Overview
Reconstructs supporting-power ratios required by published rotation curves for DDO 154, NGC 2403, and NGC 7814 under the adopted OQG correspondence. The fitted profile describes two of the three galaxies at the adopted error level and misses substantial structure in NGC 2403. These inferred requirements are targets for a microscopic scattering model; they do not establish a replacement for dark matter.
Publication and version record
Author manuscript selected by the founding editor for Volume 1, Issue 1. Inclusion does not represent independent JOATP peer review.
Included in the JOATP founding collection, 20 October 2026. The author retains copyright; original publisher terms continue to apply to previously published work.
Supporting materials
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