{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:OACHB67XZY627AIMSX2ATVA7SU","short_pith_number":"pith:OACHB67X","schema_version":"1.0","canonical_sha256":"700470fbf7ce3daf810c95f409d41f9521562acd00980aed9cdc561cd8650cde","source":{"kind":"arxiv","id":"2407.11410","version":1},"attestation_state":"computed","paper":{"title":"High-energy neutrino emission from tidal disruption event outflow-cloud interactions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.HE","authors_text":"Hanji Wu, Kai Wang, Wei Wang","submitted_at":"2024-07-16T05:52:54Z","abstract_excerpt":"Tidal disruption events (TDEs), characterized by their luminous transients and high-velocity outflows, have emerged as plausible sources of high-energy neutrinos contributing to the diffuse neutrino. In this study, we calculate the contribution of TDEs to the diffuse neutrino by employing the outflow-cloud model within the TDE framework. Our analysis indicates that the contribution of TDEs becomes negligible when the redshift $Z$ exceeds 2. Employing a set of fiducial values, which includes outflow energy $E_{\\rm kin}=10^{51}$ erg, a proton spectrum cutoff energy $E_{\\rm p,max}=100$ PeV, a vol"},"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":"2407.11410","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2024-07-16T05:52:54Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"17732f2e0d1bf525a4482638608eebc36f94b64ce1a7cae66c3d52f0ea9bff87","abstract_canon_sha256":"bbf93e6278a1c96f2884dba9c2dcd0313655230ad5d3cef2909fa98ad2cf4a8e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:44:24.100061Z","signature_b64":"kqzsUcJZFV6rBfLzuuOEko48sxix4h8fPB9RqsJYjN9EQg18R228bmPguOU6Yo9WhPM0QVTLMMLHJzqJb3KuBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"700470fbf7ce3daf810c95f409d41f9521562acd00980aed9cdc561cd8650cde","last_reissued_at":"2026-07-05T08:44:24.099663Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:44:24.099663Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"High-energy neutrino emission from tidal disruption event outflow-cloud interactions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.HE","authors_text":"Hanji Wu, Kai Wang, Wei Wang","submitted_at":"2024-07-16T05:52:54Z","abstract_excerpt":"Tidal disruption events (TDEs), characterized by their luminous transients and high-velocity outflows, have emerged as plausible sources of high-energy neutrinos contributing to the diffuse neutrino. In this study, we calculate the contribution of TDEs to the diffuse neutrino by employing the outflow-cloud model within the TDE framework. Our analysis indicates that the contribution of TDEs becomes negligible when the redshift $Z$ exceeds 2. Employing a set of fiducial values, which includes outflow energy $E_{\\rm kin}=10^{51}$ erg, a proton spectrum cutoff energy $E_{\\rm p,max}=100$ PeV, a vol"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2407.11410","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2407.11410/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":"2407.11410","created_at":"2026-07-05T08:44:24.099721+00:00"},{"alias_kind":"arxiv_version","alias_value":"2407.11410v1","created_at":"2026-07-05T08:44:24.099721+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2407.11410","created_at":"2026-07-05T08:44:24.099721+00:00"},{"alias_kind":"pith_short_12","alias_value":"OACHB67XZY62","created_at":"2026-07-05T08:44:24.099721+00:00"},{"alias_kind":"pith_short_16","alias_value":"OACHB67XZY627AIM","created_at":"2026-07-05T08:44:24.099721+00:00"},{"alias_kind":"pith_short_8","alias_value":"OACHB67X","created_at":"2026-07-05T08:44:24.099721+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/OACHB67XZY627AIMSX2ATVA7SU","json":"https://pith.science/pith/OACHB67XZY627AIMSX2ATVA7SU.json","graph_json":"https://pith.science/api/pith-number/OACHB67XZY627AIMSX2ATVA7SU/graph.json","events_json":"https://pith.science/api/pith-number/OACHB67XZY627AIMSX2ATVA7SU/events.json","paper":"https://pith.science/paper/OACHB67X"},"agent_actions":{"view_html":"https://pith.science/pith/OACHB67XZY627AIMSX2ATVA7SU","download_json":"https://pith.science/pith/OACHB67XZY627AIMSX2ATVA7SU.json","view_paper":"https://pith.science/paper/OACHB67X","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2407.11410&json=true","fetch_graph":"https://pith.science/api/pith-number/OACHB67XZY627AIMSX2ATVA7SU/graph.json","fetch_events":"https://pith.science/api/pith-number/OACHB67XZY627AIMSX2ATVA7SU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OACHB67XZY627AIMSX2ATVA7SU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OACHB67XZY627AIMSX2ATVA7SU/action/storage_attestation","attest_author":"https://pith.science/pith/OACHB67XZY627AIMSX2ATVA7SU/action/author_attestation","sign_citation":"https://pith.science/pith/OACHB67XZY627AIMSX2ATVA7SU/action/citation_signature","submit_replication":"https://pith.science/pith/OACHB67XZY627AIMSX2ATVA7SU/action/replication_record"}},"created_at":"2026-07-05T08:44:24.099721+00:00","updated_at":"2026-07-05T08:44:24.099721+00:00"}