期刊
CLASSICAL AND QUANTUM GRAVITY
卷 19, 期 7, 页码 1267-1278出版社
IOP PUBLISHING LTD
DOI: 10.1088/0264-9381/19/7/305
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Binary black holes are the most promising candidate sources for the first generation of earth-based interferometric gravitational-wave detectors. We summarize and discuss the state-of-the-art analytical techniques developed during the last few years to better describe the late dynamical evolution of binary black holes of comparable masses.
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