CDN-262 — The Tully-Fisher Prediction (GCFT Art Edition)
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.
Authors
- Nicky Joseph Hubertus Catharina Hacquier (ORCID: https://orcid.org/0009-0004-8093-976X)
Institutions
- Dynamique du noyau (FR)
Publication Details
- Journal
- Zenodo (CERN European Organization for Nuclear Research)
- Published
- 2026-06-17
- DOI
- https://doi.org/10.5281/zenodo.20724995
- Primary Topic
- Galaxies: Formation, Evolution, Phenomena
- Type
- article
- Field-Weighted Citation Impact
- 0.00