General-relativistic precession in a black-hole binary

Author:

Hannam MarkORCID,Hoy Charlie,Thompson Jonathan E.,Fairhurst StephenORCID,Raymond Vivien,Colleoni Marta,Davis Derek,Estellés Héctor,Haster Carl-Johan,Helmling-Cornell Adrian,Husa Sascha,Keitel David,Massinger T. J.,Menéndez-Vázquez Alexis,Mogushi Kentaro,Ossokine Serguei,Payne Ethan,Pratten Geraint,Romero-Shaw Isobel,Sadiq Jam,Schmidt Patricia,Tenorio Rodrigo,Udall Richard,Veitch John,Williams Daniel,Yelikar Anjali Balasaheb,Zimmerman Aaron

Publisher

Springer Science and Business Media LLC

Subject

Multidisciplinary

Reference68 articles.

1. Farr, W. M. et al. Distinguishing spin-aligned and isotropic black hole populations with gravitational waves. Nature 548, 426–429 (2017).

2. Abbott, R. et al. The population of merging compact binaries inferred using gravitational waves through GWTC-3. Preprint at https://arxiv.org/abs/2111.03634 (2021).

3. Abbott, R. GW190412: observation of a binary-black-hole coalescence with asymmetric masses. Phys. Rev. D 102, 043015 (2020).

4. Abbott, R. Properties and astrophysical implications of the 150 M⊙ binary black hole merger GW190521. Astrophys. J. Lett. 900, L13 (2020).

5. Abbott, R. et al. GWTC-3: compact binary coalescences observed by LIGO and Virgo during the second part of the third observing run. Preprint at https://arxiv.org/abs/2111.03606 (2021).

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