{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:IXVJ6HFUGNSPN5B3QVK4ZNGVZD","short_pith_number":"pith:IXVJ6HFU","schema_version":"1.0","canonical_sha256":"45ea9f1cb43364f6f43b8555ccb4d5c8f63c4096d7ea98d7eff71b5818afbf0e","source":{"kind":"arxiv","id":"1806.00691","version":1},"attestation_state":"computed","paper":{"title":"Radiation Transport Through Super-Eddington Stellar Winds","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Chris Fryer, Joyce A. Guzik, Stanley P. Owocki, Todd J. Urbatsch","submitted_at":"2018-06-02T19:09:08Z","abstract_excerpt":"We present results of simulations to assess the feasibility of modeling outflows from massive stars using the Los Alamos 3-D radiation hydrodynamics code Cassio developed for inertial confinement fusion (ICF) applications. We find that a 1-D stellar envelope simulation relaxes into hydrostatic equilibrium using computing resources that would make the simulation tractable in 2-D. We summarize next steps to include more physics fidelity and model the response to a large and abrupt energy deposition at the base of the envelope."},"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":"1806.00691","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2018-06-02T19:09:08Z","cross_cats_sorted":[],"title_canon_sha256":"b054a00fd16df9ad38a4bfefc1a114783562be69d5259d905669937b5ac2d30e","abstract_canon_sha256":"da97011f480078a55c887dc7392d3a17b80d63ecd7f434e942121b8b4bccd927"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:14:18.716399Z","signature_b64":"USTMTOz8phAKzAogKe/YgETLMwlyQjxuxeuiolqyURbGYX7WLHyZ51SZNcRWp0JTUejKwzCfz6KXHi2ey4HSCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"45ea9f1cb43364f6f43b8555ccb4d5c8f63c4096d7ea98d7eff71b5818afbf0e","last_reissued_at":"2026-05-18T00:14:18.715867Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:14:18.715867Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Radiation Transport Through Super-Eddington Stellar Winds","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Chris Fryer, Joyce A. Guzik, Stanley P. Owocki, Todd J. Urbatsch","submitted_at":"2018-06-02T19:09:08Z","abstract_excerpt":"We present results of simulations to assess the feasibility of modeling outflows from massive stars using the Los Alamos 3-D radiation hydrodynamics code Cassio developed for inertial confinement fusion (ICF) applications. We find that a 1-D stellar envelope simulation relaxes into hydrostatic equilibrium using computing resources that would make the simulation tractable in 2-D. We summarize next steps to include more physics fidelity and model the response to a large and abrupt energy deposition at the base of the envelope."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1806.00691","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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1806.00691","created_at":"2026-05-18T00:14:18.715952+00:00"},{"alias_kind":"arxiv_version","alias_value":"1806.00691v1","created_at":"2026-05-18T00:14:18.715952+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1806.00691","created_at":"2026-05-18T00:14:18.715952+00:00"},{"alias_kind":"pith_short_12","alias_value":"IXVJ6HFUGNSP","created_at":"2026-05-18T12:32:31.084164+00:00"},{"alias_kind":"pith_short_16","alias_value":"IXVJ6HFUGNSPN5B3","created_at":"2026-05-18T12:32:31.084164+00:00"},{"alias_kind":"pith_short_8","alias_value":"IXVJ6HFU","created_at":"2026-05-18T12:32:31.084164+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/IXVJ6HFUGNSPN5B3QVK4ZNGVZD","json":"https://pith.science/pith/IXVJ6HFUGNSPN5B3QVK4ZNGVZD.json","graph_json":"https://pith.science/api/pith-number/IXVJ6HFUGNSPN5B3QVK4ZNGVZD/graph.json","events_json":"https://pith.science/api/pith-number/IXVJ6HFUGNSPN5B3QVK4ZNGVZD/events.json","paper":"https://pith.science/paper/IXVJ6HFU"},"agent_actions":{"view_html":"https://pith.science/pith/IXVJ6HFUGNSPN5B3QVK4ZNGVZD","download_json":"https://pith.science/pith/IXVJ6HFUGNSPN5B3QVK4ZNGVZD.json","view_paper":"https://pith.science/paper/IXVJ6HFU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1806.00691&json=true","fetch_graph":"https://pith.science/api/pith-number/IXVJ6HFUGNSPN5B3QVK4ZNGVZD/graph.json","fetch_events":"https://pith.science/api/pith-number/IXVJ6HFUGNSPN5B3QVK4ZNGVZD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IXVJ6HFUGNSPN5B3QVK4ZNGVZD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IXVJ6HFUGNSPN5B3QVK4ZNGVZD/action/storage_attestation","attest_author":"https://pith.science/pith/IXVJ6HFUGNSPN5B3QVK4ZNGVZD/action/author_attestation","sign_citation":"https://pith.science/pith/IXVJ6HFUGNSPN5B3QVK4ZNGVZD/action/citation_signature","submit_replication":"https://pith.science/pith/IXVJ6HFUGNSPN5B3QVK4ZNGVZD/action/replication_record"}},"created_at":"2026-05-18T00:14:18.715952+00:00","updated_at":"2026-05-18T00:14:18.715952+00:00"}