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Galaxy Rotation Curves Show a Surface-Density–Dependent Transition Geometry (κ–Σ) That MOND Does Not Reproduce: A Surface-Density-Constrained, Non-Tuned Framework Evaluated on 174 SPARC Galaxies

Fuente: Zenodo

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Détails bibliographiques
Auteur principal:	Stacey, Caleb
Format:	Recurso digital
Langue:	anglais
Publié:	Zenodo 2026
Sujets:	galaxy rotation curves SPARC dataset MOND comparison baryonic physics empirical model gravitational modeling emergent systems
Accès en ligne:	Acceder al recurso
Tags:	Ajouter un tag Pas de tags, Soyez le premier à ajouter un tag!

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