Barrow black hole corrected-entropy model and Tsallis nonextensivity
Everton M. C. Abreu, Jorge Ananias Neto

TL;DR
This paper explores the effects of quantum fluctuations on Barrow black hole entropy using Tsallis nonextensive thermodynamics, analyzing stability and thermodynamic properties with a new generalized equipartition law.
Contribution
It introduces a master equation for the equipartition law incorporating Tsallis' nonextensivity into quantum-corrected Barrow entropy, analyzing stability across various parameters.
Findings
Derived a generalized equipartition law for Barrow black holes with Tsallis q-parameter.
Analyzed thermal stability as a function of quantum fluctuation and nonextensivity parameters.
Identified conditions for stability and phase transitions in the black hole thermodynamics.
Abstract
The quantum scenario concerning Hawking radiation, gives us a precious clue that a black hole has its temperature directly connected to its area gravity and that its entropy is proportional to the horizon area. These results have shown that there exist a deep association between thermodynamics and gravity. The recently introduced Barrow formulation of back holes entropy, influenced by the spacetime geometry, shows the quantum fluctuations effects through Barrow exponent, , where represents the usual spacetime and its maximum value, , characterizes a fractal spacetime. The quantum fluctuations are responsible for such fractality. Loop quantum gravity approach provided the logarithmic corrections to the entropy. This correction arises from quantum and thermal equilibrium fluctuations. In this paper we have analyzed the nonextensive thermodynamical effects of…
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