Quantum corrected thermodynamics and $P-V$ criticality of self-gravitating Skyrmion black holes

TL;DR

This paper investigates quantum corrections to the thermodynamics of self-gravitating Skyrmion black holes, revealing phase transitions and critical behavior influenced by model parameters, with implications for experimental bounds.

Contribution

It introduces quantum-corrected thermodynamics for Einstein-Skyrmion black holes and analyzes their $P-V$ criticality, highlighting parameter dependence and phase transition phenomena.

Findings

Quantum corrections induce stability and phase transitions.

The $P-V$ criticality depends on parameters $$ and $K$.

Potential to estimate bounds on model parameters from thermodynamic behavior.

Abstract

In this paper, we study the quantum corrected thermodynamics of a class of black holes generated by self-gravitating Skyrmion models. One such black hole solution is Einstein-Skrymion black hole. We first compute the ADM mass of Einstein-Skyrmion black hole using on-shell Hamiltonian formalism present already in the literature. We then consider non-extended phase space thermodynamics and derive expressions for various thermodynamic quantities like the Hawking temperature, entropy, pressure, Gibbs free energy, and heat capacity. Next, we study the effect of quantum corrections on the thermodynamics of the Einstein-Skyrmion black hole. We observe that apart from leading to stability, the quantum correction induce an AdS (anti-de sitter) to dS (de Sitter) phase transition in Einstein-Skrymion black hole. Treating cosmological constant as the pressure, we determine the $P-V$ criticality of the Einstein-Skrymion black hole and observe that the $P-V$ criticality depends on model parameters $\lambda$ and $K$. The study of $P-V$ criticality done here could help to estimate the experimental bound on the values of parameters $\lambda$ and $K$.