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March 1, 20260 citationsOpen Access

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

DGDirk Goussey

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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Cite This Study

Dirk Goussey (2026) studied this question.

synapsesocial.com/papers/69a3d887ec16d51705d2f762https://doi.org/10.5281/zenodo.18800341
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