The General Relativistic Two Body Problem and the Effective One Body Formalism

DOI10.1007/978-3-319-06349-2_5zbMath1328.83006arXiv1212.3169OpenAlexW1759063409MaRDI QIDQ5260827

Thibault Damour

Publication date: 30 June 2015

Published in: General Relativity, Cosmology and Astrophysics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1212.3169

zbMATH Keywords

effective one body formalismgeneral relativistic two body problemgravitational self-force (GSF)gravitational wave (GW)

Mathematics Subject Classification ID

Black holes (83C57) Research exposition (monographs, survey articles) pertaining to relativity and gravitational theory (83-02) Equations of motion in general relativity and gravitational theory (83C10) Gravitational waves (83C35)

Related Items (4)

The overlap of numerical relativity, perturbation theory and post-Newtonian theory in the binary black hole problem ⋮ Interpreting binary neutron star mergers: describing the binary neutron star dynamics, modelling gravitational waveforms, and analyzing detections ⋮ Scattering of two spinning black holes in post-Minkowskian gravity, to all orders in spin, and effective-one-body mappings ⋮ The SAGEX review on scattering amplitudes Chapter 13: Post-Minkowskian expansion from scattering amplitudes

Cites Work

• Unnamed Item
• Unnamed Item
• Unnamed Item
• Analytic black hole perturbation approach to gravitational radiation
• Generation of Post-Newtonian Gravitational Radiation via Direct Integration of the Relaxed Einstein Equations
• Gravitational Radiation for Extreme Mass Ratio Inspirals to the 14th Post-Newtonian Order
• The Effective One-Body Description of the Two-Body Problem
• Maximum Kick from Nonspinning Black-Hole Binary Inspiral
• The third and a half-post-Newtonian gravitational wave quadrupole mode for quasi-circular inspiralling compact binaries
• 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
• Tensor-multi-scalar theories of gravitation
• Quadrupole-quadrupole gravitational waves
• Gravitational-wave tails of tails
• Colliding black holes: The close limit
• Gravitational radiation reaction in the equations of motion of compact binaries to 3.5 post-Newtonian order
• Binary black hole merger in the extreme-mass-ratio limit
• Gravitational radiation from post-Newtonian sources and inspiralling compact binaries
• Dimensional regularization of the gravitational interaction of point masses

This page was built for publication: The General Relativistic Two Body Problem and the Effective One Body Formalism