Thermodynamical stability of -AdS black holes in grand canonical ensemble
arXiv:1812.04220 · doi:10.1007/s10714-018-2491-0
Abstract
In this paper, -dimensional ( is a positive integer) -AdS black holes is divided into Schwazschild-AdS (SAdS) like ones and Reissner-Nordström-AdS (RN-AdS) like ones. Thermodynamical stability of them in grand canonical ensemble is investigated. Locally, we find that the RN-AdS like black holes will experience either type-one or type-two phase transitions from unstable states to stable states, whereas there are only type-two phase transitions between that two states for SAdS like black holes. Globally, we find that there are type-one Hawking-Page like phase transitions between thermal AdS state and black holes. Using thermodynamical geometry method, we find that thermodynamical extrinsic curvature can only provide accurate stability information near type-two (not type-one) phase transition points for black holes in grand canonical ensemble.
arXiv comment9 pages
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