Dark matter, MOND or non-local gravity?
F. Darabi

TL;DR
This paper introduces a Machian model of gravity at galactic scales that aims to explain galaxy rotation curves without resorting to dark matter or MOND, offering a new perspective on gravitational interactions.
Contribution
It presents a novel Machian gravitational model that accounts for galactic rotation curves without dark matter or MOND, challenging existing paradigms.
Findings
Successfully reproduces galaxy rotation curves
Eliminates need for dark matter in galactic dynamics
Provides a new theoretical framework for gravity at large scales
Abstract
We propose a Machian model of gravitational interaction at galactic scales to explain the rotation curves of these large structures without the need for dark matter or MOND.
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 · Cosmology and Gravitation Theories · Geomagnetism and Paleomagnetism Studies
