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- W2014487466 abstract "After introducing the connection between the black hole horizon and the cosmological horizon, we discuss the thermodynamic properties of Reissner–Nordström–de Sitter (RN–dS) space–time. We present the condition under which RN–dS black hole can exist. Employing Ehrenfest' classification, we conclude that the phase transition of RN–dS black hole is the second-order one. The position of the phase transition point is irrelevant to the electric charge of the system. It only depends on the ratio of the black hole horizon and the cosmological horizon." @default.
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- W2014487466 date "2014-04-08" @default.
- W2014487466 modified "2023-10-16" @default.
- W2014487466 title "Existence condition and phase transition of Reissner–Nordström–de Sitter black hole" @default.
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- W2014487466 doi "https://doi.org/10.1142/s0217751x1450050x" @default.
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