This model demonstrates emergent dark matter behaviors in galaxies and clusters, suggesting new observational predictions.
We present a field-theoretic model in which dark-matter phenomenology emerges from the dynamics of a self-organizing scalar field. The theory is fully specified, uses a single global parameter set, and reproduces galaxy rotation curves, gravitational lensing behavior, and collisionless dynamics in cluster mergers. In the quasi-static limit, the field admits an effective dark-fluid description that is emergent rather than fundamental. The model is falsifiable and makes testable observational predictions.
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Badour Nathan (2026) studied this question.
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