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P-V criticality in AdS black holes of massive gravity

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arxiv 1611.05329 v3 pith:SLXOSGDL submitted 2016-11-16 gr-qc

classification gr-qc
keywords blackholescriticalgravitymassivephasecomputedexponents
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In this paper we have studied the extended phase space thermodynamics in the canonical ensemble of black holes in massive gravity in AdS space. The black holes considered here belong to a theory of massive gravity where the graviton gain a mass due to Lorentz symmetry breaking. We have computed various thermodynamical quantities such as temperature, pressure, Gibbs free energy and specific heat capacity. The local and the global thermodynamical stability of the black holes are studied in detail. For a specific value of the parameter in the theory, the black holes undergo a first order phase transition similar to the Van der Waals phase transitions between gas and liquid under constant temperature. This transition is between the small and the large black hole. The critical exponents are computed at the critical values and shown to be the same as for the Van der Waals critical exponents.

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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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