11-orbit inspiral of a mass ratio 4:1 black-hole binary

DOI10.1088/0264-9381/28/13/134004zbMath1219.83069OpenAlexW2066385193MaRDI QIDQ3086985

Ulrich Sperhake, Doreen Müller, Carlos F. Sopuerta, Bernd Brügmann

Publication date: 1 August 2011

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

Full work available at URL: https://doi.org/10.1088/0264-9381/28/13/134004

Mathematics Subject Classification ID

Black holes (83C57) Equations of motion in general relativity and gravitational theory (83C10) Computational methods for problems pertaining to relativity and gravitational theory (83-08) Gravitational waves (83C35) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)

Related Items (3)

Numerical relativity: the role of black holes in gravitational wave physics, astrophysics and high-energy physics ⋮ The overlap of numerical relativity, perturbation theory and post-Newtonian theory in the binary black hole problem ⋮ Orbiting black-hole binaries and apparent horizons in higher dimensions

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