© Synapse Social LLC, 2026개인정보 처리방침

피드 탐색 트렌드 질문 연구자

⌘K

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

February 2, 2026Open Access

Structural Constraints Leading to a Tully–Fisher–Type Scaling

Read Full Paperexternally

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.

Connected Papers

Building similarity graph...

Analyzing shared references across papers

Discussion

Loading...

Authors

M

Matheus Wilker Magalhães de Almeida Almeida

Actions

Institutions

ORCID

References and Citations

Connected Papers

Building similarity graph...

Analyzing shared references across papers

Discussion

Loading...

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