Assesses rotation curves in galaxies, highlighting their dynamical behavior under different models.
Applies CDN-258 unbounded κ(a) = 0.152·(1+(a_t/a)^1.10) to 12 galaxy rotation curves (102 radial points, M_bar = 5×10⁷–1.2×10¹¹ M☉) with zero free parameters. GCFT: 77% within 20%, wins 4/12 low-mass irregulars. MOND: 87% within 20%, wins 8/12. D9 paid in full; D10 opened (γ scale-dependence).
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Nicky Joseph Hubertus Catharina Hacquier (2026) studied this question.
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