Galactic dark matter effects from purely geometrical aspects of general relativity
Davide Astesiano, Matteo Luca Ruggiero
Abstract
We study disk galaxies in the framework of general relativity to focus on the possibility that, even in the low energy limit, there are relevant corrections with respect to the purely Newtonian approach. Our analysis encompasses the model by considering both a low energy expansion and exact solutions, making clear the connection between these different approaches. In particular, we focus on two different limits: the well-known gravitomagnetic analogy and a new limit, called ``strong gravitomagnetism,'' which has corrections in $c$ of the same order as the Newtonian terms. We show that these two limits of the general class of solutions can account for the observed flat velocity profile, which is contrary to what happens using Newtonian models, where a dark matter contribution is required. Hence, we suggest a geometrical origin for a certain amount of dark matter effects.