{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:VUOIE3GDNPSJ6YGHDW7IEKHRJC","short_pith_number":"pith:VUOIE3GD","schema_version":"1.0","canonical_sha256":"ad1c826cc36be49f60c71dbe8228f148a2dedfcb9b72af2dac5d9b0e03335d95","source":{"kind":"arxiv","id":"2210.10053","version":3},"attestation_state":"computed","paper":{"title":"Nozzle Shocks, Disk Tearing and Streamers Drive Rapid Accretion in 3D GRMHD Simulations of Warped Thin Disks","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Alexander Tchekhovskoy, Gibwa Musoke, Jonatan Jacquemin-Ide, Matthew T.P. Liska, Nicholas Kaaz, Oliver Porth, Zachary L. Andalman","submitted_at":"2022-10-18T18:00:00Z","abstract_excerpt":"The angular momentum of gas feeding a black hole (BH) is typically misaligned with respect to the BH spin, resulting in a tilted accretion disk. Rotation of the BH drags the surrounding space-time, manifesting as Lense-Thirring torques that lead to disk precession and warping. We study these processes by simulating a thin ($H/r=0.02$), highly tilted ($\\mathcal{T}=65^\\circ$) accretion disk around a rapidly rotating ($a=0.9375$) BH at extremely high resolutions, which we performed using the general-relativistic magnetohydrodynamic (GRMHD) code H-AMR. The disk becomes significantly warped and con"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"2210.10053","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2022-10-18T18:00:00Z","cross_cats_sorted":[],"title_canon_sha256":"c64b8f94aeb927edc7812c11d3c0e23579574593308f55f41445d300e1f57c6c","abstract_canon_sha256":"e0ca4fdbd757c98144aacaded88aed61798f0e8476da09eebc91e241bcd0f4d4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:15:34.236011Z","signature_b64":"1npN5fxwvLHSX0p82iOnXm5LlouYKYhwBwh7AiKD2htI7fZ87+6oCLp0zKb7B9MJcA6AREkTHqKOCTt3MvPNDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ad1c826cc36be49f60c71dbe8228f148a2dedfcb9b72af2dac5d9b0e03335d95","last_reissued_at":"2026-07-05T08:15:34.235593Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:15:34.235593Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Nozzle Shocks, Disk Tearing and Streamers Drive Rapid Accretion in 3D GRMHD Simulations of Warped Thin Disks","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Alexander Tchekhovskoy, Gibwa Musoke, Jonatan Jacquemin-Ide, Matthew T.P. Liska, Nicholas Kaaz, Oliver Porth, Zachary L. Andalman","submitted_at":"2022-10-18T18:00:00Z","abstract_excerpt":"The angular momentum of gas feeding a black hole (BH) is typically misaligned with respect to the BH spin, resulting in a tilted accretion disk. Rotation of the BH drags the surrounding space-time, manifesting as Lense-Thirring torques that lead to disk precession and warping. We study these processes by simulating a thin ($H/r=0.02$), highly tilted ($\\mathcal{T}=65^\\circ$) accretion disk around a rapidly rotating ($a=0.9375$) BH at extremely high resolutions, which we performed using the general-relativistic magnetohydrodynamic (GRMHD) code H-AMR. The disk becomes significantly warped and con"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2210.10053","kind":"arxiv","version":3},"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/2210.10053/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"},"aliases":[{"alias_kind":"arxiv","alias_value":"2210.10053","created_at":"2026-07-05T08:15:34.235657+00:00"},{"alias_kind":"arxiv_version","alias_value":"2210.10053v3","created_at":"2026-07-05T08:15:34.235657+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2210.10053","created_at":"2026-07-05T08:15:34.235657+00:00"},{"alias_kind":"pith_short_12","alias_value":"VUOIE3GDNPSJ","created_at":"2026-07-05T08:15:34.235657+00:00"},{"alias_kind":"pith_short_16","alias_value":"VUOIE3GDNPSJ6YGH","created_at":"2026-07-05T08:15:34.235657+00:00"},{"alias_kind":"pith_short_8","alias_value":"VUOIE3GD","created_at":"2026-07-05T08:15:34.235657+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2601.02487","citing_title":"Thick Disks, Thin Hopes: Suppressed Capture and Merger Rates in AGN","ref_index":46,"is_internal_anchor":false},{"citing_arxiv_id":"2604.20499","citing_title":"Reshaping the inner shadow of a Kerr black hole by a torn accretion disk","ref_index":64,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/VUOIE3GDNPSJ6YGHDW7IEKHRJC","json":"https://pith.science/pith/VUOIE3GDNPSJ6YGHDW7IEKHRJC.json","graph_json":"https://pith.science/api/pith-number/VUOIE3GDNPSJ6YGHDW7IEKHRJC/graph.json","events_json":"https://pith.science/api/pith-number/VUOIE3GDNPSJ6YGHDW7IEKHRJC/events.json","paper":"https://pith.science/paper/VUOIE3GD"},"agent_actions":{"view_html":"https://pith.science/pith/VUOIE3GDNPSJ6YGHDW7IEKHRJC","download_json":"https://pith.science/pith/VUOIE3GDNPSJ6YGHDW7IEKHRJC.json","view_paper":"https://pith.science/paper/VUOIE3GD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2210.10053&json=true","fetch_graph":"https://pith.science/api/pith-number/VUOIE3GDNPSJ6YGHDW7IEKHRJC/graph.json","fetch_events":"https://pith.science/api/pith-number/VUOIE3GDNPSJ6YGHDW7IEKHRJC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VUOIE3GDNPSJ6YGHDW7IEKHRJC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VUOIE3GDNPSJ6YGHDW7IEKHRJC/action/storage_attestation","attest_author":"https://pith.science/pith/VUOIE3GDNPSJ6YGHDW7IEKHRJC/action/author_attestation","sign_citation":"https://pith.science/pith/VUOIE3GDNPSJ6YGHDW7IEKHRJC/action/citation_signature","submit_replication":"https://pith.science/pith/VUOIE3GDNPSJ6YGHDW7IEKHRJC/action/replication_record"}},"created_at":"2026-07-05T08:15:34.235657+00:00","updated_at":"2026-07-05T08:15:34.235657+00:00"}