A Model of f(R) Gravity as an Alternative for Dark Matter in Spiral Galaxies
Solmaz Asgari, Reza Saffari

TL;DR
This paper derives a metric f(R) gravity model that explains flat rotation curves in spiral galaxies without dark matter, aligning with key astrophysical relations like Tully-Fisher and MOND.
Contribution
It introduces a generic f(R) gravity action consistent with galactic rotation curves, providing an alternative explanation to dark matter.
Findings
Solutions match observed flat rotation curves
Consistent with Tully-Fisher relation
Aligns with modified Newtonian dynamics
Abstract
In this paper we study consistent solutions of spherically symmetric space in metric f(R) gravity theory. Here we inversely obtain a generic action from metric solutions that describe flat rotation curves in spiral galaxies without dark matter. Then we show that obtained solutions are in conformity with Tully-Fisher relation and modified Newtonian dynamics, which are two strong constraints in justification of flat rotation curves in spiral galaxies.
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.
