Fitting dwarf galaxy rotation curves with conformal gravity
James G. O'Brien, Philip D. Mannheim

TL;DR
This study demonstrates that conformal gravity can accurately fit the rotation curves of 138 galaxies, including dwarf galaxies, without requiring dark matter, highlighting the theory's potential as an alternative to dark matter in explaining galactic dynamics.
Contribution
The paper extends previous conformal gravity analyses to include 27 additional galaxies, mainly dwarfs, confirming the theory's ability to fit rotation curves without dark matter across a larger sample.
Findings
Conformal gravity fits 138 galaxy rotation curves successfully.
The theory accounts for systematics across diverse galaxy types.
Dark matter is unnecessary when considering global physics contributions.
Abstract
We continue our study of the application of the conformal gravity theory to galactic rotation curves. Previously we had studied a varied 111 spiral galaxy sample consisting of high surface brightness galaxies, low surface brightness galaxies and dwarf galaxies. With no free parameters other than galactic mass to light ratios, we had found that the theory is able to account for the systematics that is observed in the entire set of galactic rotation curves without the need for any dark matter whatsoever. In the present paper we extend our study to incorporate a further 27 galaxies of which 25 are dwarf galaxies and provide updated studies of 3 additional galaxies that had been in the original sample, and again without dark matter find fully acceptable fits, save only for just a few galaxies that we find to be somewhat troublesome. Our current study brings to 138 the number of rotation…
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.
