Viscous Emergent Spacetime and the Origin of Black Hole Entropy

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Authors: Mikheil Rusishvili
Cited by: 0

Abstract

The Bekenstein-Hawking entropy formula S = A/4G remains one of the most profound hints of a deeper microscopic theory of gravity. In this paper, we derive this formula from first principles within the Viscous Emergent Spacetime (VES) framework. VES is built on four axioms: covariance, conservation of information, irreversible coarse-graining, and minimalism. From these, spacetime geometry emerges as the macroscopic imprint of information flow with bulk viscosity. We show that black hole horizons correspond to informational barriers where the viscous information current vanishes. The resulting “viscous core” replaces the classical singularity and stores information holographically on its surface. The Bekenstein-Hawking entropy emerges naturally from the critical information density I∗ and the bulk viscosity coefficient γ0, with small corrections for stellar-mass black holes that may be testable by future gravitational wave observations.

Fields of Study & Subjects

Black Holes and Theoretical Physics Noncommutative and Quantum Gravity Theories Relativity and Gravitational Theory

Publication details

Journal / source
Zenodo (CERN European Organization for Nuclear Research)
Publication date
7 March 2026
Language
EN
Document type
Preprint