Black hole thermodynamical entropy
Constantino Tsallis, Leonardo J. L. Cirto

TL;DR
This paper explores the limitations of Boltzmann-Gibbs entropy in describing black hole thermodynamics and proposes a generalized nonadditive entropy to resolve the area law and nonextensivity issues.
Contribution
It introduces a generalized entropy framework that addresses the thermodynamic inconsistencies of black holes and strongly entangled quantum systems.
Findings
The BG entropy is inadequate for black hole and quantum entangled systems.
A generalized nonadditive entropy can restore thermodynamic consistency.
The approach explains the area law and nonextensivity in these systems.
Abstract
As early as 1902, Gibbs pointed out that systems whose partition function diverges, e.g. gravitation, lie outside the validity of the Boltzmann-Gibbs (BG) theory. Consistently, since the pioneering Bekenstein-Hawking results, physically meaningful evidence (e.g., the holographic principle) has accumulated that the BG entropy of a black hole is proportional to its area ( being a characteristic linear length), and not to its volume . Similarly it exists the \emph{area law}, so named because, for a wide class of strongly quantum-entangled -dimensional systems, is proportional to if , and to if , instead of being proportional to (). These results violate the extensivity of the thermodynamical entropy of a -dimensional system. This thermodynamical inconsistency disappears if we realize that the…
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