A note on singular and non-singular black holes
General Relativity and Quantum Cosmology
2017-05-24 v2 High Energy Physics - Theory
Abstract
An attempt is made in order to clarify the so called regular black holes issue. It is revisited that if one works within General Relativity minimally coupled with non linear source, mainly of electromagnetic origin, and within a static spherically symmetric ansatz for the metric, there is still room for singular contribution to the black hole solution. A reconstruction method is proposed and several examples are discussed, including new ones. A possible way to obtain a non singular black hole is introduced, and in this case, several known examples are re-discussed, and new ones are provided.
Cite
@article{arxiv.1704.08516,
title = {A note on singular and non-singular black holes},
author = {Stefano Chinaglia and Sergio Zerbini},
journal= {arXiv preprint arXiv:1704.08516},
year = {2017}
}
Comments
15 pages, version to appear in GRG, references added