{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:6HRDQGJUS2P5CQ2GWGLGOR2JK3","short_pith_number":"pith:6HRDQGJU","schema_version":"1.0","canonical_sha256":"f1e2381934969fd14346b19667474956e7098e0f8de76b0e541a46ec2d77a0d8","source":{"kind":"arxiv","id":"2301.10785","version":2},"attestation_state":"computed","paper":{"title":"Roles of fast neutrino-flavor conversion on the neutrino-heating mechanism of core-collapse supernova","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph","nucl-th"],"primary_cat":"astro-ph.HE","authors_text":"Hiroki Nagakura","submitted_at":"2023-01-25T19:00:04Z","abstract_excerpt":"One of the greatest uncertainties in any modeling of inner engine of core-collapse supernova (CCSN) is neutrino flavor conversions driven by neutrino self-interactions. We carry out large-scale numerical simulations of multi-energy, multi-angle, three-flavor framework, and general relativistic quantum kinetic neutrino transport in spherical symmetry with an essential set of neutrino-matter interactions under a realistic fluid profile of CCSN. Our result suggests that the neutrino heating in the gain region is reduced by $\\sim 40\\%$ due to fast neutrino-flavor conversion (FFC). We also find tha"},"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":"2301.10785","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2023-01-25T19:00:04Z","cross_cats_sorted":["gr-qc","hep-ph","nucl-th"],"title_canon_sha256":"8436ffae38833d31a2690e450f05f862da797fb4c73a8e36a9565ddcf850daf5","abstract_canon_sha256":"344d35bd0fb0dd94c8da418b3b2770a3965feb53aab6d1f20e72ea592a47376a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:18:10.516274Z","signature_b64":"Q8L+DG+kC9LpsR7UemQ9VIC3DUaXJWkmnd+m7/15CKxBhZJc8FQfmWUGoOjQgZQQGGU+C3KGtAvVecA4ylaaBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f1e2381934969fd14346b19667474956e7098e0f8de76b0e541a46ec2d77a0d8","last_reissued_at":"2026-07-05T06:18:10.515840Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:18:10.515840Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Roles of fast neutrino-flavor conversion on the neutrino-heating mechanism of core-collapse supernova","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph","nucl-th"],"primary_cat":"astro-ph.HE","authors_text":"Hiroki Nagakura","submitted_at":"2023-01-25T19:00:04Z","abstract_excerpt":"One of the greatest uncertainties in any modeling of inner engine of core-collapse supernova (CCSN) is neutrino flavor conversions driven by neutrino self-interactions. We carry out large-scale numerical simulations of multi-energy, multi-angle, three-flavor framework, and general relativistic quantum kinetic neutrino transport in spherical symmetry with an essential set of neutrino-matter interactions under a realistic fluid profile of CCSN. Our result suggests that the neutrino heating in the gain region is reduced by $\\sim 40\\%$ due to fast neutrino-flavor conversion (FFC). We also find tha"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2301.10785","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/2301.10785/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":"2301.10785","created_at":"2026-07-05T06:18:10.515889+00:00"},{"alias_kind":"arxiv_version","alias_value":"2301.10785v2","created_at":"2026-07-05T06:18:10.515889+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2301.10785","created_at":"2026-07-05T06:18:10.515889+00:00"},{"alias_kind":"pith_short_12","alias_value":"6HRDQGJUS2P5","created_at":"2026-07-05T06:18:10.515889+00:00"},{"alias_kind":"pith_short_16","alias_value":"6HRDQGJUS2P5CQ2G","created_at":"2026-07-05T06:18:10.515889+00:00"},{"alias_kind":"pith_short_8","alias_value":"6HRDQGJU","created_at":"2026-07-05T06:18:10.515889+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":5,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.16504","citing_title":"Neutrino Flavor Conversion Shapes the Rate of Failed Core-collapse Supernovae","ref_index":56,"is_internal_anchor":false},{"citing_arxiv_id":"2605.18972","citing_title":"Flavor Conversion Enhances or Suppresses Supernova Explodability Independent of the Progenitor Mass","ref_index":58,"is_internal_anchor":false},{"citing_arxiv_id":"2601.08269","citing_title":"Bifurcated Impact of Neutrino Fast Flavor Conversion on Core-collapse Supernovae Informed by Multi-angle Neutrino Radiation Hydrodynamics","ref_index":49,"is_internal_anchor":false},{"citing_arxiv_id":"2601.11272","citing_title":"Intermittent Turbulence, Fast Flavor Conversion, and Observable Supernova Probes","ref_index":5,"is_internal_anchor":false},{"citing_arxiv_id":"2604.25687","citing_title":"Collective neutrino-antineutrino pair oscillations","ref_index":44,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/6HRDQGJUS2P5CQ2GWGLGOR2JK3","json":"https://pith.science/pith/6HRDQGJUS2P5CQ2GWGLGOR2JK3.json","graph_json":"https://pith.science/api/pith-number/6HRDQGJUS2P5CQ2GWGLGOR2JK3/graph.json","events_json":"https://pith.science/api/pith-number/6HRDQGJUS2P5CQ2GWGLGOR2JK3/events.json","paper":"https://pith.science/paper/6HRDQGJU"},"agent_actions":{"view_html":"https://pith.science/pith/6HRDQGJUS2P5CQ2GWGLGOR2JK3","download_json":"https://pith.science/pith/6HRDQGJUS2P5CQ2GWGLGOR2JK3.json","view_paper":"https://pith.science/paper/6HRDQGJU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2301.10785&json=true","fetch_graph":"https://pith.science/api/pith-number/6HRDQGJUS2P5CQ2GWGLGOR2JK3/graph.json","fetch_events":"https://pith.science/api/pith-number/6HRDQGJUS2P5CQ2GWGLGOR2JK3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6HRDQGJUS2P5CQ2GWGLGOR2JK3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6HRDQGJUS2P5CQ2GWGLGOR2JK3/action/storage_attestation","attest_author":"https://pith.science/pith/6HRDQGJUS2P5CQ2GWGLGOR2JK3/action/author_attestation","sign_citation":"https://pith.science/pith/6HRDQGJUS2P5CQ2GWGLGOR2JK3/action/citation_signature","submit_replication":"https://pith.science/pith/6HRDQGJUS2P5CQ2GWGLGOR2JK3/action/replication_record"}},"created_at":"2026-07-05T06:18:10.515889+00:00","updated_at":"2026-07-05T06:18:10.515889+00:00"}