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Structural Constraints Leading to a Tully–Fisher–Type Scaling | Synapse

February 2, 2026Open Access

Structural Constraints Leading to a Tully–Fisher–Type Scaling

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Key Points

This research aims to derive a Tully–Fisher-type scaling from structural principles in causal cosmology.
Deriving scaling relations through dimensional consistency
Analyzing global causal constraints in cosmological contexts
Exploring implications without modifying gravity or dark matter phenomenology
Establishes a relation of the form v^4 ∝ M
Identifies structural constraints on galactic scaling relations
Findings challenge the need for observational fitting in traditional models

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 v⁴ ∝ 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.

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Cite this study

Matheus Wilker Magalhães de Almeida Almeida (Thu,) studied this question.

synapsesocial.com/papers/6980fc91c1c9540dea80e69d — DOI: https://doi.org/10.5281/zenodo.18408278

Authors

M

Matheus Wilker Magalhães de Almeida Almeida

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