Quantum effects in black hole interiors

22 February 1993

journal article
Published by American Physical Society (APS) in Physical Review Letters

Vol. 70 (8) , 1041-1044
https://doi.org/10.1103/physrevlett.70.1041

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.Comment: 13 pages, 1 figure (not included), RevTe

Keywords

BLACK HOLE
QUANTUM
COLLAPSE GROWS
RADIATIVE TAIL
CONFORMALLY COUPLED
SPHERICAL MODEL
PARTIAL ABSORPTION

All Related Versions

Version 1, 1992-10-23, ArXiv

This publication has 2 references indexed in Scilit:

Mass inflation: The semiclassical regime
Physical Review Letters, 1993
How singular are black hole interiors?
Physics Letters A, 1991