Double Neutron Star Binaries: A "Foreground" Source for the Gravitational-Wave Stochastic Background

被引：0
|
作者：
Allen, Bruce [1 ,2 ]
机构：
[1] Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-30167 Hannover, Germany
[2] Univ Wisconsin, Milwaukee, WI 53201 USA
来源：
PROGRESS OF THEORETICAL PHYSICS SUPPLEMENT | 2011年 / 190期
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D O I：
暂无
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
Cosmological sources of gravitational wave backgrounds can be hidden by "foreground" sources: signals produced recently by normal astrophysical sources. Here, we briefly examine one such foreground source: the signals produced by the inspiral of Double Neutron Star (DNS) binaries. We do simple estimates of the spectrum and statistical properties of the resulting foreground, and discuss when the signals might be removable and when they form a central-limit-theorem confusion noise.
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页码：316 / 321
页数：6
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