QUANTUM EFFECTS IN BLACK-HOLE INTERIORS

被引:21
作者
ANDERSON, WG
BRADY, PR
ISRAEL, W
MORSINK, SM
机构
[1] Canadian Institute for Advanced Research Cosmology Program, Theoretical Physics Institute, University of Alberta, Edmonton
关键词
D O I
10.1103/PhysRevLett.70.1041
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
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.
引用
收藏
页码:1041 / 1044
页数:4
相关论文
共 20 条
[1]  
ADLER SL, 1977, ANN PHYS-NEW YORK, V106, P27
[2]  
ANDERSON WG, IN PRESS CLASSICAL Q
[3]   HOW SINGULAR ARE BLACK-HOLE INTERIORS [J].
BALBINOT, R ;
BRADY, PR ;
ISRAEL, W ;
POISSON, E .
PHYSICS LETTERS A, 1991, 161 (03) :223-226
[4]   MASS INFLATION - THE SEMICLASSICAL REGIME [J].
BALBINOT, R ;
POISSON, E .
PHYSICAL REVIEW LETTERS, 1993, 70 (01) :13-16
[5]   COVARIANT PERTURBATION-THEORY .2. 2ND-ORDER IN THE CURVATURE - GENERAL ALGORITHMS [J].
BARVINSKY, AO ;
VILKOVISKY, GA .
NUCLEAR PHYSICS B, 1990, 333 (02) :471-511
[6]  
BIRRELL ND, 1989, QUANTUM FIELDS CURVE
[7]   CONFORMAL INVARIANCE AND ASYMPTOTIC FREEDOM IN QUANTUM GRAVITY [J].
FRADKIN, ES ;
VILKOVISKY, GA .
PHYSICS LETTERS B, 1978, 77 (03) :262-266
[8]   SPHERICALLY SYMMETRIC COLLAPSE IN QUANTUM-GRAVITY [J].
FROLOV, VP ;
VILKOVISKY, GA .
PHYSICS LETTERS B, 1981, 106 (04) :307-313
[9]  
Fulling S A., 1989, ASPECTS QUANTUM FIEL, V1st edn
[10]   EVOLUTION OF THE INTERIOR OF A CHARGED BLACK-HOLE [J].
HISCOCK, WA .
PHYSICS LETTERS A, 1981, 83 (03) :110-112