Comparison of post-Newtonian mode amplitudes with numerical relativity simulations of binary black holes-Reference-Cited by-同舟云学术

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Comparison of post-Newtonian mode amplitudes with numerical relativity simulations of binary black holes

Published:2020-02-18 Issue:6 Volume:37 Page:065006
ISSN:0264-9381
Container-title:Classical and Quantum Gravity
language:
Short-container-title:Class. Quantum Grav.

Author:

Borhanian S^ORCID,Arun K G^ORCID,Pfeiffer H P^ORCID,Sathyaprakash B S^ORCID

Funder

Indo-US Science and Technology Forum through the Indo-US Centre for the Exploration of Extreme Gravity

National Science Foundation, USA

Publisher

IOP Publishing

Subject

Physics and Astronomy (miscellaneous)

Link

https://iopscience.iop.org/article/10.1088/1361-6382/ab6a21/pdf

Reference70 articles.

1. Observation of Gravitational Waves from a Binary Black Hole Merger

2. GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence

3. GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2

4. GW170608: Observation of a 19 Solar-mass Binary Black Hole Coalescence

5. GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence

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1. Erratum: Extracting linear and nonlinear quasinormal modes from black hole merger simulations [Phys. Rev. D 109 , 044069 (2024)];Physical Review D;2024-08-19

2. Post-Newtonian theory for gravitational waves;Living Reviews in Relativity;2024-07-10

3. Do black holes remember what they are made of?;Classical and Quantum Gravity;2024-06-25

4. Extracting linear and nonlinear quasinormal modes from black hole merger simulations;Physical Review D;2024-02-28

5. Bounds on tidal charges from gravitational wave ringdown observations;Physical Review D;2024-01-19

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