1992/10/23 by Warren G. Anderson, W. G. Anderson, Patrick R. Brady +4 · 2 citations
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Quantum Electrodynamics and Casimir Effect #gr-qc
paper · pdf · doi:10.1103/physrevlett.70.1041
published as Phys.Rev.Lett. 70 (1993) 1041-1044 · 13 pages, 1 figure (not included), RevTex
arxiv created 1992/10/23 · openalex publication_date 1993/02/22 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
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.