The Boundary Conditions of Vacuum Stiffness and the Limits of Geometry

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1. Verfasser: Labhard, Michael
Format: Recurso digital
Sprache:Englisch
Veröffentlicht: Zenodo 2026
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author Labhard, Michael
author_facet Labhard, Michael
contents <p><em>This paper is archived as a speculative research work</em>.</p> <p>Black holes occupy a unique and persistent position in fundamental physics, simultaneously con-<br>firming General Relativity while exposing its conceptual limits. Traditional treatments regard black<br>holes as objects with interiors governed by unknown physics, leading to singularities, information<br>paradoxes, and unresolved questions about quantum gravity. In this work, we show that these prob-<br>lems arise from a misplaced assumption: that gravity is a dynamical interaction operating within<br>a spacetime interior. Building on the identification of the Higgs field as a scalar vacuum-stiffness<br>assignment and General Relativity as its geometric bookkeeping, we reinterpret black holes as satu-<br>ration boundaries of vacuum stiffness. The event horizon marks the limit at which admissible causal<br>and geometric representation fails, not the presence of hidden interior structure. The black-hole in-<br>terior is therefore undefined rather than singular, and all physically meaningful information is fully<br>encoded in the exterior stiffness assignment. This reinterpretation resolves long-standing puzzles<br>concerning singularities, unitarity, holography, Hawking radiation, and rotation without modifying<br>General Relativity or introducing new degrees of freedom. Black holes emerge as probes of the<br>causal limits imposed by the underlying kernel of admissibility, not as sites of exotic new physics.</p>
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language eng
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spellingShingle The Boundary Conditions of Vacuum Stiffness and the Limits of Geometry
Labhard, Michael
Entanglement-Algebraic Spacetime (EAS)
causality boundaries
event horizons
holographic principle reinterpretation
black hole information paradox dissolution
<p><em>This paper is archived as a speculative research work</em>.</p> <p>Black holes occupy a unique and persistent position in fundamental physics, simultaneously con-<br>firming General Relativity while exposing its conceptual limits. Traditional treatments regard black<br>holes as objects with interiors governed by unknown physics, leading to singularities, information<br>paradoxes, and unresolved questions about quantum gravity. In this work, we show that these prob-<br>lems arise from a misplaced assumption: that gravity is a dynamical interaction operating within<br>a spacetime interior. Building on the identification of the Higgs field as a scalar vacuum-stiffness<br>assignment and General Relativity as its geometric bookkeeping, we reinterpret black holes as satu-<br>ration boundaries of vacuum stiffness. The event horizon marks the limit at which admissible causal<br>and geometric representation fails, not the presence of hidden interior structure. The black-hole in-<br>terior is therefore undefined rather than singular, and all physically meaningful information is fully<br>encoded in the exterior stiffness assignment. This reinterpretation resolves long-standing puzzles<br>concerning singularities, unitarity, holography, Hawking radiation, and rotation without modifying<br>General Relativity or introducing new degrees of freedom. Black holes emerge as probes of the<br>causal limits imposed by the underlying kernel of admissibility, not as sites of exotic new physics.</p>
title The Boundary Conditions of Vacuum Stiffness and the Limits of Geometry
topic Entanglement-Algebraic Spacetime (EAS)
causality boundaries
event horizons
holographic principle reinterpretation
black hole information paradox dissolution
url https://doi.org/10.5281/zenodo.18134763