在 O3 早期 LIGO 数据中全天空搜索来自双星系统中未知中子星的连续引力波信号
广义相对论与量子宇宙学
2021-03-22 v2 高能天体物理现象
摘要
快速旋转的中子星是持久的连续引力波的有望来源。探测此类信号将允许探测极端条件下物质的物理性质。已知脉冲星种群的很大一部分属于双星系统。搜索双星系统中的未知中子星需要专门的算法以应对未知轨道频率调制。我们提出一项利用半相干、GPU 加速的 BinarySkyHough 流水线，在 Advanced LIGO 与 Advanced Virgo 探测器的第三次观测运行早期数据中搜索双星系统内中子星发射的连续引力波。该搜索分析了 LIGO 探测器最灵敏的频带，50 - 300 Hz。双星轨道参数被划分为四个区域，包含 3 - 45 天的轨道周期与 2 - 40 光秒的投影半长轴。未报告探测结果。我们使用模拟连续波信号估计搜索的灵敏度，在分析的参数空间内实现了迄今最灵敏的结果。
引用
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journal= {arXiv preprint arXiv:2012.12128},
year = {2021}
}
备注
23 pages, 12 figures, 7 tables