CDN-264: The SPARC Fit — GCFT Computational Discovery Note
Fits GCFT coupling parameters (κ_cl, a_t, γ) directly to the SPARC Radial Acceleration Relation (14 bins, 2630 data points, 153 galaxies). Best-fit: κ_cl=0.210, a_t/a₀=2.20, γ=0.76 — radically different from the dSph-calibrated CDN-258 values. Functional form marginally survives kill condition (RMS 0.046 ≤ 0.05 dex) but remains 2.4× worse than MOND simple. Cross-check against 22 dwarf spheroidals: 0/22 within 20% at any parameter set, with predicted velocity dispersions 15–50× too low. Joint optimization finds no connecting valley between galaxy-RAR and dSph parameter space. Two-sector coupling definitively confirmed. CDN-265 pre-registered for alternative functional forms.
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.20725155
- Primary Topic
- Galaxies: Formation, Evolution, Phenomena
- Type
- article
- Field-Weighted Citation Impact
- 0.00