{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1996:E6EDZDMCG3JDXPZEHALWKZCWMN","short_pith_number":"pith:E6EDZDMC","schema_version":"1.0","canonical_sha256":"27883c8d8236d23bbf2438176564566354bf0f85256e3fa68826622cbc7054dd","source":{"kind":"arxiv","id":"hep-ph/9601311","version":2},"attestation_state":"computed","paper":{"title":"High Energy Cosmic Neutrinos and the Equivalence Principle","license":"","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Alexei Yu. Smirnov, Hisakazu Minakata","submitted_at":"1996-01-23T10:11:03Z","abstract_excerpt":"Observation of the ultra-high energy neutrinos, in particular, detection of $\\nu_{\\tau}$ from cosmologically distant sources like active galactic nuclei (AGN) opens new possibilities to search for neutrino flavor conversion. We consider effects of violation of the equivalence principle (VEP) on propagation of these cosmic neutrinos. Two effects are studied: (1) the oscillations of neutrinos due to the VEP in the gravitational field of our Galaxy and in the intergalactic space, (2) the resonance flavor conversion driven by the gravitational potential of the AGN. We show that the ultra-high ener"},"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":"hep-ph/9601311","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"hep-ph","submitted_at":"1996-01-23T10:11:03Z","cross_cats_sorted":[],"title_canon_sha256":"e5458de9a3fdc98eaa1e6c3cecebb23605665ba223edce7c3521c9bd0ca3e2d5","abstract_canon_sha256":"42ca8e6032f82c56832a7e0d4b11ebca2df046c675540a63ba0378fc6a5cda37"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T17:18:26.167188Z","signature_b64":"WUBZ31zG7VsPv6RTqgnKwMZvPRu/Mdvgg6oHkYmP+35NL9OSb+nAySf3TBN/Tv7/YvhdnoSmN8HQghsu2DnTCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"27883c8d8236d23bbf2438176564566354bf0f85256e3fa68826622cbc7054dd","last_reissued_at":"2026-07-04T17:18:26.166844Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T17:18:26.166844Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"High Energy Cosmic Neutrinos and the Equivalence Principle","license":"","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Alexei Yu. Smirnov, Hisakazu Minakata","submitted_at":"1996-01-23T10:11:03Z","abstract_excerpt":"Observation of the ultra-high energy neutrinos, in particular, detection of $\\nu_{\\tau}$ from cosmologically distant sources like active galactic nuclei (AGN) opens new possibilities to search for neutrino flavor conversion. We consider effects of violation of the equivalence principle (VEP) on propagation of these cosmic neutrinos. Two effects are studied: (1) the oscillations of neutrinos due to the VEP in the gravitational field of our Galaxy and in the intergalactic space, (2) the resonance flavor conversion driven by the gravitational potential of the AGN. We show that the ultra-high ener"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-ph/9601311","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/hep-ph/9601311/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":"hep-ph/9601311","created_at":"2026-07-04T17:18:26.166903+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-ph/9601311v2","created_at":"2026-07-04T17:18:26.166903+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-ph/9601311","created_at":"2026-07-04T17:18:26.166903+00:00"},{"alias_kind":"pith_short_12","alias_value":"E6EDZDMCG3JD","created_at":"2026-07-04T17:18:26.166903+00:00"},{"alias_kind":"pith_short_16","alias_value":"E6EDZDMCG3JDXPZE","created_at":"2026-07-04T17:18:26.166903+00:00"},{"alias_kind":"pith_short_8","alias_value":"E6EDZDMC","created_at":"2026-07-04T17:18:26.166903+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.29105","citing_title":"Visible inelasticity as a probe of tau flavor content of astrophysical neutrinos","ref_index":51,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/E6EDZDMCG3JDXPZEHALWKZCWMN","json":"https://pith.science/pith/E6EDZDMCG3JDXPZEHALWKZCWMN.json","graph_json":"https://pith.science/api/pith-number/E6EDZDMCG3JDXPZEHALWKZCWMN/graph.json","events_json":"https://pith.science/api/pith-number/E6EDZDMCG3JDXPZEHALWKZCWMN/events.json","paper":"https://pith.science/paper/E6EDZDMC"},"agent_actions":{"view_html":"https://pith.science/pith/E6EDZDMCG3JDXPZEHALWKZCWMN","download_json":"https://pith.science/pith/E6EDZDMCG3JDXPZEHALWKZCWMN.json","view_paper":"https://pith.science/paper/E6EDZDMC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-ph/9601311&json=true","fetch_graph":"https://pith.science/api/pith-number/E6EDZDMCG3JDXPZEHALWKZCWMN/graph.json","fetch_events":"https://pith.science/api/pith-number/E6EDZDMCG3JDXPZEHALWKZCWMN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/E6EDZDMCG3JDXPZEHALWKZCWMN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/E6EDZDMCG3JDXPZEHALWKZCWMN/action/storage_attestation","attest_author":"https://pith.science/pith/E6EDZDMCG3JDXPZEHALWKZCWMN/action/author_attestation","sign_citation":"https://pith.science/pith/E6EDZDMCG3JDXPZEHALWKZCWMN/action/citation_signature","submit_replication":"https://pith.science/pith/E6EDZDMCG3JDXPZEHALWKZCWMN/action/replication_record"}},"created_at":"2026-07-04T17:18:26.166903+00:00","updated_at":"2026-07-04T17:18:26.166903+00:00"}