{"paper":{"title":"Stable characteristic evolution of generic 3-dimensional single-black-hole spacetimes","license":"","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"A.Abrahams, A.Anderson, A.Teukolsky, B.Szilagyi, C.Evans, D.Shoemaker, E.Seidel, F.Saied, G.Cook, G.Fox, J.Lenaghan, J.Masso, J.Winicour, J.W.York, K.Camarda, L.Finn, L.Kidder, L.Lehner, L.Rezzolla, L.Smarr, M.Choptuik, M.H.P.M.van Putten, M.Huq, M.Parashar, M.Rupright, M.Scheel, N.Bishop, P.Anninos, P.Laguna, P.Papadopoulos, P.Saylor, P.Walker, R.A.Matzner, R.Correl, R. Marsa, S.Brandt J.Browne, S.Klasky, S.Mitra, S.Shapiro, T.Baumgarte, T.Haupt, The Binary Black Hole Grand Challenge Alliance: R.Gomez, W.Landry","submitted_at":"1998-01-20T22:07:31Z","abstract_excerpt":"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."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"gr-qc/9801069","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}