High-Accuracy Comparison Between the Post-Newtonian and Self-Force Dynamics of Black-Hole Binaries

DOI10.1007/978-90-481-3015-3_15zbMath1213.83083arXiv1007.2614OpenAlexW3121331405MaRDI QIDQ2999509

Steven Detweiler, Luc Blanchet, Alexandre Le Tiec, Bernard F. Whiting

Publication date: 13 May 2011

Published in: Mass and Motion in General Relativity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1007.2614

Mathematics Subject Classification ID

Black holes (83C57) Gravitational energy and conservation laws; groups of motions (83C40) Equations of motion in general relativity and gravitational theory (83C10) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)

Related Items (5)

High-Order Post-Newtonian Contributions to Gravitational Self-force Effects in Black Hole Spacetimes ⋮ Analytic approximations, perturbation theory, effective field theory methods and their applications ⋮ Multipolar particles in helically symmetric spacetimes ⋮ The motion of point particles in curved spacetime ⋮ The radial action from probe amplitudes to all orders

Cites Work

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• The third post-Newtonian gravitational wave polarizations and associated spherical harmonic modes for inspiralling compact binaries in quasi-circular orbits
• Gravitational self-force in extreme mass-ratio inspirals
• Radiative gravitational fields in general relativity I. General structure of the field outside the source
• Gravitational waveforms from inspiralling compact binaries to second-post-Newtonian order
• Perspective on gravitational self-force analyses
• A rigorous derivation of gravitational self-force
• Dimensional regularization of the gravitational interaction of point masses

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