Dynamical effects of the scale invariance of the empty space: The fall of dark matter ?
Andre Maeder

TL;DR
This paper proposes a cosmological model based on the scale invariance of empty space that explains accelerated expansion and galaxy rotation curves without dark matter or dark energy, supported by modified equations of motion and virial theorem.
Contribution
It introduces a new theoretical framework linking scale invariance to cosmological dynamics, eliminating the need for dark matter and dark energy in explaining observations.
Findings
Clusters' dynamical masses are 5-10 times smaller than standard estimates.
Galaxy rotation curves can be explained as an age effect without dark matter.
The model accounts for the increase in stellar velocity dispersion with age.
Abstract
The hypothesis of the scale invariance of the macroscopic empty space, which intervenes through the cosmological constant, has led to new cosmological models. They show an accelerated cosmic expansion and satisfy several major cosmological tests. No unknown particles are needed. Developing the weak field approximation, we find that the here derived equation of motion corresponding to Newton's equation also contains a small outwards acceleration term. The new term is particularly significant for very low density systems. A modified virial theorem is derived and applied to clusters of galaxies. For the Coma and Abell 2029 clusters, the dynamical masses are about a factor of 5 to 10 smaller than in the standard case. This tends to let no room for dark matter in these clusters. Then, the two-body problem is studied and an equation corresponding to the Binet equation is obtained. The…
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.
