{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:PM4N6FSCE6T45KYKS356FG644T","short_pith_number":"pith:PM4N6FSC","schema_version":"1.0","canonical_sha256":"7b38df164227a7ceab0a96fbe29bdce4d02b7f1c329294e8e97c4ad09bcd9e86","source":{"kind":"arxiv","id":"2405.07695","version":2},"attestation_state":"computed","paper":{"title":"High-energy neutrinos from late-time jets of gamma-ray bursts seeded with cocoon photons","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Hamid Hamidani, Riki Matsui, Shigeo S Kimura","submitted_at":"2024-05-13T12:30:09Z","abstract_excerpt":"In gamma-ray bursts (GRBs), $\\sim$ 100 - 1000 s after the prompt emission, afterglow observations have consistently shown X-ray excesses detected in the form of flares (XFs; in long GRBs) or extended emission (EEs; in short GRBs). These observations are interpreted as emissions from jets launched by late central engine activity. However, the characteristics of these late-time jets, particularly the dissipation radius ($r_{\\rm diss}$), Lorentz factor ($\\Gamma$), and cosmic-ray loading factor ($\\xi_p$), remain unknown despite their importance. Here, in order to understand the properties of the l"},"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":"2405.07695","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2024-05-13T12:30:09Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"cb10e5ef8f1378a45bd49a37c2f92513b8898fb6bb3e9f00b901550d4518a460","abstract_canon_sha256":"07500f54dadada66cab8b64c2d09fdc5db2dae5f9e214e000f8ff009f37c857a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:19:45.191708Z","signature_b64":"/Dj788HCCcAFJVBfByzv7NcOTO4Cx3MFg3jANCMoEaHFC18T6Azu4h0BfGvWAQlNNwR7fVhnX6Go7lmMmVL6Dg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7b38df164227a7ceab0a96fbe29bdce4d02b7f1c329294e8e97c4ad09bcd9e86","last_reissued_at":"2026-07-05T08:19:45.191260Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:19:45.191260Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"High-energy neutrinos from late-time jets of gamma-ray bursts seeded with cocoon photons","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Hamid Hamidani, Riki Matsui, Shigeo S Kimura","submitted_at":"2024-05-13T12:30:09Z","abstract_excerpt":"In gamma-ray bursts (GRBs), $\\sim$ 100 - 1000 s after the prompt emission, afterglow observations have consistently shown X-ray excesses detected in the form of flares (XFs; in long GRBs) or extended emission (EEs; in short GRBs). These observations are interpreted as emissions from jets launched by late central engine activity. However, the characteristics of these late-time jets, particularly the dissipation radius ($r_{\\rm diss}$), Lorentz factor ($\\Gamma$), and cosmic-ray loading factor ($\\xi_p$), remain unknown despite their importance. Here, in order to understand the properties of the l"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2405.07695","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/2405.07695/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":"2405.07695","created_at":"2026-07-05T08:19:45.191321+00:00"},{"alias_kind":"arxiv_version","alias_value":"2405.07695v2","created_at":"2026-07-05T08:19:45.191321+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2405.07695","created_at":"2026-07-05T08:19:45.191321+00:00"},{"alias_kind":"pith_short_12","alias_value":"PM4N6FSCE6T4","created_at":"2026-07-05T08:19:45.191321+00:00"},{"alias_kind":"pith_short_16","alias_value":"PM4N6FSCE6T45KYK","created_at":"2026-07-05T08:19:45.191321+00:00"},{"alias_kind":"pith_short_8","alias_value":"PM4N6FSC","created_at":"2026-07-05T08:19:45.191321+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/PM4N6FSCE6T45KYKS356FG644T","json":"https://pith.science/pith/PM4N6FSCE6T45KYKS356FG644T.json","graph_json":"https://pith.science/api/pith-number/PM4N6FSCE6T45KYKS356FG644T/graph.json","events_json":"https://pith.science/api/pith-number/PM4N6FSCE6T45KYKS356FG644T/events.json","paper":"https://pith.science/paper/PM4N6FSC"},"agent_actions":{"view_html":"https://pith.science/pith/PM4N6FSCE6T45KYKS356FG644T","download_json":"https://pith.science/pith/PM4N6FSCE6T45KYKS356FG644T.json","view_paper":"https://pith.science/paper/PM4N6FSC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2405.07695&json=true","fetch_graph":"https://pith.science/api/pith-number/PM4N6FSCE6T45KYKS356FG644T/graph.json","fetch_events":"https://pith.science/api/pith-number/PM4N6FSCE6T45KYKS356FG644T/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PM4N6FSCE6T45KYKS356FG644T/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PM4N6FSCE6T45KYKS356FG644T/action/storage_attestation","attest_author":"https://pith.science/pith/PM4N6FSCE6T45KYKS356FG644T/action/author_attestation","sign_citation":"https://pith.science/pith/PM4N6FSCE6T45KYKS356FG644T/action/citation_signature","submit_replication":"https://pith.science/pith/PM4N6FSCE6T45KYKS356FG644T/action/replication_record"}},"created_at":"2026-07-05T08:19:45.191321+00:00","updated_at":"2026-07-05T08:19:45.191321+00:00"}