TOTAL TRANSMISSION THROUGH THE SCHWARZSCHILD BLACK-HOLE POTENTIAL BARRIER

被引：12
作者：
ANDERSSON, N
机构：
[1] Department of Physics and Astronomy, University of Wales College of Cardiff
来源：
CLASSICAL AND QUANTUM GRAVITY | 1994年 / 11卷 / 03期
关键词：
D O I：
10.1088/0264-9381/11/3/001
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
A phase-integral condition determining frequencies for which a gravitational wave would pass through the curvature potential that surrounds a Schwarzschild black hole is derived. Numerical results obtained from this condition agree well with the eigenfrequencies that distinguish the so-called 'algebraically special' perturbations of the hole. The results suggest that the 'special' modes should perhaps be identified as total transmission solutions.
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收藏
页码：L39 / L44
页数：6
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