Abstract

In this work, we investigate the thermodynamics of four-dimensional charged anti-de Sitter (AdS) black hole surrounded by perfect fluids in the context of Rastall theory. We derive the equations of state by considering the charge square [Formula: see text] and the metric parameter [Formula: see text] as the thermodynamic variables. The [Formula: see text] and [Formula: see text] figures for some special surrounding fields were analyzed in detail. To better explain the phase transition, the behavior of the Gibbs free energy is presented. Note that the critical exponents are in perfect agreement with the van der Waals (vdWs) fluid system. In addition, we discuss Joule–Thomson (J-T) expansion in extended phase space. We determine the region where cooling or heating by investigating J-T coefficient. The inversion curves and the isenthalpic curves are plotted in the [Formula: see text] plane. Also, we calculate the minimum inversion temperature [Formula: see text] and find that the ratio [Formula: see text] is independent of the radiation field parameter [Formula: see text].

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