{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:RAFOZH2XUALXQDNVIT6MCJBBME","short_pith_number":"pith:RAFOZH2X","schema_version":"1.0","canonical_sha256":"880aec9f57a017780db544fcc12421613ab9a285c80aa609b8280bbe866f5d9a","source":{"kind":"arxiv","id":"1402.1453","version":2},"attestation_state":"computed","paper":{"title":"Impact of sterile neutrinos on the early time flux from a galactic supernova","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","astro-ph.HE"],"primary_cat":"hep-ph","authors_text":"Arman Esmaili, O. L. G. Peres, Pasquale Dario Serpico","submitted_at":"2014-02-06T18:50:04Z","abstract_excerpt":"We study the impact of the existence of an eV-mass scale sterile neutrino---with parameters in the ballpark of what is required to fit the laboratory anomalies---on the early time profile of the electron neutrino and antineutrino fluxes associated to a core-collapse supernova (SN). In particular, we focus on the universal feature of neutronization burst expected in the first tens of ms of the signal: provided that a detector with sufficient sensitivity is available, it is well-known that in the 3 neutrino framework the detection of the neutronization burst in neutrino channel would signal inve"},"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":"1402.1453","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2014-02-06T18:50:04Z","cross_cats_sorted":["astro-ph.GA","astro-ph.HE"],"title_canon_sha256":"dae7e53a78d2a802eadb2c206d88966f1981285b99605101c63da0abfe7700f1","abstract_canon_sha256":"6cb98bb96d6c0d6e8f26da66707c302a38d3cfb561f71468c5f1f067dc104131"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:44:47.472607Z","signature_b64":"Sw784SDhYe4GStiLFe5NkkUsEyuVP5U33G8TxpVP7Jc8XydHAKiTRUJzIWhjrSbH1mKuVEtetfyrGakYf+0AAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"880aec9f57a017780db544fcc12421613ab9a285c80aa609b8280bbe866f5d9a","last_reissued_at":"2026-05-18T02:44:47.472131Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:44:47.472131Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Impact of sterile neutrinos on the early time flux from a galactic supernova","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","astro-ph.HE"],"primary_cat":"hep-ph","authors_text":"Arman Esmaili, O. L. G. Peres, Pasquale Dario Serpico","submitted_at":"2014-02-06T18:50:04Z","abstract_excerpt":"We study the impact of the existence of an eV-mass scale sterile neutrino---with parameters in the ballpark of what is required to fit the laboratory anomalies---on the early time profile of the electron neutrino and antineutrino fluxes associated to a core-collapse supernova (SN). In particular, we focus on the universal feature of neutronization burst expected in the first tens of ms of the signal: provided that a detector with sufficient sensitivity is available, it is well-known that in the 3 neutrino framework the detection of the neutronization burst in neutrino channel would signal inve"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1402.1453","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":"1402.1453","created_at":"2026-05-18T02:44:47.472194+00:00"},{"alias_kind":"arxiv_version","alias_value":"1402.1453v2","created_at":"2026-05-18T02:44:47.472194+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1402.1453","created_at":"2026-05-18T02:44:47.472194+00:00"},{"alias_kind":"pith_short_12","alias_value":"RAFOZH2XUALX","created_at":"2026-05-18T12:28:46.137349+00:00"},{"alias_kind":"pith_short_16","alias_value":"RAFOZH2XUALXQDNV","created_at":"2026-05-18T12:28:46.137349+00:00"},{"alias_kind":"pith_short_8","alias_value":"RAFOZH2X","created_at":"2026-05-18T12:28:46.137349+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/RAFOZH2XUALXQDNVIT6MCJBBME","json":"https://pith.science/pith/RAFOZH2XUALXQDNVIT6MCJBBME.json","graph_json":"https://pith.science/api/pith-number/RAFOZH2XUALXQDNVIT6MCJBBME/graph.json","events_json":"https://pith.science/api/pith-number/RAFOZH2XUALXQDNVIT6MCJBBME/events.json","paper":"https://pith.science/paper/RAFOZH2X"},"agent_actions":{"view_html":"https://pith.science/pith/RAFOZH2XUALXQDNVIT6MCJBBME","download_json":"https://pith.science/pith/RAFOZH2XUALXQDNVIT6MCJBBME.json","view_paper":"https://pith.science/paper/RAFOZH2X","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1402.1453&json=true","fetch_graph":"https://pith.science/api/pith-number/RAFOZH2XUALXQDNVIT6MCJBBME/graph.json","fetch_events":"https://pith.science/api/pith-number/RAFOZH2XUALXQDNVIT6MCJBBME/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RAFOZH2XUALXQDNVIT6MCJBBME/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RAFOZH2XUALXQDNVIT6MCJBBME/action/storage_attestation","attest_author":"https://pith.science/pith/RAFOZH2XUALXQDNVIT6MCJBBME/action/author_attestation","sign_citation":"https://pith.science/pith/RAFOZH2XUALXQDNVIT6MCJBBME/action/citation_signature","submit_replication":"https://pith.science/pith/RAFOZH2XUALXQDNVIT6MCJBBME/action/replication_record"}},"created_at":"2026-05-18T02:44:47.472194+00:00","updated_at":"2026-05-18T02:44:47.472194+00:00"}