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

Borhanian, S., Arun, K. G., Pfeiffer, H., & Sathyaprakash, B. S. (2020). Comparison of post-Newtonian mode amplitudes with numerical relativity simulations of binary black holes. Classical and Quantum Gravity, 37(6): 065006. doi:10.1088/1361-6382/ab6a21.

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Item Permalink: http://hdl.handle.net/21.11116/0000-0005-B76C-4 Version Permalink: http://hdl.handle.net/21.11116/0000-0005-B76D-3
Genre: Journal Article

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Borhanian_2020_Class._Quantum_Grav._37_065006.pdf (Publisher version), 3MB
 
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 Creators:
Borhanian, S., Author
Arun, K. G., Author
Pfeiffer, H.1, Author              
Sathyaprakash, B. S., Author
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1Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_1933290              

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 Dates: 2020
 Publication Status: Published in print
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 Identifiers: DOI: 10.1088/1361-6382/ab6a21
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Title: Classical and Quantum Gravity
Source Genre: Journal
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Pages: - Volume / Issue: 37 (6) Sequence Number: 065006 Start / End Page: - Identifier: -