Exciting black hole modes via misaligned coalescences. II. The mode content of late-time coalescence waveforms

© 2019 American Physical Society. Using inspiral and plunge trajectories we construct with a generalized Ori-Thorne algorithm, we use a time-domain black hole perturbation theory code to compute the corresponding gravitational waves. The last cycles of these waveforms are a superposition of Kerr qua...

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Bibliographic Details
Main Authors: Lim, Halston, Khanna, Gaurav, Apte, Anuj, Hughes, Scott A
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:English
Published: American Physical Society (APS) 2021
Online Access:https://hdl.handle.net/1721.1/136507