How to avoid artificial boundaries in the numerical calculation of black hole spacetimes

DOI10.1088/0264-9381/16/7/301zbMath0938.83016arXivgr-qc/9804065OpenAlexW2113806133MaRDI QIDQ4700011

Peter Hübner

Publication date: 18 November 1999

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

Full work available at URL: https://arxiv.org/abs/gr-qc/9804065

zbMATH Keywords

black holesconformal field equationsnumerical implementationasymptotically flat spacetimeshyperbolic first-order systemconformally rescaled Einstein equationfirst-order time evolution equations

Mathematics Subject Classification ID

Black holes (83C57) Computational methods for problems pertaining to relativity and gravitational theory (83-08) First-order hyperbolic systems (35L40)

Related Items (6)

Spectral methods for the spin-2 equation near the cylinder at spatial infinity ⋮ Local twistors and the conformal field equations ⋮ Numerical approaches to spacetime singularities ⋮ The Einstein-Vlasov system/kinetic theory ⋮ Conformal infinity ⋮ Conformal infinity

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