Black Holes in the W-Structure

In the W-Structure, a black hole is the saturation limit 3W: all possible links are realized and nothing changes inside; there is no singularity. Outside, space densifies layer by layer: clock rate e^(−δ), steps per unit path e^(+δ). With δ = GM/(rc²) this is the exponential metric (as in Papapetrou and Yilmaz), which differs from general relativity: throat at e·GM/c² ≈ 2.72 GM/c², shadow radius 2e·GM/c² ≈ 5.44 GM/c², 4.6% larger than in GR (non-rotating layers). New here: the derivation of the field form from layers and links, and what lies beyond the throat; the numbers for this metric are known. Predictions: larger shadow; finite redshift of light near the throat; no black holes lighter than the neutron-star limit (minus mass lost in collapse); no echoes and no Hawking radiation from 3W. Underived points are listed as open questions. English text with the Russian original included.

Authors

Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-11-06
DOI
https://doi.org/10.5281/zenodo.24016340
Primary Topic
Black Holes and Theoretical Physics
Type
preprint
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preprint

Black Holes in the W-Structure

Hrachya Danielyan
3 links
Zenodo (CERN European Organization for Nuclear Research)
Black Holes and Theoretical Physics
preprint

Black Holes in the W-Structure

Hrachya Danielyan
preprint en

Abstract

In the W-Structure, a black hole is the saturation limit 3W: all possible links are realized and nothing changes inside; there is no singularity. Outside, space densifies layer by layer: clock rate e^(−δ), steps per unit path e^(+δ). With δ = GM/(rc²) this is the exponential metric (as in Papapetrou and Yilmaz), which differs from general relativity: throat at e·GM/c² ≈ 2.72 GM/c², shadow radius 2e·GM/c² ≈ 5.44 GM/c², 4.6% larger than in GR (non-rotating layers). New here: the derivation of the field form from layers and links, and what lies beyond the throat; the numbers for this metric are known. Predictions: larger shadow; finite redshift of light near the throat; no black holes lighter than the neutron-star limit (minus mass lost in collapse); no echoes and no Hawking radiation from 3W. Underived points are listed as open questions. English text with the Russian original included.

Zenodo (CERN European Organization for Nuclear Research)
Black Holes and Theoretical Physics
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