Slowly rotating and charged Black-holes in Entangled Relativity
General Relativity and Quantum Cosmology
2025-02-06 v2
Abstract
Entangled Relativity is a non-linear reformulation of Einstein's General Theory of Relativity (General Relativity) that offers a more parsimonious formulation. This non-linear approach notably requires the simultaneous definition of matter fields, thus aligning more closely with Einstein's \textit{principle of relativity of inertia} than General Relativity does. Solutions for spherically charged black holes have already been identified. After exploring further some of the properties of these solutions, we present new solutions for the field equations pertaining to slowly rotating charged black holes.
Keywords
Cite
@article{arxiv.2411.09327,
title = {Slowly rotating and charged Black-holes in Entangled Relativity},
author = {Maxime Wavasseur and Theo Abrial and Olivier Minazzoli},
journal= {arXiv preprint arXiv:2411.09327},
year = {2025}
}
Comments
17 pages. V2: minor changes