Non-extended phase space thermodynamics of Lovelock AdS black holes in grand canonical ensemble

TL;DR

This paper investigates the phase transitions of Lovelock AdS black holes in the grand canonical ensemble using thermodynamic geometry, revealing second order phase transitions and the effectiveness of Ruppeiner metric in probing black hole thermodynamics.

Contribution

It provides a detailed analysis of non-extended phase space thermodynamics of Lovelock AdS black holes, including phase transition conditions and geometric methods, which is a novel perspective compared to prior extended phase space studies.

Findings

Two critical points for n=6, k=1 case.

No phase transition point for k=0.

Ruppeiner scalar curvature divergence matches specific heat divergence.

Abstract

Recently, extended phase space thermodynamics of Lovelock AdS black holes has been of great interest. To provide insight from a different perspective and gain a unified phase transition picture, non-extended phase space thermodynamics of $(n+1)$-dimensional charged topological Lovelock AdS black holes is investigated detailedly in the grand canonical ensemble. Specifically, the specific heat at constant electric potential is calculated and phase transition in the grand canonical ensemble is discussed. To probe the impact of the various parameters, we utilize the control variate method and solve the phase transition condition equation numerically for the case $k=1,-1$. There are two critical points for the case $n=6,k=1$ while there is only one for other cases. For $k=0$, there exists no phase transition point. To figure out the nature of phase transition in the grand canonical ensemble, we carry out an analytic check of the analog form of Ehrenfest equations proposed by Banerjee et al. It is shown that Lovelock AdS black holes in the grand canonical ensemble undergo a second order phase transition. To examine the phase structure in the grand canonical ensemble, we utilize the thermodynamic geometry method and calculate both the Weinhold metric and Ruppeiner metric. It is shown that for both analytic and graphical results that the divergence structure of the Ruppeiner scalar curvature coincides with that of the specific heat. Our research provides one more example that Ruppeiner metric serves as a wonderful tool to probe the phase structures of black holes.