00689-9

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