What question did this study set out to answer?

The aim is to present a model replacing singularities in black holes with maximum compression states and exploring entropy.

March 1, 2026Open Access

A Mechanistic Model of Black Hole Dynamics: Interstitial n=0 Flux Entrapment and the S=A/4 Topology

Key Points

The aim is to present a model replacing singularities in black holes with maximum compression states and exploring entropy.
Developed a non-singular model for black holes through Push-theory.
Replaced mathematical singularities with n=3 8-Möbius Voxel compression.
Derived mechanical expressions for Hawking radiation and entropy law based on surface curvature.
Demonstrated black holes act as topological storage units for zero point energy.
Challenged the No-Hair Theorem by proposing the concept of Topological Hair in black holes.
Established that information is archived within interstitial flux rather than lost.

Abstract

This paper introduces a non-singular model for Black Holes within the framework of Push-theory (DOI: 10.5281/zenodo.18799096 & DOI: 10.5281/zenodo.18740415). By replacing mathematical singularities with a state of maximum 8-Möbius Voxel (n=3) compression, we demonstrate that Black Holes function as topological storage units for the universal Zero Point Energy (ZPE) flux (n=0). We provide a mechanical derivation for Hawking radiation and the S=A/4 entropy law based on surface curvature and interstitial flux release. This model challenges the classical No-Hair Theorem by demonstrating that black holes possess Topological Hair in the form of n=3 voxel configurations. The information is not lost but archived within the interstitial n=0 flux.

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