Fast frequency-domain waveforms for spin-precessing binary inspirals
Fast frequency-domain waveforms for spin-precessing binary inspirals
The detection and characterization of gravitational wave signals from compact binary coalescence events relies on accurate waveform templates in the frequency domain. The stationary phase approximation (SPA) can be used to compute closed-form frequency-domain waveforms for nonprecessing, quasicircular binary inspirals. However, until now, no fast frequency-domain waveforms have existed for …