{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:NXHYHK5GN25FGCRY2F5GVCU6GI","short_pith_number":"pith:NXHYHK5G","schema_version":"1.0","canonical_sha256":"6dcf83aba66eba530a38d17a6a8a9e322950f45c4ae0854d4bfd16eec4acfe1a","source":{"kind":"arxiv","id":"1710.00715","version":2},"attestation_state":"computed","paper":{"title":"Neutrino oscillations: the rise of the PMNS paradigm","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"hep-ex","authors_text":"Claudio Giganti, Marco Zito, St\\'ephane Lavignac","submitted_at":"2017-10-02T15:12:34Z","abstract_excerpt":"Since the discovery of neutrino oscillations, the experimental progress in the last two decades has been very fast, with the precision measurements of the neutrino squared-mass differences and of the mixing angles, including the last unknown mixing angle $\\theta_{13}$.\n  Today a very large set of oscillation results obtained with a variety of experimental configurations and techniques can be interpreted in the framework of three active massive neutrinos, whose mass and flavour eigenstates are related by a 3 $\\times$ 3 unitary mixing matrix, the Pontecorvo-Maki-Nakagawa-Sakata (PMNS) matrix, pa"},"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":"1710.00715","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ex","submitted_at":"2017-10-02T15:12:34Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"c30121d66d339cfe887c8df2f02f99299e5850ab783ab1e3b9eb9fef3938be18","abstract_canon_sha256":"398589620231aec625729b2cc08ba1915dd86029c4583ca539615ccbb34a805e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:25:52.785505Z","signature_b64":"5QiCfyOpMbIX1dOmq891WGzC74YMyKxoPNABbMvh20kJlMM7YfsOC88j9A/n/Wzx1qO3YCyHdOnimc1LpWxbDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6dcf83aba66eba530a38d17a6a8a9e322950f45c4ae0854d4bfd16eec4acfe1a","last_reissued_at":"2026-05-18T00:25:52.785084Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:25:52.785084Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Neutrino oscillations: the rise of the PMNS paradigm","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"hep-ex","authors_text":"Claudio Giganti, Marco Zito, St\\'ephane Lavignac","submitted_at":"2017-10-02T15:12:34Z","abstract_excerpt":"Since the discovery of neutrino oscillations, the experimental progress in the last two decades has been very fast, with the precision measurements of the neutrino squared-mass differences and of the mixing angles, including the last unknown mixing angle $\\theta_{13}$.\n  Today a very large set of oscillation results obtained with a variety of experimental configurations and techniques can be interpreted in the framework of three active massive neutrinos, whose mass and flavour eigenstates are related by a 3 $\\times$ 3 unitary mixing matrix, the Pontecorvo-Maki-Nakagawa-Sakata (PMNS) matrix, pa"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1710.00715","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":""},"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":"1710.00715","created_at":"2026-05-18T00:25:52.785142+00:00"},{"alias_kind":"arxiv_version","alias_value":"1710.00715v2","created_at":"2026-05-18T00:25:52.785142+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1710.00715","created_at":"2026-05-18T00:25:52.785142+00:00"},{"alias_kind":"pith_short_12","alias_value":"NXHYHK5GN25F","created_at":"2026-05-18T12:31:34.259226+00:00"},{"alias_kind":"pith_short_16","alias_value":"NXHYHK5GN25FGCRY","created_at":"2026-05-18T12:31:34.259226+00:00"},{"alias_kind":"pith_short_8","alias_value":"NXHYHK5G","created_at":"2026-05-18T12:31:34.259226+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2401.12829","citing_title":"A non-unitary solar constraint for long-baseline neutrino experiments","ref_index":6,"is_internal_anchor":true},{"citing_arxiv_id":"2505.23895","citing_title":"Black hole spectroscopy: from theory to experiment","ref_index":143,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/NXHYHK5GN25FGCRY2F5GVCU6GI","json":"https://pith.science/pith/NXHYHK5GN25FGCRY2F5GVCU6GI.json","graph_json":"https://pith.science/api/pith-number/NXHYHK5GN25FGCRY2F5GVCU6GI/graph.json","events_json":"https://pith.science/api/pith-number/NXHYHK5GN25FGCRY2F5GVCU6GI/events.json","paper":"https://pith.science/paper/NXHYHK5G"},"agent_actions":{"view_html":"https://pith.science/pith/NXHYHK5GN25FGCRY2F5GVCU6GI","download_json":"https://pith.science/pith/NXHYHK5GN25FGCRY2F5GVCU6GI.json","view_paper":"https://pith.science/paper/NXHYHK5G","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1710.00715&json=true","fetch_graph":"https://pith.science/api/pith-number/NXHYHK5GN25FGCRY2F5GVCU6GI/graph.json","fetch_events":"https://pith.science/api/pith-number/NXHYHK5GN25FGCRY2F5GVCU6GI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NXHYHK5GN25FGCRY2F5GVCU6GI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NXHYHK5GN25FGCRY2F5GVCU6GI/action/storage_attestation","attest_author":"https://pith.science/pith/NXHYHK5GN25FGCRY2F5GVCU6GI/action/author_attestation","sign_citation":"https://pith.science/pith/NXHYHK5GN25FGCRY2F5GVCU6GI/action/citation_signature","submit_replication":"https://pith.science/pith/NXHYHK5GN25FGCRY2F5GVCU6GI/action/replication_record"}},"created_at":"2026-05-18T00:25:52.785142+00:00","updated_at":"2026-05-18T00:25:52.785142+00:00"}