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Robust evolution system for Numerical Relativity

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arxiv gr-qc/9902053 v2 pith:HQXMGWFP submitted 1999-02-18 gr-qc

classification gr-qc
keywords numericalevolutionblackholerelativityrobustallowapplied
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The paper combines theoretical and applied ideas which have been previously considered separately into a single set of evolution equations for Numerical Relativity. New numerical ingredients are presented which avoid gauge pathologies and allow one to perform robust 3D calculations. The potential of the resulting numerical code is demonstrated by using the Schwarzschild black hole as a test-bed. Its evolution can be followed up to times greater than one hundred black hole masses.

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Cited by 1 Pith paper

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  1. Proca stars in excited states

    gr-qc 2024-11 conditional novelty 6.0 of 10

    Excited Proca stars are always unstable: under perturbations they collapse, disperse, or migrate to the ground state, with migration possible only for a narrow set of negative-binding-energy configurations.

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