The status of black-hole binary merger simulations with numerical relativity

DOI10.1088/0264-9381/28/13/134001zbMath1219.83048arXiv1012.2872OpenAlexW2064461074MaRDI QIDQ3086983

Sean T. McWilliams

Publication date: 1 August 2011

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

Full work available at URL: https://arxiv.org/abs/1012.2872

Mathematics Subject Classification ID

Black holes (83C57) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Research exposition (monographs, survey articles) pertaining to relativity and gravitational theory (83-02) Galactic and stellar structure (85A15) 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) Einstein-Maxwell equations (83C22)

Related Items (2)

The overlap of numerical relativity, perturbation theory and post-Newtonian theory in the binary black hole problem ⋮ Improvements to the construction of binary black hole initial data

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