Quantum Effects in Black Hole Interiors
General Relativity and Quantum Cosmology
2009-10-22 v1
Abstract
The Weyl curvature inside a black hole formed in a generic collapse grows, classically without bound, near to the inner horizon, due to partial absorption and blueshifting of the radiative tail of the collapse. Using a spherical model, we examine how this growth is modified by quantum effects of conformally coupled massless fields.
Cite
@article{arxiv.gr-qc/9210013,
title = {Quantum Effects in Black Hole Interiors},
author = {Warren G. Anderson and Patrick R. Brady and Werner Israel and Sharon M. Morsink},
journal= {arXiv preprint arXiv:gr-qc/9210013},
year = {2009}
}
Comments
13 pages, 1 figure (not included), RevTex