Next-to-leading tail-induced spin–orbit effects in the gravitational radiation flux of compact binaries

DOI10.1088/0264-9381/31/2/025023zbMath1292.83020arXiv1307.6793OpenAlexW2062247415MaRDI QIDQ5412866

Sylvain Marsat, Luc Blanchet, Alejandro Bohé, Alessandra Buonanno

Publication date: 28 April 2014

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

Full work available at URL: https://arxiv.org/abs/1307.6793

zbMATH Keywords

gravitational wavespost-Newtoniancompact binariesspin-orbitgravitational radiation fluxtail-effect

Mathematics Subject Classification ID

Black holes (83C57) Gravitational energy and conservation laws; groups of motions (83C40) Observational and experimental questions in relativity and gravitational theory (83B05) Galactic and stellar dynamics (85A05) Equations of motion in general relativity and gravitational theory (83C10) Gravitational waves (83C35)

Related Items (4)

Analytical effective one-body formalism for extreme-mass-ratio inspirals with eccentric orbits ⋮ Analytic approximations, perturbation theory, effective field theory methods and their applications ⋮ 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

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