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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

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

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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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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    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.