{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:CFPYYUEYLCQQFEXJUVQYQ5LQIL","short_pith_number":"pith:CFPYYUEY","schema_version":"1.0","canonical_sha256":"115f8c509858a10292e9a56188757042f725d9dcb8e4d25dad3e81d92b42cb24","source":{"kind":"arxiv","id":"2508.18441","version":1},"attestation_state":"computed","paper":{"title":"Super-Accreting Active Galactic Nuclei as Neutrino Sources","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Gustavo E. Romero, Pablo Sotomayor","submitted_at":"2025-08-25T19:39:30Z","abstract_excerpt":"Active galactic nuclei (AGNs) often exhibit broad-line regions (BLRs), populated by high-velocity clouds in Keplerian orbits around the central supermassive black hole (SMBH) at subparsec scales. During episodes of intense super-Eddington accretion, the disk can launch a powerful radiation-driven wind that overtakes the BLR clouds, forming bowshocks. Two shocks arise: one into the wind and another into the cloud. If adiabatic, electrons and protons are efficiently accelerated via Fermi processes to relativistic energies. In dense winds, the resulting high-energy photons are absorbed and reproc"},"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":"2508.18441","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2025-08-25T19:39:30Z","cross_cats_sorted":[],"title_canon_sha256":"b416bc6a99d30232cbbbcd6def04e2686f9f94dcece45e735fa05c3b3150b3db","abstract_canon_sha256":"fe6dc313b50635ca5c3a628471a225596b797a4e6457385c03b16887b26d713a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:59:24.385958Z","signature_b64":"sB39DIjKL/grEB9ErKIzoTNc6VU6ksuoNJg4SH8P5SDY1ym/w+hxNUz2Q2U+bbFj85odhi/Jxh+hnJNFT5bzAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"115f8c509858a10292e9a56188757042f725d9dcb8e4d25dad3e81d92b42cb24","last_reissued_at":"2026-07-05T11:59:24.385462Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:59:24.385462Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Super-Accreting Active Galactic Nuclei as Neutrino Sources","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Gustavo E. Romero, Pablo Sotomayor","submitted_at":"2025-08-25T19:39:30Z","abstract_excerpt":"Active galactic nuclei (AGNs) often exhibit broad-line regions (BLRs), populated by high-velocity clouds in Keplerian orbits around the central supermassive black hole (SMBH) at subparsec scales. During episodes of intense super-Eddington accretion, the disk can launch a powerful radiation-driven wind that overtakes the BLR clouds, forming bowshocks. Two shocks arise: one into the wind and another into the cloud. If adiabatic, electrons and protons are efficiently accelerated via Fermi processes to relativistic energies. In dense winds, the resulting high-energy photons are absorbed and reproc"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2508.18441","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/2508.18441/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":"2508.18441","created_at":"2026-07-05T11:59:24.385528+00:00"},{"alias_kind":"arxiv_version","alias_value":"2508.18441v1","created_at":"2026-07-05T11:59:24.385528+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2508.18441","created_at":"2026-07-05T11:59:24.385528+00:00"},{"alias_kind":"pith_short_12","alias_value":"CFPYYUEYLCQQ","created_at":"2026-07-05T11:59:24.385528+00:00"},{"alias_kind":"pith_short_16","alias_value":"CFPYYUEYLCQQFEXJ","created_at":"2026-07-05T11:59:24.385528+00:00"},{"alias_kind":"pith_short_8","alias_value":"CFPYYUEY","created_at":"2026-07-05T11:59:24.385528+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/CFPYYUEYLCQQFEXJUVQYQ5LQIL","json":"https://pith.science/pith/CFPYYUEYLCQQFEXJUVQYQ5LQIL.json","graph_json":"https://pith.science/api/pith-number/CFPYYUEYLCQQFEXJUVQYQ5LQIL/graph.json","events_json":"https://pith.science/api/pith-number/CFPYYUEYLCQQFEXJUVQYQ5LQIL/events.json","paper":"https://pith.science/paper/CFPYYUEY"},"agent_actions":{"view_html":"https://pith.science/pith/CFPYYUEYLCQQFEXJUVQYQ5LQIL","download_json":"https://pith.science/pith/CFPYYUEYLCQQFEXJUVQYQ5LQIL.json","view_paper":"https://pith.science/paper/CFPYYUEY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2508.18441&json=true","fetch_graph":"https://pith.science/api/pith-number/CFPYYUEYLCQQFEXJUVQYQ5LQIL/graph.json","fetch_events":"https://pith.science/api/pith-number/CFPYYUEYLCQQFEXJUVQYQ5LQIL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CFPYYUEYLCQQFEXJUVQYQ5LQIL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CFPYYUEYLCQQFEXJUVQYQ5LQIL/action/storage_attestation","attest_author":"https://pith.science/pith/CFPYYUEYLCQQFEXJUVQYQ5LQIL/action/author_attestation","sign_citation":"https://pith.science/pith/CFPYYUEYLCQQFEXJUVQYQ5LQIL/action/citation_signature","submit_replication":"https://pith.science/pith/CFPYYUEYLCQQFEXJUVQYQ5LQIL/action/replication_record"}},"created_at":"2026-07-05T11:59:24.385528+00:00","updated_at":"2026-07-05T11:59:24.385528+00:00"}