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Preprint | PUBDB-2023-01454 |
; ; ; ;
2023
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Please use a persistent id in citations: doi:10.3204/PUBDB-2023-01454
Report No.: DESY-23-044; arXiv:2304.11186
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.
Keyword(s): binary, compact ; energy, flux ; gravitational radiation, energy ; regularization, dimensional ; gravitational radiation, frequency ; gravitational radiation, flux ; multipole ; commutation relations ; infrared ; orbit ; Einstein
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Journal Article
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 (2023) [10.1103/PhysRevD.108.064041]
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