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...
Main Authors: | , , , |
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Other Authors: | |
Format: | Article |
Language: | English |
Published: |
American Physical Society (APS)
2021
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Online Access: | https://hdl.handle.net/1721.1/136507 |