Black Holes as Collapse-Dominated Structures: Curvature, Runaway Feedback, and the Breakdown of Continuation

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Main Author: Doy, David Michael
Format: Recurso digital
Language:English
Published: Zenodo 2026
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_version_ 1866901343377031168
author Doy, David Michael
author_facet Doy, David Michael
contents <p>*Black Holes as Collapse‑Dominated Structures* develops a structural interpretation of black holes in which gravitational collapse is understood as a runaway feedback process that overwhelms stabilised continuation. Instead of treating black holes as merely dense astrophysical objects or as singular solutions of general relativity, the report reframes them as regions where collapse becomes dominant, effective density diverges, and geometric description fails. The event horizon is interpreted as a phase boundary between stabilised and collapse‑dominated regimes, the interior as a pre‑geometric domain where continuation cannot be maintained, and the singularity as the structural failure point of definability.</p> <p>The report identifies the positive feedback loop—collapse → effective density → curvature → destabilisation → collapse—that drives black‑hole formation and explains why black holes represent a qualitatively distinct phase of spacetime organisation. Hawking radiation is recast as a boundary‑level stabilisation effect arising from the tension between stabilised modes outside the horizon and collapse‑dominated dynamics inside. The framework preserves the empirical content of general relativity while offering a generative explanation for curvature, horizon structure, interior behaviour, and the cosmological role of black holes as conditioners of the underlying substrate.</p> <p>This document provides a self‑contained account of black holes within the broader generative architecture, unifying collapse, curvature, and geometric failure under a single structural mechanism.</p>
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institution Zenodo
language eng
publishDate 2026
publisher Zenodo
record_format zenodo
spellingShingle Black Holes as Collapse-Dominated Structures: Curvature, Runaway Feedback, and the Breakdown of Continuation
Doy, David Michael
Blackholes
black holes
collapse
gravity
density
curvature
light
continuation
structture
substrate
singularity
potential
geometry
horizon
<p>*Black Holes as Collapse‑Dominated Structures* develops a structural interpretation of black holes in which gravitational collapse is understood as a runaway feedback process that overwhelms stabilised continuation. Instead of treating black holes as merely dense astrophysical objects or as singular solutions of general relativity, the report reframes them as regions where collapse becomes dominant, effective density diverges, and geometric description fails. The event horizon is interpreted as a phase boundary between stabilised and collapse‑dominated regimes, the interior as a pre‑geometric domain where continuation cannot be maintained, and the singularity as the structural failure point of definability.</p> <p>The report identifies the positive feedback loop—collapse → effective density → curvature → destabilisation → collapse—that drives black‑hole formation and explains why black holes represent a qualitatively distinct phase of spacetime organisation. Hawking radiation is recast as a boundary‑level stabilisation effect arising from the tension between stabilised modes outside the horizon and collapse‑dominated dynamics inside. The framework preserves the empirical content of general relativity while offering a generative explanation for curvature, horizon structure, interior behaviour, and the cosmological role of black holes as conditioners of the underlying substrate.</p> <p>This document provides a self‑contained account of black holes within the broader generative architecture, unifying collapse, curvature, and geometric failure under a single structural mechanism.</p>
title Black Holes as Collapse-Dominated Structures: Curvature, Runaway Feedback, and the Breakdown of Continuation
topic Blackholes
black holes
collapse
gravity
density
curvature
light
continuation
structture
substrate
singularity
potential
geometry
horizon
url https://doi.org/10.5281/zenodo.19035873