Non-linear multipole interactions and gravitational-wave octupole modes for inspiralling compact binaries to third-and-a-half post-Newtonian order

DOI10.1088/0264-9381/32/4/045016zbMath1308.83089arXiv1409.3546OpenAlexW2069389772MaRDI QIDQ4982308

Luc Blanchet, Guillaume Faye, Bala R. Iyer

Publication date: 24 March 2015

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1409.3546

zbMATH Keywords

black holes gravitational waves neutron stars post-Newtonian approximation pertubation theory related approximations

Mathematics Subject Classification ID

Black holes (83C57) Galactic and stellar structure (85A15) Galactic and stellar dynamics (85A05) Equations of motion in general relativity and gravitational theory (83C10) Gravitational waves (83C35) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)

Related Items (9)

The Poincaré and BMS flux-balance laws with application to binary systems ⋮ The quadrupole moment of compact binaries to the fourth post-Newtonian order: I. Non-locality in time and infra-red divergencies ⋮ The quadrupole moment of compact binaries to the fourth post-Newtonian order: II. Dimensional regularization and renormalization ⋮ The quadrupole moment of compact binaries to the fourth post-Newtonian order: from source to canonical moment ⋮ The mass quadrupole moment of compact binary systems at the fourth post-Newtonian order ⋮ The current-type quadrupole moment and gravitational-wave mode (ℓ, m) = (2, 1) of compact binary systems at the third post-Newtonian order ⋮ Gravitational radiation from post-Newtonian sources and inspiralling compact binaries ⋮ Multipole expansion of gravitational waves: from harmonic to Bondi coordinates ⋮ The quadrupole moment of compact binaries to the fourth post-Newtonian order: relating the harmonic and radiative metrics

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