Randomized trial tests Baryonic Tully-Fisher Relation in galaxies, suggesting stronger predictions from GCFT's model.
Establishes GCFT's κ(a) as a MOND interpolation function ν(x)=1+κ(x·a₀). Tests the Baryonic Tully-Fisher Relation: GCFT QUMOND slope (3.408) tracks observed (3.429) better than MOND simple (3.095) on 12 CDN-260 galaxies. Identifies External Field Effect tension for nearby ultrafaint dSphs. D11 reframed from "what is κ?" to "why this interpolation function?" Pre-registers CDN-263 for EFE resolution.
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Nicky Joseph Hubertus Catharina Hacquier (2026) studied this question.
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