Contact-Time Model of Black Hole Cores
Year: 2026
Type: preprint
Abstract: If time and space are produced by contact between matter, and every black hole is filled to its contact capacity, black holes have finite cores. Defining contact as normalized quantum mutual information, with its vacuum fall-off of 1/distance⁴, motivates a candidate regular black hole metric. Under the hypothesis that each black hole sits at its degenerate-horizon (“full”) limit, core size is fixed by spin, and black hole shadows are predicted to be 7–9% smaller than in general relativity. Calculations were assisted by an AI and have not been peer reviewed.
Author: Enemuwe, Robin
Language: English
Subfield: Nuclear and High Energy Physics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: green
OpenAlex ID: W7221593409
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