{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:LQPCJE3YWTMSZUUQJDR7GNQTYT","short_pith_number":"pith:LQPCJE3Y","schema_version":"1.0","canonical_sha256":"5c1e249378b4d92cd29048e3f33613c4fefbccdb0da80b4d2652ff6757916ef4","source":{"kind":"arxiv","id":"2101.11028","version":2},"attestation_state":"computed","paper":{"title":"Outflow from super-Eddington flow: where it originates from and how much impact it gives?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Ken Ohsuga, Shin Mineshige, Takaaki Kitaki, Tomohisa Kawashima","submitted_at":"2021-01-26T19:00:40Z","abstract_excerpt":"It is widely believed that super-Eddington accretion flow can produce powerful outflow, but where it originates from and how much mass and energy are carried away to which directions? To answer to these questions, we newly perform a large-box, two-dimensional radiation hydrodynamic simulation, paying special attention lest the results should depend on adopted initial and boundary conditions. We could achieve a quasi-steady state in an unprecedentedly large range, $r=2~r_{\\rm S}$-$600~r_{\\rm S}$ (with $r_{\\rm S}$ being the Schwarzschild radius) from the black hole. The accretion rate onto the c"},"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":"2101.11028","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2021-01-26T19:00:40Z","cross_cats_sorted":[],"title_canon_sha256":"05f172bc1bd29812162aeb25d4155e6c3387c3c89f0266b00384c9138352d37d","abstract_canon_sha256":"a139a17df9dca977bdc43e221bfaf231d8adfcaa6147ba0a8242a0fd88d28878"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:11:26.257525Z","signature_b64":"x84buxlgfaqWrIe+1aPVdhRv6cYabYoFNW5dKukFqPCWwmspd/Ek7O4yeAtP0qDuBy54DlSFQvVrGU3jCizDAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5c1e249378b4d92cd29048e3f33613c4fefbccdb0da80b4d2652ff6757916ef4","last_reissued_at":"2026-07-05T02:11:26.257132Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:11:26.257132Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Outflow from super-Eddington flow: where it originates from and how much impact it gives?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Ken Ohsuga, Shin Mineshige, Takaaki Kitaki, Tomohisa Kawashima","submitted_at":"2021-01-26T19:00:40Z","abstract_excerpt":"It is widely believed that super-Eddington accretion flow can produce powerful outflow, but where it originates from and how much mass and energy are carried away to which directions? To answer to these questions, we newly perform a large-box, two-dimensional radiation hydrodynamic simulation, paying special attention lest the results should depend on adopted initial and boundary conditions. We could achieve a quasi-steady state in an unprecedentedly large range, $r=2~r_{\\rm S}$-$600~r_{\\rm S}$ (with $r_{\\rm S}$ being the Schwarzschild radius) from the black hole. The accretion rate onto the c"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2101.11028","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2101.11028/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":"2101.11028","created_at":"2026-07-05T02:11:26.257188+00:00"},{"alias_kind":"arxiv_version","alias_value":"2101.11028v2","created_at":"2026-07-05T02:11:26.257188+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2101.11028","created_at":"2026-07-05T02:11:26.257188+00:00"},{"alias_kind":"pith_short_12","alias_value":"LQPCJE3YWTMS","created_at":"2026-07-05T02:11:26.257188+00:00"},{"alias_kind":"pith_short_16","alias_value":"LQPCJE3YWTMSZUUQ","created_at":"2026-07-05T02:11:26.257188+00:00"},{"alias_kind":"pith_short_8","alias_value":"LQPCJE3Y","created_at":"2026-07-05T02:11:26.257188+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2509.03735","citing_title":"Effects of Bethe-Heitler pair production in ultraluminous X-ray sources","ref_index":17,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/LQPCJE3YWTMSZUUQJDR7GNQTYT","json":"https://pith.science/pith/LQPCJE3YWTMSZUUQJDR7GNQTYT.json","graph_json":"https://pith.science/api/pith-number/LQPCJE3YWTMSZUUQJDR7GNQTYT/graph.json","events_json":"https://pith.science/api/pith-number/LQPCJE3YWTMSZUUQJDR7GNQTYT/events.json","paper":"https://pith.science/paper/LQPCJE3Y"},"agent_actions":{"view_html":"https://pith.science/pith/LQPCJE3YWTMSZUUQJDR7GNQTYT","download_json":"https://pith.science/pith/LQPCJE3YWTMSZUUQJDR7GNQTYT.json","view_paper":"https://pith.science/paper/LQPCJE3Y","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2101.11028&json=true","fetch_graph":"https://pith.science/api/pith-number/LQPCJE3YWTMSZUUQJDR7GNQTYT/graph.json","fetch_events":"https://pith.science/api/pith-number/LQPCJE3YWTMSZUUQJDR7GNQTYT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LQPCJE3YWTMSZUUQJDR7GNQTYT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LQPCJE3YWTMSZUUQJDR7GNQTYT/action/storage_attestation","attest_author":"https://pith.science/pith/LQPCJE3YWTMSZUUQJDR7GNQTYT/action/author_attestation","sign_citation":"https://pith.science/pith/LQPCJE3YWTMSZUUQJDR7GNQTYT/action/citation_signature","submit_replication":"https://pith.science/pith/LQPCJE3YWTMSZUUQJDR7GNQTYT/action/replication_record"}},"created_at":"2026-07-05T02:11:26.257188+00:00","updated_at":"2026-07-05T02:11:26.257188+00:00"}