Transmission and reflection coefficients for a scalar field inside a charged black hole
General Relativity and Quantum Cosmology
2009-10-30 v1
Abstract
Using the late-time expansion we calculate the leading-order coefficients describing the evolution of a massless scalar field inside a Reissner-Nordstrom black hole. These coefficients may be interpreted as the reflection and transmission coefficients for scalar-field modes propagating from the event horizon to the Cauchy horizon. Our results agree with those obtained previously by Gursel et al by a different method.
Keywords
Cite
@article{arxiv.gr-qc/9711034,
title = {Transmission and reflection coefficients for a scalar field inside a charged black hole},
author = {Amos Ori},
journal= {arXiv preprint arXiv:gr-qc/9711034},
year = {2009}
}
Comments
7 pages, RevTeX, no figures. Accepted to Phys. Rev. D (Brief Report)