LISA偏振分辨率

O. Jennrich, M. Peterseim, K. Danzmann
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引用次数: 4

摘要

我们讨论了LISA对固定频率和振幅的引力波的不同极化状态的分辨能力。假设双星作为引力波的源,它的方向与所发射的引力波的极化有关。利用信号处理的方法,计算了测量源方向的1-不确定度范围。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Polarization Resolution of LISA
We discuss LISA's ability to resolve different polarizational states of a gravitational wave with fixed frequency and amplitude. Assuming a binary as the source of the gravitational wave, its orientation is connected with the polarization of the gravitational wave emitted. Using methods of signal processing, we calculate the 1- uncertainty range for measuring the orientation of the source.
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