Substrate Tension as a Driver for Galactic Precession An Addendum to the Omni-Angular 2D Substrate Hypothesis

This addendum synthesizes observational data from the ESA Gaia DR2 mission (Visualized: Spaleta/Space.com) with the Omni-Angular 2D Substrate Hypothesis. It proposes that the observed galactic warp is not a collisional artifact but a mechanical byproduct of substrate shear. We explore the "Lily Pad" effect, where galactic mass union is achieved through the exhaustion of surrounding "Free Points," creating observed cosmic voids.

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Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-04-21
DOI
https://doi.org/10.5281/zenodo.19675759
Primary Topic
Galaxies: Formation, Evolution, Phenomena
Type
article
Field-Weighted Citation Impact
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article

Substrate Tension as a Driver for Galactic Precession An Addendum to the Omni-Angular 2D Substrate Hypothesis

Nicolas Antony Brown
Zenodo (CERN European Organization for Nuclear Research)
Galaxies: Formation, Evolution, Phenomena
article

Substrate Tension as a Driver for Galactic Precession An Addendum to the Omni-Angular 2D Substrate Hypothesis

Nicolas Antony Brown
article en

Abstract

This addendum synthesizes observational data from the ESA Gaia DR2 mission (Visualized: Spaleta/Space.com) with the Omni-Angular 2D Substrate Hypothesis. It proposes that the observed galactic warp is not a collisional artifact but a mechanical byproduct of substrate shear. We explore the "Lily Pad" effect, where galactic mass union is achieved through the exhaustion of surrounding "Free Points," creating observed cosmic voids.

Zenodo (CERN European Organization for Nuclear Research)
Openalex Percentile: Top 6%
Galaxies: Formation, Evolution, Phenomena
DOIOpen Access PDFOpenAlex
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Substrate Tension as a Driver for Galactic Precession An Addendum to the Omni-Angular 2D Substrate Hypothesis — Nicolas Antony Brown · Zenodo (CERN European Organization for Nuclear Research) (2026) | TGRS Research Map | TGRS