Ruppeiner Geometry, Reentrant Phase transition and Microstructure of Born-Infeld AdS Black Hole

TL;DR

This paper investigates the microstructure and phase transitions of Born-Infeld AdS black holes using Ruppeiner geometry, revealing distinct microstructural behaviors for standard and reentrant phase transitions and their relation to quantum gases.

Contribution

It introduces a novel Ruppeiner geometry approach to analyze the microstructure of Born-Infeld AdS black holes, uncovering differences between standard and reentrant phase transitions.

Findings

Standard phase transition involves RN-AdS microstructure with repulsive interactions.

Reentrant phase transition features dominant attractive interactions, with black holes behaving like a bosonic gas.

Curvature scalar signals the critical phenomena and phase transition signatures.

Abstract

Born-Infeld AdS black hole exhibits a reentrant phase transition for certain values of the Born-Infeld parameter $b$. This behaviour is an additional feature compared to the van der Waals like phase transition observed in charged AdS black holes. Therefore, it is worth observing the underlying microscopic origin of this reentrant phase transition. Depending on the value of the parameter $b$, the black hole system has four different cases: no phase transition, a reentrant phase transition with two scenarios, or a van der Waals-like (standard) phase transition. In this article, by employing a novel Ruppeiner geometry method in the parameter space of temperature and volume, we investigate the microstructure of Born-Infeld AdS black hole via the phase transition study, which includes standard and reentrant phase transition. We find that the microstructures of the black hole that lead to standard and reentrant phase transitions are distinct in nature. The standard phase transition is characterised by the typical RN-AdS microstructure. In this case, the small black hole phase has a dominant repulsive interaction for the low temperature case. Interestingly, during the reentrant phase transition, displayed by the system in a range of pressures for specific $b$ values, the dominant attractive nature of interaction in the microstructure is preserved. Our results suggest that in the reentrant phase transition case, the intermediate black holes behave like a bosonic gas, and in the standard phase transition case the small black holes behave like a quantum anyon gas. In both cases, the large black hole phase displays an interaction similar to the bosonic gas. The critical phenomenon is observed from the curvature scalar, including the signature of the reentrant phase transition.