Gravitational Wave Flux and Quadrupole Modes from Quasi-Circular Non-Spinning 
Compact Binaries to the Fourth Post-Newtonian Order

Blanchet, Luc; Faye, Guillaume; Henry, Quentin; Larrouturou, François; Trestini, David

doi:10.1103/PhysRevD.108.064041

Item

ITEM ACTIONSEXPORT

Add to Basket

Local TagsRelease HistoryDetailsSummary

Released

Journal Article

Gravitational Wave Flux and Quadrupole Modes from Quasi-Circular Non-Spinning Compact Binaries to the Fourth Post-Newtonian Order

MPS-Authors

/persons/resource/persons266528

Henry, Quentin
Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

External Resource

No external resources are shared

Fulltext (restricted access)

There are currently no full texts shared for your IP range.

Fulltext (public)

2304.11186.pdf
(Preprint), 600KB

PhysRevD.108.064041.pdf
(Publisher version), 635KB

Supplementary Material (public)

There is no public supplementary material available

Citation

Blanchet, L., Faye, G., Henry, Q., Larrouturou, F., & Trestini, D. (2023). Gravitational Wave Flux and Quadrupole Modes from Quasi-Circular Non-Spinning Compact Binaries to the Fourth Post-Newtonian Order. Physical Review D, 108(6): 064041. doi:10.1103/PhysRevD.108.064041.

Cite as: https://hdl.handle.net/21.11116/0000-000D-13DC-6

Abstract

This article provides the details on the technical derivation of the
gravitational waveform and total gravitational-wave energy flux of non-spinning
compact binary systems to the 4PN (fourth post-Newtonian) 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 "post-adiabatic" correction needed to evaluate the
tail integral with 2.5PN relative precision; (iv) we discuss the relation
between the binary's orbital frequency in quasi-circular 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.