Galactic dark matter as a bulk effect on the brane
C. G. Boehmer, T. Harko

TL;DR
This paper explores how dark matter effects in galaxies can be explained by a brane world model, deriving exact solutions and observable predictions related to galactic rotation curves.
Contribution
It provides an exact analytic solution for vacuum gravitational fields on the brane with constant tangential velocity, linking dark radiation and dark pressure to observable galactic parameters.
Findings
Derived explicit form of bulk Weyl tensor projections on the brane.
Expressed physical quantities in terms of observable galactic parameters.
Provided a framework for testing brane world models with galactic rotation data.
Abstract
The behavior of the angular velocity of a test particle moving in a stable circular orbit in the vacuum on the brane is considered. In the brane world scenario, the four dimensional effective Einstein equation acquire extra terms, called dark radiation and dark pressure, respectively, which arise from the embedding of the 3-brane in the bulk. A large number of independent observations have shown that the rotational velocities of test particles gravitating around galaxies tend, as a function of the distance from the galactic center, toward constant values. By assuming a constant tangential velocity, the general solution of the vacuum gravitational field equations on the brane can be obtained in an exact analytic form. This allows us to obtain the explicit form of the projections of the bulk Weyl tensor on the brane, and the equation of state of the dark pressure as a function of the dark…
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.
