Quasi-Normal Modes of a Schwarzschild White Hole
General Relativity and Quantum Cosmology
2009-09-24 v1
Abstract
We investigate perturbations of the Schwarzschild geometry using a linearization of the Einstein vacuum equations within a Bondi-Sachs, or null cone, formalism. We develop a numerical method to calculate the quasi-normal modes, and present results for the case . The values obtained are different to those of a Schwarzschild black hole, and we interpret them as quasi-normal modes of a Schwarzschild white hole.
Keywords
Cite
@article{arxiv.0907.1882,
title = {Quasi-Normal Modes of a Schwarzschild White Hole},
author = {Nigel T. Bishop and Amos S. Kubeka},
journal= {arXiv preprint arXiv:0907.1882},
year = {2009}
}
Comments
5 pages, 4 Figures