{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2004:UKNO2QEWJAYBOW5XZV4ELDFJ7T","short_pith_number":"pith:UKNO2QEW","schema_version":"1.0","canonical_sha256":"a29aed40964830175bb7cd78458ca9fcf31a2c2d46c82be011c33cdfbcdf24d6","source":{"kind":"arxiv","id":"hep-th/0410196","version":1},"attestation_state":"computed","paper":{"title":"Neutrino mixing and cosmological constant","license":"","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Antonio Capolupo, Giuseppe Vitiello, Massimo Blasone, Salvatore Capozziello, Sante Carloni","submitted_at":"2004-10-19T14:44:12Z","abstract_excerpt":"We report on the recent result that the non--perturbative vacuum structure associated with neutrino mixing leads to a non--zero contribution to the value of the cosmological constant. Its value is estimated by using the natural cut--off appearing in the quantum field theory formalism for neutrino mixing."},"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-th/0410196","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"hep-th","submitted_at":"2004-10-19T14:44:12Z","cross_cats_sorted":[],"title_canon_sha256":"39699a989bdec3fb8b6ac904ef1c079518124f0e34ac237155601a8329950db1","abstract_canon_sha256":"dd4c0a60949222f40db336fd1af410bacda0def25f5478e9b91ae881a71ee13b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:01:06.772142Z","signature_b64":"FHC+jw//sOOrum/t2cjXDRKeBb/XTGiIbfIxLdxNS2b53Z/8y19Ac4MBcjKhgzqH8+i3x+cKXLCyykGbDhBGAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a29aed40964830175bb7cd78458ca9fcf31a2c2d46c82be011c33cdfbcdf24d6","last_reissued_at":"2026-05-18T01:01:06.771581Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:01:06.771581Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Neutrino mixing and cosmological constant","license":"","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Antonio Capolupo, Giuseppe Vitiello, Massimo Blasone, Salvatore Capozziello, Sante Carloni","submitted_at":"2004-10-19T14:44:12Z","abstract_excerpt":"We report on the recent result that the non--perturbative vacuum structure associated with neutrino mixing leads to a non--zero contribution to the value of the cosmological constant. Its value is estimated by using the natural cut--off appearing in the quantum field theory formalism for neutrino mixing."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-th/0410196","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":""},"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-th/0410196","created_at":"2026-05-18T01:01:06.771687+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-th/0410196v1","created_at":"2026-05-18T01:01:06.771687+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-th/0410196","created_at":"2026-05-18T01:01:06.771687+00:00"},{"alias_kind":"pith_short_12","alias_value":"UKNO2QEWJAYB","created_at":"2026-05-18T12:25:52.687210+00:00"},{"alias_kind":"pith_short_16","alias_value":"UKNO2QEWJAYBOW5X","created_at":"2026-05-18T12:25:52.687210+00:00"},{"alias_kind":"pith_short_8","alias_value":"UKNO2QEW","created_at":"2026-05-18T12:25:52.687210+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/UKNO2QEWJAYBOW5XZV4ELDFJ7T","json":"https://pith.science/pith/UKNO2QEWJAYBOW5XZV4ELDFJ7T.json","graph_json":"https://pith.science/api/pith-number/UKNO2QEWJAYBOW5XZV4ELDFJ7T/graph.json","events_json":"https://pith.science/api/pith-number/UKNO2QEWJAYBOW5XZV4ELDFJ7T/events.json","paper":"https://pith.science/paper/UKNO2QEW"},"agent_actions":{"view_html":"https://pith.science/pith/UKNO2QEWJAYBOW5XZV4ELDFJ7T","download_json":"https://pith.science/pith/UKNO2QEWJAYBOW5XZV4ELDFJ7T.json","view_paper":"https://pith.science/paper/UKNO2QEW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-th/0410196&json=true","fetch_graph":"https://pith.science/api/pith-number/UKNO2QEWJAYBOW5XZV4ELDFJ7T/graph.json","fetch_events":"https://pith.science/api/pith-number/UKNO2QEWJAYBOW5XZV4ELDFJ7T/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UKNO2QEWJAYBOW5XZV4ELDFJ7T/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UKNO2QEWJAYBOW5XZV4ELDFJ7T/action/storage_attestation","attest_author":"https://pith.science/pith/UKNO2QEWJAYBOW5XZV4ELDFJ7T/action/author_attestation","sign_citation":"https://pith.science/pith/UKNO2QEWJAYBOW5XZV4ELDFJ7T/action/citation_signature","submit_replication":"https://pith.science/pith/UKNO2QEWJAYBOW5XZV4ELDFJ7T/action/replication_record"}},"created_at":"2026-05-18T01:01:06.771687+00:00","updated_at":"2026-05-18T01:01:06.771687+00:00"}