{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:AYOLZFOL476ERK6WMIBVPZ3JAB","short_pith_number":"pith:AYOLZFOL","schema_version":"1.0","canonical_sha256":"061cbc95cbe7fc48abd6620357e7690046694005e2ecd4f4cff55fe6d8c58353","source":{"kind":"arxiv","id":"1704.07864","version":2},"attestation_state":"computed","paper":{"title":"Radiation-driven turbulent accretion onto massive black holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"John H. Wise, Kwangho Park, Tamara Bogdanovi\\'c","submitted_at":"2017-04-25T19:00:00Z","abstract_excerpt":"Accretion of gas and interaction of matter and radiation are at the heart of many questions pertaining to black hole (BH) growth and coevolution of massive BHs and their host galaxies. To answer them it is critical to quantify how the ionizing radiation that emanates from the innermost regions of the BH accretion flow couples to the surrounding medium and how it regulates the BH fueling. In this work we use high resolution 3-dimensional (3D) radiation-hydrodynamic simulations with the code Enzo, equipped with adaptive ray tracing module Moray, to investigate radiation-regulated BH accretion of"},"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":"1704.07864","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-04-25T19:00:00Z","cross_cats_sorted":[],"title_canon_sha256":"54b9ebfd9928bc4467488b236674d09cba793fbb8a82c6ba2c564dbfd76ed986","abstract_canon_sha256":"53ec979fa66171df38cc1211277e9410bf937d4d3c9480dff0fd1ac58788869a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:33:50.148530Z","signature_b64":"Mq+w2Zkr/EO/tVj/Om89YWSKvTtoU6ltSuYLu99BrmZFa0I+rZUvve4S/lxOhPP7kOkag0Z+r/tabowQNLjLDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"061cbc95cbe7fc48abd6620357e7690046694005e2ecd4f4cff55fe6d8c58353","last_reissued_at":"2026-05-18T00:33:50.147928Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:33:50.147928Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Radiation-driven turbulent accretion onto massive black holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"John H. Wise, Kwangho Park, Tamara Bogdanovi\\'c","submitted_at":"2017-04-25T19:00:00Z","abstract_excerpt":"Accretion of gas and interaction of matter and radiation are at the heart of many questions pertaining to black hole (BH) growth and coevolution of massive BHs and their host galaxies. To answer them it is critical to quantify how the ionizing radiation that emanates from the innermost regions of the BH accretion flow couples to the surrounding medium and how it regulates the BH fueling. In this work we use high resolution 3-dimensional (3D) radiation-hydrodynamic simulations with the code Enzo, equipped with adaptive ray tracing module Moray, to investigate radiation-regulated BH accretion of"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1704.07864","kind":"arxiv","version":2},"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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1704.07864","created_at":"2026-05-18T00:33:50.148010+00:00"},{"alias_kind":"arxiv_version","alias_value":"1704.07864v2","created_at":"2026-05-18T00:33:50.148010+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1704.07864","created_at":"2026-05-18T00:33:50.148010+00:00"},{"alias_kind":"pith_short_12","alias_value":"AYOLZFOL476E","created_at":"2026-05-18T12:31:08.081275+00:00"},{"alias_kind":"pith_short_16","alias_value":"AYOLZFOL476ERK6W","created_at":"2026-05-18T12:31:08.081275+00:00"},{"alias_kind":"pith_short_8","alias_value":"AYOLZFOL","created_at":"2026-05-18T12:31:08.081275+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/AYOLZFOL476ERK6WMIBVPZ3JAB","json":"https://pith.science/pith/AYOLZFOL476ERK6WMIBVPZ3JAB.json","graph_json":"https://pith.science/api/pith-number/AYOLZFOL476ERK6WMIBVPZ3JAB/graph.json","events_json":"https://pith.science/api/pith-number/AYOLZFOL476ERK6WMIBVPZ3JAB/events.json","paper":"https://pith.science/paper/AYOLZFOL"},"agent_actions":{"view_html":"https://pith.science/pith/AYOLZFOL476ERK6WMIBVPZ3JAB","download_json":"https://pith.science/pith/AYOLZFOL476ERK6WMIBVPZ3JAB.json","view_paper":"https://pith.science/paper/AYOLZFOL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1704.07864&json=true","fetch_graph":"https://pith.science/api/pith-number/AYOLZFOL476ERK6WMIBVPZ3JAB/graph.json","fetch_events":"https://pith.science/api/pith-number/AYOLZFOL476ERK6WMIBVPZ3JAB/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AYOLZFOL476ERK6WMIBVPZ3JAB/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AYOLZFOL476ERK6WMIBVPZ3JAB/action/storage_attestation","attest_author":"https://pith.science/pith/AYOLZFOL476ERK6WMIBVPZ3JAB/action/author_attestation","sign_citation":"https://pith.science/pith/AYOLZFOL476ERK6WMIBVPZ3JAB/action/citation_signature","submit_replication":"https://pith.science/pith/AYOLZFOL476ERK6WMIBVPZ3JAB/action/replication_record"}},"created_at":"2026-05-18T00:33:50.148010+00:00","updated_at":"2026-05-18T00:33:50.148010+00:00"}