Quantum Effects in Black Hole Interiors

Preprint

23 October 1992

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.gr-qc/9210013

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.

Keywords

BLACK HOLE INTERIORS
CONFORMALLY COUPLED
QUANTUM EFFECTS
HOLE INTERIORS
WEYL CURVATURE
ABSORPTION

All Related Versions

Version 1, 1992-10-23, ArXiv
Published version: Physical Review Letters, 70 (8), 1041.

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