Criticality In the Extended Phase Space of Charged Accelerating AdS Black Holes
arXiv:1607.00496 · doi:10.1142/S0217732316501996
Abstract
In this paper, we investigate the criticality and phase transition of charged accelerating AdS black holes in the extended thermodynamic phase space in analogy between black hole system and Van der Waals liquid-gas system, where the cosmological constant is treated as a thermodynamical variable interpreted as dynamic pressure and its conjugate quantity is the thermodynamic volume of the black holes. When the electric charge vanishes, we find that no criticality will appear but the Hawking-Page like phase transition will be present, just as what Schwarzschild-AdS black holes behave like. For the charged case, the criticality appears and the accelerating black holes will undergo a small black hole/large phase transition under the condition that the acceleration parameter and the horizon radius meet a certain simple relation , where is a constant in our discussion. To make criticality appear, there exists an upper bounds for constant . When criticality appears, we calculate the critical pressure , critical temperature and critical specific volume , and we find that is an universal number.
14pages,5 figures,references added
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Cited by in corpus (4)
- Thermodynamic stability and P-V criticality of nonsingular-AdS black holes endowed with clouds of strings
- Charged Accelerating BTZ black holes
- The extended phase space thermodynamics of Planck-scale-corrected Reissner-Nordström-anti-de Sitter black hole
- The generalization of charged AdS black hole specific volume and number density