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Extended phase space thermodynamics and $P-V$ criticality of charged black holes in Brans-Dicke theory

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arxiv 1503.07070 v1 pith:3EFEAKWC submitted 2015-03-23 gr-qc hep-th

S. H. Hendi , Z. Armanfard This is my paper · ORCID
classification gr-qchep-th
keywords blackphasechargedextendedholespacetheorythermodynamic
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abstract

In this paper, taking in to account Brans-Dick theory, we investigate thermodynamic behavior of charged black hole solutions. We study the analogy of the black hole solution with the Van der Waals liquid-gas system in the extended phase space by considering the cosmological constant as dynamical pressure. We obtain critical values of thermodynamic coordinates and plot $P-r_{+}$ and $G-T$ diagrams to study the phase transition.

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  1. Effects of quantum corrections on the criticality and efficiency of black holes surrounded by a perfect fluid

    gr-qc 2019-08 conditional novelty 5.0 of 10

    For a quantum-corrected Schwarzschild black hole in a Kiselev perfect fluid, first-order PV criticality appears when the fluid parameter satisfies omega > -1/3 and omega differs from zero, while a Hawking-Page-like tr...

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