Cauchy horizon singularity without mass inflation
General Relativity and Quantum Cosmology
2009-10-22 v1 Astrophysics
Abstract
A perturbed Reissner-Nordstr\"om-de Sitter solution is used to emphasize the nature of the singularity along the Cauchy horizon of a charged spherically symmetric black hole. For these solutions, conditions may prevail under which the mass function is bounded and yet the curvature scalar diverges.
Cite
@article{arxiv.gr-qc/9211026,
title = {Cauchy horizon singularity without mass inflation},
author = {P. R. Brady and D. Nunez and S. Sinha},
journal= {arXiv preprint arXiv:gr-qc/9211026},
year = {2009}
}
Comments
typeset in RevTex, 13 pages