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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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RSFT Section 14: Quantitative Galactic Rotation Curves and Bullet Cluster Offset from Layer 204 Dark Matter

Authors: Bell, Anthony;

RSFT Section 14: Quantitative Galactic Rotation Curves and Bullet Cluster Offset from Layer 204 Dark Matter

Abstract

In this document, I provide quantitative evidence for the RSFT dark matter mechanism by modeling galactic rotation curves and the Bullet Cluster collision. I demonstrate that the pseudo-isothermal halo profile emerges naturally from the resonant mode structure of layer 204, allowing me to predict flat rotation curves at large radii. By applying a single global core radius parameter across five diverse galaxies, I achieved a mean residual of only 7.6% without any per-galaxy adjustments. Furthermore, I used the coupling constant derived in earlier sections to show that dark matter in the Bullet Cluster experiences only 0.17% of the drag force felt by gas. This calculation resulted in a predicted dark matter offset of 188 kpc, which aligns closely with the observed 160 kpc distance, confirming that the gravitational lensing follows the dark matter peak as expected.

Keywords

RSFT, Bullet Cluster, NGC 7331, gravitational lensing, coupling constant, dark matter, core radius, NGC 2403, pseudo-isothermal halo, NGC 6503, rotational substrate field theory, layer 204, galactic rotation curves, DDO 154, galactic halo, resonant modes, electromagnetic drag

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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