Gravitational Radiation for Extreme Mass Ratio Inspirals to the 14th Post-Newtonian Order
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Publication:2911570
DOI10.1143/PTP.127.583zbMath1250.83026arXiv1104.5615MaRDI QIDQ2911570
Publication date: 31 August 2012
Published in: Progress of Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1104.5615
Black holes (83C57) 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)
Analytical effective one-body formalism for extreme-mass-ratio inspirals with eccentric orbits ⋮ Gravitational-wave tail effects to quartic non-linear 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 ⋮ Analytic approximations in GR and gravitational waves ⋮ The General Relativistic Two Body Problem and the Effective One Body Formalism
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