MOND-like behavior in the Dirac-Milne universe -- Flat rotation curves and mass/velocity relations in galaxies and clusters
Gabriel Chardin, Yohan Dubois, Giovanni Manfredi, Bruce Miller,, Cl\'ement Stahl

TL;DR
This paper demonstrates that the Dirac-Milne universe naturally produces flat galaxy rotation curves, Tully-Fisher and Faber-Jackson relations, and mimics MOND-like behavior, offering an alternative explanation to dark matter and dark energy.
Contribution
It introduces the Dirac-Milne cosmology as a matter-antimatter symmetric universe that reproduces key galactic dynamics and gravitational effects similar to MOND, with novel simulation results.
Findings
Rotation curves are flat beyond 3 virial radii.
A Tully-Fisher relation with exponent ~3 is satisfied.
The model reproduces a MOND-like additional surface gravity.
Abstract
We show that in the Dirac-Milne universe (a matter-antimatter symmetric universe where the two components repel each other), rotation curves are generically flat beyond the characteristic distance of about 3 virial radii, and that a Tully-Fisher relation with exponent is satisfied. Using 3D simulations with a modified version of the RAMSES code, we show that the Dirac-Milne cosmology presents a Faber-Jackson relation with a very small scatter and an exponent equal to between the mass and the velocity dispersion. We also show that the mass derived from the rotation curves assuming Newtonian gravity is systematically overestimated compared to the mass really present. We also show that the Dirac-Milne universe, featuring a polarization between its matter and antimatter components, presents a behavior similar to that of MOND (Modified Newtonian Dynamics),…
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.
