Work

Structural Constraints Leading to a Tully–Fisher–Type Scaling

Year: 2026

Type: article

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.

Source: Zenodo (CERN European Organization for Nuclear Research)

DOI: 10.5281/zenodo.18408277

Author: Almeida, Matheus Wilker Magalhães de

Language: English

Topic: Galaxies: Formation, Evolution, Phenomena

Subfield: Astronomy and Astrophysics

Field: Physics and Astronomy

Domain: Physical Sciences

Open Access status: green

OpenAlex ID: W7126066617

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