Black-holes and neutron stars in entangled relativity
General Relativity and Quantum Cosmology
2022-03-22 v1
Abstract
I present two results that show that, despite its unusual non-linear form, the phenomenology of entangled relativity remains close to the one of general relativity -- without having any free parameter that can be fine tuned in order to facilitate this. In particular, I present the analytical solutions for spherically charged black-holes, and both the analytical and numerical solutions for neutron stars.
Cite
@article{arxiv.2203.11122,
title = {Black-holes and neutron stars in entangled relativity},
author = {Olivier Minazzoli},
journal= {arXiv preprint arXiv:2203.11122},
year = {2022}
}
Comments
Contribution to the 2022 Gravitation session of the 56th Rencontres de Moriond