MOND and the mass discrepancies in tidal dwarf galaxies
Mordehai Milgrom

TL;DR
This paper demonstrates that MOND accurately predicts the rotation curves of three tidal dwarf galaxies without requiring dark matter, challenging the cold dark matter paradigm.
Contribution
It shows that MOND can explain the observed velocities of tidal dwarf galaxies solely with visible baryonic matter, countering claims for additional dark matter in these systems.
Findings
MOND predictions align with observed velocities
No need for additional dark matter in tidal dwarf galaxies
Challenges the cold dark matter paradigm in these cases
Abstract
I consider in light of MOND the three debris galaxies discussed recently by Bournaud et al.. These exhibit mass discrepancies of a factor of a few within several scale lengths of the visible galaxy, which, arguably, flies in the face of the cold dark matter paradigm. I show here that the rotational velocities predicted by MOND agree well with the observed velocities for each of the three galaxies, with only the observed baryonic matter as the source of gravity. There is thus no need to invoke a new form of baryonic, yet-undetected matter that dominates the disc of spiral galaxies, as advocated by Bournaud et al. I argue on other grounds that the presence of such ubiquitous disc dark matter, in addition to cold dark matter, is not likely.
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.
