Published January 30, 2022 | Version v1
Conference paper

Black-holes and neutron stars in entangled relativity

Description

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.

Abstract

International audience

Additional details

Created:
December 3, 2022
Modified:
November 29, 2023