{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:FT6T2OO6LJQ4LMKER3VPG3GVYZ","short_pith_number":"pith:FT6T2OO6","schema_version":"1.0","canonical_sha256":"2cfd3d39de5a61c5b1448eeaf36cd5c65fddf0de87526ce99140bdbc76bc8b1e","source":{"kind":"arxiv","id":"2412.09699","version":2},"attestation_state":"computed","paper":{"title":"Neutrinos from explosive transients at the dawn of multi-messenger astronomy","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-ex","hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Irene Tamborra","submitted_at":"2024-12-12T19:38:31Z","abstract_excerpt":"With the advent of time-domain astronomy and the game-changing next generation of telescopes, we have unprecedented opportunities to explore the most energetic events in our Universe through electromagnetic radiation, gravitational waves, and neutrinos. These are elementary particles, which exist in three different flavors and change the latter as they propagate in the dense core of astrophysical sources as well as en route to Earth. To capitalize on existing and upcoming multi-messenger opportunities, it is crucial to understand: 1. the role of neutrinos in explosive transient sources as well"},"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":"2412.09699","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2024-12-12T19:38:31Z","cross_cats_sorted":["hep-ex","hep-ph"],"title_canon_sha256":"fce6355f96778d7ec1bc0a19fc8c63c18053406e9b77855843ab863f5b27570e","abstract_canon_sha256":"6d9032c00020868de6e045d98b1b52f4cf3d891c817524369670ab2a64711959"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:14:00.606030Z","signature_b64":"RraeWacXPR5rY2JwAVeloGjlfvS1stC7/7AHs+1uTGyJOQSYNr4lmPu+EfN4MMs/zBaNeu+EKcEpn49zCqbdAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2cfd3d39de5a61c5b1448eeaf36cd5c65fddf0de87526ce99140bdbc76bc8b1e","last_reissued_at":"2026-07-05T11:14:00.605529Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:14:00.605529Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Neutrinos from explosive transients at the dawn of multi-messenger astronomy","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-ex","hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Irene Tamborra","submitted_at":"2024-12-12T19:38:31Z","abstract_excerpt":"With the advent of time-domain astronomy and the game-changing next generation of telescopes, we have unprecedented opportunities to explore the most energetic events in our Universe through electromagnetic radiation, gravitational waves, and neutrinos. These are elementary particles, which exist in three different flavors and change the latter as they propagate in the dense core of astrophysical sources as well as en route to Earth. To capitalize on existing and upcoming multi-messenger opportunities, it is crucial to understand: 1. the role of neutrinos in explosive transient sources as well"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2412.09699","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/2412.09699/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":"2412.09699","created_at":"2026-07-05T11:14:00.605589+00:00"},{"alias_kind":"arxiv_version","alias_value":"2412.09699v2","created_at":"2026-07-05T11:14:00.605589+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2412.09699","created_at":"2026-07-05T11:14:00.605589+00:00"},{"alias_kind":"pith_short_12","alias_value":"FT6T2OO6LJQ4","created_at":"2026-07-05T11:14:00.605589+00:00"},{"alias_kind":"pith_short_16","alias_value":"FT6T2OO6LJQ4LMKE","created_at":"2026-07-05T11:14:00.605589+00:00"},{"alias_kind":"pith_short_8","alias_value":"FT6T2OO6","created_at":"2026-07-05T11:14:00.605589+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":7,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2602.15119","citing_title":"Detection horizon for the neutrino burst from the stellar helium flash","ref_index":17,"is_internal_anchor":false},{"citing_arxiv_id":"2605.16504","citing_title":"Neutrino Flavor Conversion Shapes the Rate of Failed Core-collapse Supernovae","ref_index":43,"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":24,"is_internal_anchor":false},{"citing_arxiv_id":"2605.17563","citing_title":"Charged-current neutrino opacity within the relativistic Hartree-Fock framework for astrophysical simulations of core-collapse supernovae and binary neutron star mergers","ref_index":32,"is_internal_anchor":false},{"citing_arxiv_id":"2512.00155","citing_title":"Magnetized Shocks Mediated by Radiation from Leptonic and Hadronic Processes","ref_index":8,"is_internal_anchor":false},{"citing_arxiv_id":"2603.08843","citing_title":"Matter- and magnetically-driven flavor conversion of neutrinos in magnetorotational collapses","ref_index":15,"is_internal_anchor":false},{"citing_arxiv_id":"2604.25687","citing_title":"Collective neutrino-antineutrino pair oscillations","ref_index":4,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/FT6T2OO6LJQ4LMKER3VPG3GVYZ","json":"https://pith.science/pith/FT6T2OO6LJQ4LMKER3VPG3GVYZ.json","graph_json":"https://pith.science/api/pith-number/FT6T2OO6LJQ4LMKER3VPG3GVYZ/graph.json","events_json":"https://pith.science/api/pith-number/FT6T2OO6LJQ4LMKER3VPG3GVYZ/events.json","paper":"https://pith.science/paper/FT6T2OO6"},"agent_actions":{"view_html":"https://pith.science/pith/FT6T2OO6LJQ4LMKER3VPG3GVYZ","download_json":"https://pith.science/pith/FT6T2OO6LJQ4LMKER3VPG3GVYZ.json","view_paper":"https://pith.science/paper/FT6T2OO6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2412.09699&json=true","fetch_graph":"https://pith.science/api/pith-number/FT6T2OO6LJQ4LMKER3VPG3GVYZ/graph.json","fetch_events":"https://pith.science/api/pith-number/FT6T2OO6LJQ4LMKER3VPG3GVYZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FT6T2OO6LJQ4LMKER3VPG3GVYZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FT6T2OO6LJQ4LMKER3VPG3GVYZ/action/storage_attestation","attest_author":"https://pith.science/pith/FT6T2OO6LJQ4LMKER3VPG3GVYZ/action/author_attestation","sign_citation":"https://pith.science/pith/FT6T2OO6LJQ4LMKER3VPG3GVYZ/action/citation_signature","submit_replication":"https://pith.science/pith/FT6T2OO6LJQ4LMKER3VPG3GVYZ/action/replication_record"}},"created_at":"2026-07-05T11:14:00.605589+00:00","updated_at":"2026-07-05T11:14:00.605589+00:00"}