Black-holes and neutron stars in entangled relativity

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.

Contribution to the 2022 Gravitation session of the 56th Rencontres de Moriond