From modified Tsallis-Renyi entropy to a MOND-like force law, Bekenstein bound, and Landauer principle for black holes

TL;DR

This paper explores how modified Renyi entropy, derived from Tsallis entropy, leads to a MOND-like force law, supports the Bekenstein bound, and relates to black hole mass loss via the Landauer principle, offering new insights into black hole thermodynamics and gravity.

Contribution

It introduces a framework connecting modified Renyi entropy with MOND, Bekenstein bound, and black hole evaporation, providing a novel unified approach to black hole thermodynamics.

Findings

A MOND-like force law emerges from entropic considerations.

The Bekenstein bound holds under the modified Renyi entropy framework.

An expression for black hole mass loss is derived using the Landauer principle.

Abstract

We examine black hole thermodynamics within the framework of modified Renyi entropy and explore its implications in Modified Newtonian Dynamics (MOND), an extension of Newton second law proposed to explain galaxy rotation curves without invoking dark matter. We conjecture that Tsallis entropy provides an exact description of Bekenstein Hawking entropy, from which the modified Renyi entropy is derived. Using this formulation, we show that a MOND like force law emerges naturally from entropic considerations. We also analyze the Bekenstein bound conjecture, which imposes an upper limit on the entropy of confined quantum systems, and verify its validity under the Renyi modified framework for typical values of the deformation parameter. Furthermore, by invoking the Landauer principle, we obtain an expression for the mass loss due to black hole evaporation. These results suggest that modified Renyi statistics, originating from Tsallis entropy, provides a coherent and promising approach to gravitational dynamics and information theoretic aspects of black hole physics.