The third and a half-post-Newtonian gravitational wave quadrupole mode for quasi-circular inspiralling compact binaries

DOI10.1088/0264-9381/29/17/175004zbMath1251.83012arXiv1204.1043OpenAlexW2128132769MaRDI QIDQ3167787

Sylvain Marsat, Luc Blanchet, Guillaume Faye, Bala R. Iyer

Publication date: 29 October 2012

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

Full work available at URL: https://arxiv.org/abs/1204.1043

Mathematics Subject Classification ID

Celestial mechanics (70F15) 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 (12)

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 ⋮ Gravitational waves in scalar-tensor theory to one-and-a-half post-Newtonian order ⋮ Parametrizing gravitational-wave polarizations ⋮ The quadrupole moment of compact binaries to the fourth post-Newtonian order: from source to canonical moment ⋮ Least square ellipsoid fitting using iterative orthogonal transformations ⋮ Magnetic effects on the generation of gravitational waves in a black hole-neutron star binary system ⋮ 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 ⋮ The overlap of numerical relativity, perturbation theory and post-Newtonian theory in the binary black hole problem ⋮ Gravitational radiation from post-Newtonian sources and inspiralling compact binaries ⋮ The General Relativistic Two Body Problem and the Effective One Body Formalism

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