Geometrical thermodynamics and P-V criticality of the black holes with power-law Maxwell field

Abstract

We study thermodynamical structure of Einstein black holes in the presence of power Maxwell invariant nonlinear electrodynamics for two different cases. The behavior of the temperature and conditions regarding the stability of these black holes are investigated. Since the language of geometry is an effective method in general relativity, we concentrate on the geometrical thermodynamics to build a phase space for studying phase transition. In addition, taking into account the denominator of the heat capacity, we use the proportionality between cosmological constant and thermodynamical pressure to extract the critical values for these black holes. Besides, the effects of the variation of different parameters on thermodynamical structure of these black holes are investigated. In addition, some thermodynamical properties such as volume expansion coefficient, speed of sound and isothermal compressibility coefficient are calculated and some remarks regarding these quantities are given.

18 pages with 12 captioned figures. Published version

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• Geometrothermodynamics
• Higher-dimensional black holes with a conformally invariant Maxwell source
• P-V criticality in the extended phase space of black holes in massive gravity
• Higher-dimensional charged black holes solutions with a nonlinear electrodynamics source
• van der Waals like behaviour of topological AdS black holes in massive gravity
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• Thermodynamic Stability of the Stationary Lifshitz Black Hole of New Massive Gravity
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• Structure and thermodynamics of charged nonrotating black holes in higher dimensions
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