Analytical Black-Hole Binary Merger Waveforms

We present a highly accurate, fully analytical model for the late inspiral, merger, and ringdown of black-hole binaries with arbitrary mass ratios and spin vectors and the associated gravitational radiation, including the contributions of harmonics beyond the fundamental mode. This model assumes onl...

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Veröffentlicht in:	Physical review letters 2019-05, Vol.122 (19), p.191102-191102, Article 191102
1. Verfasser:	McWilliams, Sean T
Format:	Artikel
Sprache:	eng
Schlagworte:	Black holes Circular orbits Coalescing Mass ratios Mathematical models Model accuracy Numerical relativity Orbital stability Parameters Perturbation Relativity Spacetime Theory of relativity Waveforms
Online-Zugang:	Volltext
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