Gopakumar, Achamveedu, Hannam, Mark ORCID: https://orcid.org/0000-0001-5571-325X, Husa, Sascha and Brügmann, Bernd 2008. Comparison between numerical relativity and a new class of post-Newtonian gravitational-wave phase evolutions: The nonspinning equal-mass case. Physical Review D 78 (6) , 064026. 10.1103/PhysRevD.78.064026 |
Official URL: http://dx.doi.org/10.1103/PhysRevD.78.064026
Abstract
We compare the phase evolution of equal-mass nonspinning black-hole binaries from numerical relativity (NR) simulations with post-Newtonian (PN) results obtained from three PN approximants: the TaylorT1 and T4 approximants, for which NR-PN comparisons have already been performed in the literature, and the recently proposed approximant TaylorEt. The accumulated phase disagreement between NR and PN results over the frequency range Mω=0.0455 to Mω=0.1 is greater for TaylorEt than either T1 or T4, but has the attractive property of decreasing monotonically as the PN order is increased.
Item Type: | Article |
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Date Type: | Publication |
Status: | Published |
Schools: | Physics and Astronomy |
Subjects: | Q Science > QB Astronomy |
Publisher: | American Physical Society |
ISSN: | 1550-7998 |
Last Modified: | 20 Oct 2022 08:18 |
URI: | https://orca.cardiff.ac.uk/id/eprint/27872 |
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