The close-limit approximation for black hole binaries with post-Newtonian initial conditions

DOI10.1088/0264-9381/27/4/045008zbMath1186.83017arXiv0910.4593OpenAlexW2145637610MaRDI QIDQ5305373

Alexandre Le Tiec, Luc Blanchet

Publication date: 22 March 2010

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

Full work available at URL: https://arxiv.org/abs/0910.4593

Mathematics Subject Classification ID

Black holes (83C57) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Equations of motion in general relativity and gravitational theory (83C10) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)

Related Items (3)

Applications of the close-limit approximation: horizonless compact objects and scalar fields ⋮ 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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