Black hole horizon fluctuations

被引：40
|
作者：
Casher, A
Englert, F
Itzhaki, N
Massar, S
Parentani, R
机构：
[1] FREE UNIV BRUSSELS, SERV PHYS THEOR, B-1050 BRUSSELS, BELGIUM
[2] ECOLE NORMALE SUPER, PHYS THEOR LAB, UPR CNRS, F-75231 PARIS 05, FRANCE
[3] UNIV PARIS SUD, F-75231 PARIS 05, FRANCE
来源：
NUCLEAR PHYSICS B | 1997年 / 484卷 / 1-2期
关键词：
black hole; Hawking radiation;
D O I：
10.1016/S0550-3213(96)00613-X
中图分类号：
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号：
摘要：
Some authors have suggested that gravitational interactions become large at an invariant distance of order 1 from the black hole horizon. We show that due to the ''atmosphere'' of high angular particles near the horizon strong gravitational interactions already occur at an invariant distance of the order of 3 root M. The implications of these results for the origin of black hole radiation, the meaning of black hole entropy and the information puzzle are discussed.
引用
收藏
页码：419 / 434
页数：16
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