Gravitational waves: Classification, Methods of detection, Sensitivities, and Sources
Gravitational waves: Classification, Methods of detection, Sensitivities, and Sources
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DOI：
10.1142/s0218271815300311
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发表时间：
2015-11
期刊：
影响因子：
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通讯作者：
K. Kuroda;W. Ni;Wei P. Pan
中科院分区：
文献类型：
--
作者：
K. Kuroda;W. Ni;Wei P. Pan
在对引力波进行了简要介绍和分类后，对引力波的探测方法、灵敏度和源进行了回顾和总结。我们注意到实时检测在300 pHz以上是可能的。低于300 pHz时，可以在导丝印记上或间接进行检测。我们即将被发现。这一领域的进展将是充满希望和蓬勃发展的。我们将看到在未来一百年内，GW检测灵敏度在所有频带上提高几个数量级到几个数量级。
After giving a brief introduction and presenting a complete classification of gravitational waves (GWs) according to their frequencies, we review and summarize the detection methods, the sensitivities, and the sources. We notice that real-time detections are possible above 300 pHz. Below 300 pHz, the detections are possible on GW imprints or indirectly. We are on the verge of detection. The progress in this field will be promising and thriving. We will see improvement of a few orders to several orders of magnitude in the GW detection sensitivities over all frequency bands in the next hundred years.