Gravitational-wave flux and quadrupole modes from quasicircular nonspinning compact binaries to the fourth post-Newtonian order
Gravitational-wave flux and quadrupole modes from quasicircular nonspinning compact binaries to the fourth post-Newtonian order
This article provides the details on the technical derivation of the gravitational waveform and total gravitational-wave energy flux of nonspinning compact binary systems to the fourth post-Newtonian (4PN) order beyond the Einstein quadrupole formula. In particular: (i) we overview the link between the radiative multipole moments measured at infinity and the source moments in the framework of dimensional regularization; (ii) we compute special corrections to the source moments due to "infrared"commutators arising at the 4PN order; (iii) we derive a "postadiabatic"correction needed to evaluate the tail integral with 2.5PN relative precision; (iv) we discuss the relation between the binary's orbital frequency in quasicircular orbit and the gravitational-wave frequency measured at infinity; (v) we compute the hereditary effects at the 4PN order, including those coming from the recently derived tails-of-memory; and (vi) we describe the various tests we have performed to ensure the correctness of the results. Those results are collected in an ancillary file.
Blanchet, Luc
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Faye, Guillaume
462a7e27-ec6a-45d3-aaa7-37a2af14c0ae
Henry, Quentin
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Larrouturou, François
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Trestini, David
f72ecc41-21fa-453b-8209-01a7ab746b89
21 September 2023
Blanchet, Luc
d208bbd8-6eb0-4da8-adb2-e5e46afd2596
Faye, Guillaume
462a7e27-ec6a-45d3-aaa7-37a2af14c0ae
Henry, Quentin
15b9765f-56c6-40bd-8d4d-83af45c7f58d
Larrouturou, François
251e9719-46ea-42e7-a007-27a2cb15302a
Trestini, David
f72ecc41-21fa-453b-8209-01a7ab746b89
Blanchet, Luc, Faye, Guillaume, Henry, Quentin, Larrouturou, François and Trestini, David
(2023)
Gravitational-wave flux and quadrupole modes from quasicircular nonspinning compact binaries to the fourth post-Newtonian order.
Physical Review D, 108 (6), [064041].
(doi:10.1103/PhysRevD.108.064041).
Abstract
This article provides the details on the technical derivation of the gravitational waveform and total gravitational-wave energy flux of nonspinning compact binary systems to the fourth post-Newtonian (4PN) order beyond the Einstein quadrupole formula. In particular: (i) we overview the link between the radiative multipole moments measured at infinity and the source moments in the framework of dimensional regularization; (ii) we compute special corrections to the source moments due to "infrared"commutators arising at the 4PN order; (iii) we derive a "postadiabatic"correction needed to evaluate the tail integral with 2.5PN relative precision; (iv) we discuss the relation between the binary's orbital frequency in quasicircular orbit and the gravitational-wave frequency measured at infinity; (v) we compute the hereditary effects at the 4PN order, including those coming from the recently derived tails-of-memory; and (vi) we describe the various tests we have performed to ensure the correctness of the results. Those results are collected in an ancillary file.
Text
PhysRevD.108.064041
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Published date: 21 September 2023
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© 2023 authors. Published by the American Physical Society. Published by the American Physical Society under the terms of the "https://creativecommons.org/licenses/by/4.0/"Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article's title, journal citation, and DOI. Open access publication funded by the Max Planck Society.
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Local EPrints ID: 506876
URI: http://eprints.soton.ac.uk/id/eprint/506876
ISSN: 2470-0010
PURE UUID: 4d840255-3ec5-4829-abc5-18e6d772731b
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Date deposited: 19 Nov 2025 17:43
Last modified: 20 Nov 2025 03:08
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Author:
Luc Blanchet
Author:
Guillaume Faye
Author:
Quentin Henry
Author:
François Larrouturou
Author:
David Trestini
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