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ZENODO
Preprint . 2026
License: CC BY
Data sources: ZENODO
ZENODO
Preprint . 2026
License: CC BY
Data sources: Datacite
ZENODO
Preprint . 2026
License: CC BY
Data sources: Datacite
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Galaxy Rotation Curves Without Dark Matter from a Baryon-Sourced Suppression Field

Authors: Muthuswamy, Parndhaman;

Galaxy Rotation Curves Without Dark Matter from a Baryon-Sourced Suppression Field

Abstract

Galaxy rotation curves exhibit a well-known deviation from Newtonian expectations, traditionally attributed to non-baryonic dark matter halos. In this work, we show that the full radial structure of observed rotation curves, including inner Newtonian behavior, enhanced intermediate velocities, and normalization at large radii, emerges naturally from a baryon-sourced suppression field. Using an updated exponential suppression formulation, rotation curves are predicted directly from observed baryonic mass distributions, with no dark matter, no halo profiles, no parameter fitting, and no auxiliary corrections. The resulting predictions are compared against SPARC galaxy data, demonstrating that the observed rotation curve phenomenology can be explained without invoking non-baryonic matter components.

Keywords

Spiral galaxies, Mass Distribution, Galaxy rotation curves, SPARC database, Radial velocity profiles, Galactic dynamics

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
Average
Average
Average
Green