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  5. Hybrid post-Newtonian effective-one-body scheme for spin-precessing compact-binary waveforms up to merger
 
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Hybrid post-Newtonian effective-one-body scheme for spin-precessing compact-binary waveforms up to merger

Author(s)
Akcay, Sarp  
Gamba, Rossella  
Bernuzzi, Sebastiano  
Uri
http://hdl.handle.net/10197/25973
Date Issued
2021-01-15
Date Available
2024-05-20T15:08:29Z
Abstract
We introduce TEOBResumSP: an efficient yet accurate hybrid scheme for generating gravitational waveforms from spin-precessing compact binaries. The precessing waveforms are generated via the established technique of Euler rotating aligned-spin (nonprecessing) waveforms from a precessing frame to an inertial frame. We employ the effective-one-body approximant TEOBResumS to generate the aligned-spin waveforms. We obtain the Euler angles by solving the post-Newtonian precession equations expanded to (next−to) 4 leading (second post-Newtonian) order. Current version of TEOBResumSP produces precessing waveforms through the inspiral phase up to the onset of the merger. We compare TEOBResumSP to current state-of-the-art precessing approximants NRSur7dq4, SEOBNRv4PHM, and IMRPhenomPv3HM in terms of frequency-domain matches of the ℓ=2 gravitational-wave strain for 200 cases of precessing compact binary inspirals with orbital inclinations up to 90 degrees, mass ratios up to four, and the effective precession parameter χp up to 0.75. We further provide an extended comparison with SEOBNRv4PHM involving 1030 more inspirals with χp ranging up to one and mass ratios up to 10. We find that 91% of the TEOBResumSP-NRSur7dq4 matches, 85% of the TEOBResumSP SEOBNRv4PHM matches, and 77% of the TEOBResumSP-IMRPhenomPv3HM matches are greater than 0.965. Most of the significant disagreements occur for large mass ratios and χp≳0.6. We identify the mismatch of the non-precessing (2,1) mode as one of the leading causes of disagreements. We also introduce a new parameter, χ⊥, max, to measure the strength of precession and hint that the strain mismatch between the above waveform approximants shows an exponential dependence on χ⊥,max though this requires further study. Our results indicate that TEOBResumSP is on its way to becoming a robust precessing approximant to be employed in the parameter estimation of generic-spin compact binaries.
Sponsorship
Irish Research Council
University College Dublin
Type of Material
Journal Article
Publisher
American Physical Society
Journal
Physical Review D
Volume
103
Issue
2
Copyright (Published Version)
2021 American Physical Society
Subjects

General relativity

Gravitational wave de...

Gravitational wave so...

Gravitational waves

DOI
10.1103/physrevd.103.024014
Language
English
Status of Item
Peer reviewed
ISSN
2470-0010
This item is made available under a Creative Commons License
https://creativecommons.org/licenses/by-nc-nd/3.0/ie/
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2005.05338v3.pdf

Size

2.26 MB

Format

Adobe PDF

Checksum (MD5)

9a9e85de77e551cf2e88fb04110b10ab

Owning collection
Mathematics and Statistics Research Collection

Item descriptive metadata is released under a CC-0 (public domain) license: https://creativecommons.org/public-domain/cc0/.
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