二进制中子星银河系中引力波的观测限制
广义相对论与量子宇宙学
2012-08-27 v2 天体物理学
摘要
使用最优匹配滤波技术，我们搜索来自银河系内合并二进制系统发出的引力波啸叫信号。这是对该滤波技术在真实光学干涉仪数据上首次的测试。获得了银河系中中子星二进制惊喜的速率上限：以90%的置信水平，R< 0.5/小时。类似的实验将对宇宙中紧密二进制中子星系统的 Population 进行约束。
引用
@article{arxiv.gr-qc/9903108,
title = {Observational Limit on Gravitational Waves from Binary Neutron Stars in the Galaxy},
author = {B. Allen and J. K. Blackburn and P. R. Brady and J. D. E. Creighton and T. Creighton and S. Droz and A. D. Gillespie and S. A. Hughes and S. Kawamura and T. T. Lyons and J. E. Mason and B. J. Owen and F. J. Raab and M. W. Regehr and B. S. Sathyaprakash and R. L. Savage, and S. Whitcomb and A. G. Wiseman},
journal= {arXiv preprint arXiv:gr-qc/9903108},
year = {2012}
}
备注
RevTeX, minor revisions, exactly as published in PRL 83 (1999) p1498, 4 pages, 2 figures included