Square-torsion gravity, dark matter halos and the baryonic Tully-Fisher relation
Elias A. S. M\'egier

TL;DR
This paper applies square-torsion gravity to model dark matter halos, deriving solutions that reproduce galactic rotation curves and the baryonic Tully-Fisher relation, offering a theoretical basis for this empirical law.
Contribution
It introduces a novel application of square-torsion gravity to dark matter, deriving exact solutions and explaining galactic rotation phenomena within this framework.
Findings
Dark stress-energy tensor satisfies an anisotropic structure equation.
Static solutions model dark matter halos around baryonic bodies.
Reproduces the baryonic Tully-Fisher relation in the Newtonian regime.
Abstract
Square-torsion gravity is applied to the long standing dark matter problem. In this context the theory reduces to General Relativity complemented by a dark stress-energy tensor due to the torsion of spacetime and is studied under the simplifying assumption of spherical symmetry. The dark stress-energy tensor is found to satisfy an anisotropic structure equation. In vacuum this is shown to be equivalent to a wave equation with sources. A natural class of exact solutions is found which explicitly perturbs any seed spacetime metric by a conformal factor satisfying a (1+1)-dimensional wave equation. This leads to the concept of dark coating. The static solutions are then used to construct structures that model dark matter halos surrounding baryonic bodies. In the Newtonian r\'egime the baryonic mass and the flat rotation curve velocity are found to be related by the baryonic…
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.
