Thermodynamics of AdS-Schwarzschild-like black hole in loop quantum gravity

TL;DR

This paper explores the thermodynamics of loop quantum gravity-corrected Schwarzschild-AdS black holes, revealing critical behavior, phase transitions, and the impact of quantum effects on classical thermodynamic laws.

Contribution

It introduces a quantum-corrected black hole metric in AdS space and analyzes its thermodynamics, highlighting deviations from classical black hole behavior due to LQG effects.

Findings

Existence of a critical point with a unique ratio of 7/18

Quantum corrections lead to a modified first law of thermodynamics

Presence of inversion points in Joule-Thomson expansion

Abstract

We obtained the metric of the Schwarzschild-like black hole with loop quantum gravity (LQG) corrections in anti-de Sitter (AdS) space-time, under the assumption that the cosmological constant is decoupled in LQG. We investigated its thermodynamics, including the equation of state, criticality, heat capacity, and Gibbs free energy. The $P-v$ graph was plotted, and the critical behavior was calculated. It was found that, due to the LQG effect, the quantum-corrected Schwarzschild-AdS black hole exhibits a critical point and a critical ratio of $7/18$, which differs from the Reissner-Nordstr$\ddot{\mathrm{o}}$m-AdS black hole's ratio of $3/8$ (the same as that of the Van der Waals system) slightly. However, there are still some similarities compared to the Van der Waals system, such as the same critical exponents and a similar $P-v$ graph. Moreover, it is concluded that the energy-momentum tensor related to the black hole's mass could violate the conventional first law of thermodynamics. This modified first law may violate the conservation of Gibbs free energy during the small black hole-large black hole phase transitions, potentially indicating the occurrence of the zeroth-order phase transition. The Joule-Thomson expansion was also studied. Interestingly, compared to the Schwarzschild-AdS black hole, the LQG effect leads to inversion points. The inversion curve divides the $\left(P,T\right)$ coordinate system into two regions: a heating region and a cooling region, as shown in detail by the inversion curves and isenthalpic curves. The results indicated that there is a minimum inversion mass, below which any black hole will not possess an inversion point.