{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1999:NSVH72YFPFHFWFTPEBISO25QQE","short_pith_number":"pith:NSVH72YF","schema_version":"1.0","canonical_sha256":"6caa7feb05794e5b166f2051276bb081145c790178eb92a969171a80c63aca53","source":{"kind":"arxiv","id":"hep-ph/9906525","version":1},"attestation_state":"computed","paper":{"title":"Signal of neutrinoless double beta decay, neutrino spectrum and oscillation scenarios","license":"","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Francesco Vissani","submitted_at":"1999-06-28T16:29:26Z","abstract_excerpt":"The lower and upper bounds on the neutrinoless double beta (0nu-2beta) decay rate are obtained, as functions of the parameters of neutrino oscillations and of the lightest neutrino mass. The constraints on these parameters from the search for the 0nu-2beta transition, as well as from the interpretation of solar and atmospheric neutrino data in terms of oscillations, can be conveniently represented in one unitarity triangle. This representation helps to clarify the cases when the 0nu-2beta rate is small; the crucial dependence on the scenarios assumed for solar neutrino oscillations and on the "},"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/9906525","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"hep-ph","submitted_at":"1999-06-28T16:29:26Z","cross_cats_sorted":[],"title_canon_sha256":"7203bfea4a4495f9afa3915ea01694c97930e7bd6ca65172bbb0dde914bb5b34","abstract_canon_sha256":"3955c16bec72d706e4ee13e9cc9bb5eb485e86a8049e6b3d4bb2d73e73fee6de"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:14:21.769561Z","signature_b64":"DC5U4nCJd5JDJtTyWhz2d3JiMVTNSurwG7wl/sBP20C5UBG8VkYwRfh4+vkPYy5zy2kn5EIMGRQdV2ok6UPpCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6caa7feb05794e5b166f2051276bb081145c790178eb92a969171a80c63aca53","last_reissued_at":"2026-07-04T16:14:21.769133Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:14:21.769133Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Signal of neutrinoless double beta decay, neutrino spectrum and oscillation scenarios","license":"","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Francesco Vissani","submitted_at":"1999-06-28T16:29:26Z","abstract_excerpt":"The lower and upper bounds on the neutrinoless double beta (0nu-2beta) decay rate are obtained, as functions of the parameters of neutrino oscillations and of the lightest neutrino mass. The constraints on these parameters from the search for the 0nu-2beta transition, as well as from the interpretation of solar and atmospheric neutrino data in terms of oscillations, can be conveniently represented in one unitarity triangle. This representation helps to clarify the cases when the 0nu-2beta rate is small; the crucial dependence on the scenarios assumed for solar neutrino oscillations and on the "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-ph/9906525","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/hep-ph/9906525/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/9906525","created_at":"2026-07-04T16:14:21.769204+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-ph/9906525v1","created_at":"2026-07-04T16:14:21.769204+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-ph/9906525","created_at":"2026-07-04T16:14:21.769204+00:00"},{"alias_kind":"pith_short_12","alias_value":"NSVH72YFPFHF","created_at":"2026-07-04T16:14:21.769204+00:00"},{"alias_kind":"pith_short_16","alias_value":"NSVH72YFPFHFWFTP","created_at":"2026-07-04T16:14:21.769204+00:00"},{"alias_kind":"pith_short_8","alias_value":"NSVH72YF","created_at":"2026-07-04T16:14:21.769204+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2606.18987","citing_title":"From Evidence to Evident: Decisive Cosmological Evidence for the Normal Neutrino Mass Hierarchy","ref_index":47,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/NSVH72YFPFHFWFTPEBISO25QQE","json":"https://pith.science/pith/NSVH72YFPFHFWFTPEBISO25QQE.json","graph_json":"https://pith.science/api/pith-number/NSVH72YFPFHFWFTPEBISO25QQE/graph.json","events_json":"https://pith.science/api/pith-number/NSVH72YFPFHFWFTPEBISO25QQE/events.json","paper":"https://pith.science/paper/NSVH72YF"},"agent_actions":{"view_html":"https://pith.science/pith/NSVH72YFPFHFWFTPEBISO25QQE","download_json":"https://pith.science/pith/NSVH72YFPFHFWFTPEBISO25QQE.json","view_paper":"https://pith.science/paper/NSVH72YF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-ph/9906525&json=true","fetch_graph":"https://pith.science/api/pith-number/NSVH72YFPFHFWFTPEBISO25QQE/graph.json","fetch_events":"https://pith.science/api/pith-number/NSVH72YFPFHFWFTPEBISO25QQE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NSVH72YFPFHFWFTPEBISO25QQE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NSVH72YFPFHFWFTPEBISO25QQE/action/storage_attestation","attest_author":"https://pith.science/pith/NSVH72YFPFHFWFTPEBISO25QQE/action/author_attestation","sign_citation":"https://pith.science/pith/NSVH72YFPFHFWFTPEBISO25QQE/action/citation_signature","submit_replication":"https://pith.science/pith/NSVH72YFPFHFWFTPEBISO25QQE/action/replication_record"}},"created_at":"2026-07-04T16:14:21.769204+00:00","updated_at":"2026-07-04T16:14:21.769204+00:00"}