Thermal properties of Simpson–Visser Minkowski core regular black holes solution in Verlinde’s emergent gravity

In this study, we investigate the thermodynamic characteristics of the Simpson–Visser Minkowski core black hole solution within Verlinde’s emergent gravity framework. Our analysis encompasses the examination of energy emission, Gibbs free energy, and thermal fluctuations. We calculate various quantities such as the Hawking temperature, geometric mass, and heat capacity to assess the local and global thermodynamic stability. The temperature of the black hole is determined using the first law of thermodynamics, while the energy emission rate is evaluated as well. By computing the Gibbs free energy, we explore the phase transition behavior exhibited by Verlinde’s emergent gravity black holes, specifically examining the swallowing tails. Moreover, we derive the corrected entropy to investigate the influence of thermal fluctuations on small and large black holes. Notably, we compare the impact of correction terms on the thermodynamic system by comparing the results obtained for large black holes and small black holes.