P-V criticality in the extended phase space of black holes in Einstein-Horndeski gravity
arXiv:1812.09938 · doi:10.1103/PhysRevD.100.084004
Abstract
Gravity is believed to have deep and inherent relation to thermodynamics. We study phase transition and critical behavior in the extended phase space of asymptotic anti de-Sitter (AdS) black holes in Einstein-Horndeski gravity. We demonstrate that the black hole in Einstein-Horndeski gravity undergo phase transition and P-V criticality mimicking the van der Waals gas-liquid system. The key approach in our study is to introduce a more reasonable pressure instead of previous pressure related to cosmological constant , and this proper pressure is given insight from the asymptotical behaviour of this black hole. Moreover, we also first obtain P-V criticality in the two cases with and in our paper, which implicates that the cosmological constant may be not a necessary pressure candidate for black holes at the microscopic level. We present critical exponents for these phase transition processes.
arXiv comment14 pages, 5 figures, two appendixes and more contents added, version accepted by PRD
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