{"paper":{"title":"Influence of self-gravity on the runaway instability of black hole-torus systems","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"gr-qc","authors_text":"Jose A. Font, Masaru Shibata, Pedro J. Montero","submitted_at":"2010-04-19T06:22:47Z","abstract_excerpt":"Results   from  the   first  fully   general   relativistic  numerical simulations  in  axisymmetry  of  a  system formed  by  a  black  hole surrounded by  a self-gravitating torus in  equilibrium are presented, aiming to assess the influence  of the torus self-gravity on the onset of the  runaway instability. We  consider several models  with varying torus-to-black  hole  mass  ratio  and angular  momentum  distribution orbiting in equilibrium around a non-rotating black hole. The tori are perturbed  to induce  the mass  transfer towards  the black  hole. Our numerical simulations show that "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1004.3102","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/1004.3102/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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"}