Black Hole Solutions in Rastall Theory
Y. Heydarzade, H. Moradpour, F. Darabi

TL;DR
This paper derives black hole solutions within Rastall gravity, showing the cosmological constant emerges naturally from the theory's field equations, and explores various known black hole solutions as special cases.
Contribution
It presents the first derivation of Reissner-Nordström black holes in Rastall gravity with a natural cosmological constant.
Findings
Reissner-Nordström solution in Rastall gravity obtained
Cosmological constant arises naturally from field equations
Includes Schwarzschild and (anti-)de Sitter solutions as special cases
Abstract
The Reissner-Nordstr\"om black hole solution in a generic cosmological constant background in the the context of Rastall gravity is obtained. It is shown that the cosmological constant arises naturally from the consistency of the non-vacuum field equations of the Rastall theory for a spherical symmetric spacetime, rather than its {\it ad-hoc} introduction in the usual Einstein and Einstein-Maxwell field equations. The usual Reissner-Nordstr\"om, Schwarzschild and Schwarzschild-(anti)de Sitter black hole solutions in the framework of this theory are also addressed as the special independent subclasses of the obtained general solution.
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.
