Motion and gravitational wave forms of eccentric compact binaries with orbital-angular-momentum-aligned spins under next-to-leading order in spin–orbit and leading order in spin(1)–spin(2) and spin-squared couplings

DOI10.1088/0264-9381/27/16/165005zbMath1195.83019arXiv1003.2735OpenAlexW2070932520MaRDI QIDQ3586316

Johannes Hartung, Manuel Tessmer, Gerhard Schäfer

Publication date: 6 September 2010

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

Full work available at URL: https://arxiv.org/abs/1003.2735

zbMATH Keywords

equations of motion gravitational waves

Mathematics Subject Classification ID

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 (6)

Next‐to‐next‐to‐leading order post‐Newtonian linear‐in‐spin binary Hamiltonians ⋮ The quasi-Keplerian motion in regular Bardeen spacetime ⋮ General relativistic spin-orbit and spin-spin effects on the motion of rotating particles in an external gravitational field ⋮ Full-analytic frequency-domain gravitational wave forms from eccentric compact binaries to 2PN accuracy ⋮ Quasi-Keplerian motion under the generally parameterized post-Newtonian force ⋮ Post-Keplerian motion in Reissner-Nordström spacetime

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