Ruppeiner thermodynamic geometry for the Schwarzschild-AdS black hole
Zhen-Ming Xu, Bin Wu, and Wen-Li Yang

TL;DR
This paper addresses the singularity issues in Ruppeiner thermodynamic geometry for Schwarzschild-AdS black holes by proposing a scheme that uses enthalpy as the fundamental characteristic, revealing insights into black hole interactions.
Contribution
It introduces a natural approach using enthalpy for thermodynamic geometry of spherically symmetric AdS black holes, resolving singularity problems and comparing different phase space geometries.
Findings
Thermodynamic curvature is negative, indicating attractive interactions.
Curvature in different phase spaces is equivalent.
Black hole interactions vary from repulsive at low temperatures to attractive at high temperatures.
Abstract
Due to the non-independence of entropy and thermodynamic volume for spherically symmetric black holes in the AdS spacetime, when applying the Ruppeiner thermodynamic geometry theory to these black holes, we often encounter an unavoidable problem of the singularity about the line element of thermodynamic geometry. In this paper, we propose a basic and natural scheme for dealing with the thermodynamic geometry of spherically symmetric AdS black holes. We point out that enthalpy, not internal energy, is the fundamental thermodynamic characteristic function for the Ruppeiner thermodynamic geometry. Based on this fact, we give the specific forms of the line element of thermodynamic geometry for Schwarzschild AdS (SAdS) black hole in different phase spaces and the results show that the thermodynamic curvatures obtained in different phase spaces are equivalent. It is shown that the…
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