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.

引用

页码：L39 / L44

页数：6

共 12 条

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ANDERSSON, N
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ANDERSSON, N
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ANDERSSON, N
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[7] ON ALGEBRAICALLY SPECIAL PERTURBATIONS OF BLACK-HOLES
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[8] Chandrasekhar S., 1992, MATH THEORY BLACK HO
[9] BLACK-HOLE NORMAL-MODES - PHASE-INTEGRAL TREATMENT
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[10] FROMAN N, 1992, DISCOURSES MATH ITS, P121

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