RIFT can recover the masses, spins, and orbital energy and angular momentum of simulated hyperbolic black hole encounters when paired with the TEOBResumSDALI waveform model.
Bursts of Gravitational Radiation from Active Galactic Nuclei and Globular Clusters
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Parameter estimation of gravitational waves from hyperbolic black hole encounters
RIFT can recover the masses, spins, and orbital energy and angular momentum of simulated hyperbolic black hole encounters when paired with the TEOBResumSDALI waveform model.