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Stable characteristic evolution of generic 3-dimensional single-black-hole spacetimes

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arxiv gr-qc/9801069 v1 pith:EFU62GHS submitted 1998-01-20 gr-qc

The Binary Black Hole Grand Challenge Alliance: R.Gomez , L.Lehner , R. Marsa , J.Winicour , A.Abrahams , A.Anderson , P.Anninos , T.Baumgarte
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N.Bishop S.Brandt J.Browne K.Camarda M.Choptuik R.Correl G.Cook C.Evans L.Finn G.Fox T.Haupt M.Huq L.Kidder S.Klasky P.Laguna W.Landry J.Lenaghan J.Masso R.A.Matzner S.Mitra P.Papadopoulos M.Parashar L.Rezzolla M.Rupright F.Saied P.Saylor M.Scheel E.Seidel S.Shapiro D.Shoemaker L.Smarr B.Szilagyi A.Teukolsky M.H.P.M.van Putten P.Walker J.W.York
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keywords evolutioncharacteristicdimensionalgenericresultssingle-black-holespacetimesaccurate
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We report new results which establish that the accurate 3-dimensional numerical simulation of generic single-black-hole spacetimes has been achieved by characteristic evolution with unlimited long term stability. Our results cover a selection of distorted, moving and spinning single black holes, with evolution times up to 60,000M.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Towards long and accurate numerical relativity waveforms of binary black holes beyond general relativity

    gr-qc 2026-07 conditional novelty 6.5 of 10

    Spectral methods plus comoving fixing-the-equations drivers yield 40+ cycle equal-mass sGB binary waveforms with phase error ≲1 rad, distinguishable from GR and merging earlier.

  2. Conformal compactification and affine-null metric formulation of the Einstein equations

    gr-qc 2025-04 conditional novelty 6.0 of 10

    A hierarchical, boundary-regular affine-null form of the conformal Einstein-scalar equations is derived, shown equivalent to compactified physical-space equations, and used to extract the news function at null infinity.

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