Static spherically symmetric solutions in mimetic gravity: rotation curves and wormholes
By Ratbay Myrzakulov, Lorenzo Sebastiani, S. Vagnozzi, Sergio Zerbini. 2015
164 citations recorded by the source corpus.
In this work, we analyse static spherically symmetric solutions in the framework of mimetic gravity, an extension of general relativity where the conformal degree of freedom of gravity is isolated in a covariant fashion. Here we extend previous works by considering, in addition, a potential for the mimetic field. An appropriate choice of such a potential allows for the reconstruction of a number of interesting cosmological and astrophysical scenarios. We explicitly show how to reconstruct such a potential for a general static spherically symmetric space-time. A number of applications and scenarios are then explored, among which are traversable wormholes. Finally, we analytically reconstruct potentials, which leads to solutions to the equations of motion featuring polynomial corrections to the Schwarzschild space-time. Accurate choices for such corrections could provide an explanation for the inferred flat rotation curves of spiral galaxies within the mimetic gravity framework, without the need for particle dark matter.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/46ea2571d83cced93176714878009105fd54615c
Citations in the corpus
- Magnetically charged black holes from non-linear electrodynamics and the Event Horizon Telescope (2019, unknown): “[78–112].”
- Black holes with scalar hair in light of the Event Horizon Telescope (2020, unknown): “[199–229].”