Effective black hole interior and the Raychadhuri equation
General Relativity and Quantum Cosmology
2022-03-07 v2
Abstract
We show that loop quantum gravity effects leads to the finiteness of expansion and its rate of change in the effective regime in the interior of the Schwarzschild black hole. As a consequence the singularity is resolved. We find this in line with previous results about curvature scalar and strong curvature singularities in Kantowski-Sachs model which is isometric to Schwarzschild interior.
Cite
@article{arxiv.2110.05397,
title = {Effective black hole interior and the Raychadhuri equation},
author = {Keagan Blanchette and Saurya Das and Samantha Hergott and Saeed Rastgoo},
journal= {arXiv preprint arXiv:2110.05397},
year = {2022}
}
Comments
This is the contribution to the Proceedings of the MG16 Conference. 11 pages, 4 figures; v2: citations added