A stochastic background from extra-galactic double neutron stars

被引：24
|
作者：
Regimbau, T. [1 ]
Chauvineau, B. [1 ]
机构：
[1] Observ Cote Azur, Dept ARTEMIS, F-06304 Nice, France
来源：
CLASSICAL AND QUANTUM GRAVITY | 2007年 / 24卷 / 19期
关键词：
D O I：
10.1088/0264-9381/24/19/S25
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We present Monte Carlo simulations of the extra galactic population of inspiralling double neutron stars, and estimate its contribution to the astrophysical gravitational wave background, in the frequency range of ground-based interferometers, corresponding to the last 1000 s before the last stable orbit when more than 96% of the signal is released. We show that sources at redshift z > 0.5 contribute to a truly continuous background which may be detected by correlating third generation interferometers.
引用
收藏
页码：S627 / S637
页数：11
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