Galaxy rotation curves incorporating relativistic mass and comparison with Keplerian velocity curves
Jaroslaw S. Jaracz

TL;DR
This paper introduces a relativistic correction to galaxy mass distribution calculations, showing it has a small dark-matter-like effect and significantly alters rotation curves compared to Keplerian predictions.
Contribution
It derives a relativistic mass correction formula for galaxy rotation curves and compares its effects to non-relativistic models and Keplerian curves.
Findings
Relativistic correction has a small dark-matter-like effect.
Corrected rotation curves are higher than Keplerian curves away from the center.
Discrepancy increases towards the galactic edge.
Abstract
We derive a formula for the velocity distribution of an axially symmetric galaxy where the mass density is corrected using the mass formula from special relativity. We take some reasonable test mass densities and numerically compute the resulting galaxy rotation curves. We then compare these to the rotation curves obtained from a similar formula without a relativistic correction factor. We find that the correction factor has a small dark-matter like effect. Finally, we compare these to the corresponding Keplerian velocity curves. We find that there is a large discrepancy in this case, where away from the galactic center, up to the galactic edge, the curves computed using our formulas give a noticeably higher velocity.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsGeophysics and Gravity Measurements · Relativity and Gravitational Theory · Cosmology and Gravitation Theories
