Spiral Galaxies Rotation Curves with a Logarithmic Corrected Newtonian Gravitational Potential
J.C. Fabris, J.P. Campos

TL;DR
This paper introduces a logarithmic correction to Newtonian gravity to better fit spiral galaxy rotation curves, suggesting a potential link to string theory and discussing its consistency with local physics.
Contribution
The study proposes a novel logarithmic correction to Newtonian potential that accurately models galaxy rotation curves, offering a new perspective on gravitational modifications.
Findings
Rotation curves are well fitted with the corrected potential.
A new constant in the potential correlates with galaxy data.
The correction may originate from string configurations.
Abstract
We analyze the rotation curves of 10 spiral galaxies with a newtonian potential corrected with an extra logarithmic term, using a disc modelization for the spiral galaxies. There is a new constant associated with the extra term in the potential. The rotation curve of the chosen sample of spiral galaxies is well reproduced for a given range of the new constant. It is argued that this correction can have its origin from string configurations. The compatibility of this correction with local physics is discussed.
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.
