Structural Constraints Leading to a Tully–Fisher–Type Scaling
Abstract
This work derives a Tully–Fisher–type scaling as a structural consequence of causal cosmology. By combining dimensional consistency with global causal constraints, we show that a relation of the form v^4 ∝ M arises without invoking modified gravity, dark matter phenomenology, or observational fitting. The result functions as a structural constraint on admissible galactic scaling relations rather than as a dynamical explanation of rotation curves.
Fields of Study & Subjects
Galaxies: Formation
Evolution
Phenomena
Cosmology and Gravitation Theories
Stellar
planetary
and galactic studies
Publication details
- Journal / source
- Zenodo (CERN European Organization for Nuclear Research)
- Publication date
- 29 January 2026
- Language
- EN