Astrophysics of double neutron star binaries

被引：0
|
作者：
Belczynski, Krzysztof [1 ]
机构：
[1] New Mexico State Univ, Las Cruces, NM 88003 USA
来源：
Laser Interferometer Space Antenna | 2006年 / 873卷
关键词：
binaries : close; stars; evolution; neutron; gravitation;
D O I：
暂无
中图分类号：
V [航空、航天];
学科分类号：
08 ; 0825 ;
摘要：
I present a study of galactic population of double neutron star binaries to investigate if any of these systems can potentially be detected with LISA at low gravitational-wave frequencies. The number and physical properties of double neutron star systems in the Galaxy are calculated using population synthesis method. It is found that, although formation efficiency is very small, ten to hundred of such systems should be detectable with LISA depending on the instrument low-frequency sensitivity.
引用
收藏
页码：406 / 414
页数：9
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