Thermodynamic phase transition and Joule-Thomson expansion of a quantum corrected black hole in AdS spacetime

Abstract

The thermodynamics in the extended phase space of a quantum corrected black hole (BH) proposed recently is presented in this work. Our study shows that the phase transition behavior of the BH is analogous to that of conventional Schwarzschild BH in anti-de Sitter (AdS) space; however, a critical temperature exists such that when the BH temperature exceeds this critical value, the small BH phase and the large BH phase become separated, and no phase transition occurs. Due to the introduction of the quantum parameter $ξ$, the BH equation of state splits into two branches. One branch reduces to the Schwarzschild-AdS case as $ξ\to0$, with its phase transition pressure lower than the critical pressure; another branch's phase transition pressure is greater than the critical pressure. The study shows that the $T-r_{+}$ phase transition and heat capacity are similar to those of the Schwarzschild-AdS BH. The Joule-Thomson expansion is divided into two stages: in the earlier stage, the BH pressure increases until it reaches a maximum; in the later stage, the pressure gradually decreases. In each stage, the BH may undergo an inversion point, resulting in the inversion curve with two branches. In addition, each stage has a minimum inversion mass, below which any BH (in each respective stage) has no inversion point.