LIMITS ON GRAVITATIONAL RADIATION FROM 2 GRAVITATIONALLY BOUND BLACK HOLES

被引：7

作者：

GIBBONS, GW

SCHUTZ, BF

机构：

[1] Department of Applied Mathematics and Theoretical Physics, University of Cambridge, Silver Street, Cambridge, United Kingdom

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1972年 / 159卷 / 04期

关键词：

657.2 Extraterrestrial Physics and Stellar Phenomena - 931.5 Gravitation; Relativity and String Theory;

D O I：

10.1093/mnras/159.1.41P

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Upper bounds are computed for the energy emitted in gravitational radiation by two black holes falling into one another from rest at a range of separations. It is shown that before the ratio of total mass to proper separation exceeds 0.759 an event horizon must have formed around both. © 1972 Royal Astronomical Society. Provided by the NASA Astrophysics Data System.

引用

页码：P41 / &

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