Characteristic extraction in numerical relativity: binary black hole merger waveforms at null infinity

DOI10.1088/0264-9381/27/7/075014zbMath1187.83026arXiv0912.1285OpenAlexW2051442546MaRDI QIDQ3558428

Denis Pollney, Béla Szilágyi, Christian Reisswig, Nigel T. Bishop

Publication date: 5 May 2010

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

Full work available at URL: https://arxiv.org/abs/0912.1285

zbMATH Keywords

exact solutionsblack holesgravitational wavesEinstein's equations (general structure, canonical formalism, Cauchy problems)

Mathematics Subject Classification ID

Black holes (83C57) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Exact solutions to problems in general relativity and gravitational theory (83C15) 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)

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Extraction of gravitational waves in numerical relativity ⋮ Gravitational radiation by point particle eccentric binary systems in the linearised characteristic formulation of general relativity ⋮ General relativistic null-cone evolutions with a high-order scheme ⋮ Extraction of gravitational-wave energy in higher dimensional numerical relativity using the Weyl tensor ⋮ The gravitational wave strain in the characteristic formalism of numerical relativity ⋮ Spherical symmetry as a test case for unconstrained hyperboloidal evolution II: gauge conditions ⋮ Characteristic evolution and matching ⋮ AN INTRODUCTION TO WELL-POSEDNESS AND FREE-EVOLUTION ⋮ Continuum and discrete initial-boundary value problems and Einstein's field equations

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