Numerical relativity waveform surrogate model for generically precessing binary black hole mergers

A generic, noneccentric binary black hole (BBH) system emits gravitational waves (GWs) that are completely described by seven intrinsic parameters: the black hole spin vectors and the ratio of their masses. Simulating a BBH coalescence by solving Einstein’s equations numerically is computationally e...

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Veröffentlicht in:	Physical review. D 2017-07, Vol.96 (2), Article 024058
Hauptverfasser:	Blackman, Jonathan, Field, Scott E., Scheel, Mark A., Galley, Chad R., Ott, Christian D., Boyle, Michael, Kidder, Lawrence E., Pfeiffer, Harald P., Szilágyi, Béla
Format:	Artikel
Sprache:	eng
Schlagworte:	Black holes Coalescing Computer simulation Gravitational waves Mass ratios Mathematical models Numerical relativity Parameters Relativity Theory of relativity Waveforms
Online-Zugang:	Volltext
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