探测引力波信号的信息熵方法

Z. Zhanabaev
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引用次数: 0

摘要

引力波的探测来自一对合并的黑洞,标志着GW天文学时代的开始。传统上,为了从实验数据中提取引力波信号,科学合作使用标准匹配滤波技术。匹配滤波技术依赖于现有的波形模板,这使得很难找到超出理论预期的引力波信号。此外,匹配过滤器的计算成本非常高,因为它取决于所使用的模板的数量。在本文中,我们提出了一种新的信息熵方法用于引力波探测,它不需要信号模板的理论库。为了证明我们方法的可靠性,我们用模拟数据和真实数据进行了分析。通过这项研究,我们发现我们的条件信息测量可以检测到引力波信号,并且可以与匹配滤波方法一起使用。
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INFORMATION-ENTROPY METHOD FOR DETECTING GRAVITATIONAL WAVE SIGNALS
The detection of gravitational waves came from a pair of merging black holes marked the beginning of the era of GW astronomy. Traditionally, to extract gravitational wave signals from experimental data, the scientific collaborations use the standard matched filtering technique. The matched filtering technique relies on the existing waveform templates, that makes it difficult to find gravitational wave signals that go beyond theoretical expectations. Moreover, the computational cost of matched filter is veryhigh, as it depends on the number of templates used. In this article, we propose a new information-entropy method for gravitational waves detection that does not require a theoretical bank of signal templates. To demonstrate the reliability of our method we conducted an analysis using simulated and real data. Through this study, we revealed that our measure of conditional information detects the gravitational wave signals and can be used along with the matched filtering method.
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