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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.

Item is

Basic (Discarded)

Date of Discard: 2020-11-24
Comment: Dublette
 Creators:
Borhanian, S.
Arun, K. G.
Pfeiffer, H.1           
Sathyaprakash, B. S.
Affiliations:
1Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_1933290              
 Dates: 2020
Files: 1 File
Locators: 0 Locators
version ID: item_3195223_2
Item State: Discarded
Name of Context: Publications of the Group Astrophysical and Cosmological Relativity, Affiliated to: MPI for Gravitational Physics