{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:BQURUZAYC6TMDOLF2FFJ6NGDRD","short_pith_number":"pith:BQURUZAY","schema_version":"1.0","canonical_sha256":"0c291a641817a6c1b965d14a9f34c388c9ce3528325dd513c14765dad79e35e7","source":{"kind":"arxiv","id":"2206.01674","version":4},"attestation_state":"computed","paper":{"title":"On interplay between flavour anomalies and neutrino properties","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Ant\\'onio P. Morais, Felipe F. Freitas, Jo\\~ao Gon\\c{c}alves, Roman Pasechnik, Werner Porod","submitted_at":"2022-06-03T16:38:20Z","abstract_excerpt":"A minimal extension of the Standard Model (SM) featuring two scalar leptoquarks, an SU(2) doublet with hypercharge 1/6 and a singlet with hypercharge 1/3, is proposed as an economical benchmark model for studies of an interplay between flavour physics and properties of the neutrino sector. The presence of such type of leptoquarks radiatively generates neutrino masses and offers a simultaneous explanation for the current B-physics anomalies involving $b \\to c \\ell \\nu_\\ell$ decays. The model can also accommodate both the muon magnetic moment and the recently reported $W$ mass anomalies, while c"},"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":"2206.01674","kind":"arxiv","version":4},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-ph","submitted_at":"2022-06-03T16:38:20Z","cross_cats_sorted":[],"title_canon_sha256":"2d1c2b39c81486df20a51bc60b050ecba77b86b08bde2bdceb5a1c97b56367ee","abstract_canon_sha256":"199677464baa69f5f0c1fcef9e2867d97fe47555ded7864d07b76170d2b44e34"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:11:12.126476Z","signature_b64":"z1nyvVLn8LkLD5ZZ3VWrITS/kZAckQx0LGE2Z4HfnetN+w0JBYmAmsTv4Fb9YPW1Fu7WVO5Vol/E19zs3hG+Ag==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0c291a641817a6c1b965d14a9f34c388c9ce3528325dd513c14765dad79e35e7","last_reissued_at":"2026-07-05T07:11:12.125910Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:11:12.125910Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On interplay between flavour anomalies and neutrino properties","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Ant\\'onio P. Morais, Felipe F. Freitas, Jo\\~ao Gon\\c{c}alves, Roman Pasechnik, Werner Porod","submitted_at":"2022-06-03T16:38:20Z","abstract_excerpt":"A minimal extension of the Standard Model (SM) featuring two scalar leptoquarks, an SU(2) doublet with hypercharge 1/6 and a singlet with hypercharge 1/3, is proposed as an economical benchmark model for studies of an interplay between flavour physics and properties of the neutrino sector. The presence of such type of leptoquarks radiatively generates neutrino masses and offers a simultaneous explanation for the current B-physics anomalies involving $b \\to c \\ell \\nu_\\ell$ decays. The model can also accommodate both the muon magnetic moment and the recently reported $W$ mass anomalies, while c"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2206.01674","kind":"arxiv","version":4},"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/2206.01674/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":"2206.01674","created_at":"2026-07-05T07:11:12.125966+00:00"},{"alias_kind":"arxiv_version","alias_value":"2206.01674v4","created_at":"2026-07-05T07:11:12.125966+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2206.01674","created_at":"2026-07-05T07:11:12.125966+00:00"},{"alias_kind":"pith_short_12","alias_value":"BQURUZAYC6TM","created_at":"2026-07-05T07:11:12.125966+00:00"},{"alias_kind":"pith_short_16","alias_value":"BQURUZAYC6TMDOLF","created_at":"2026-07-05T07:11:12.125966+00:00"},{"alias_kind":"pith_short_8","alias_value":"BQURUZAY","created_at":"2026-07-05T07:11:12.125966+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2501.01286","citing_title":"Gravitational waves from color restoration in a leptoquark model of radiative neutrino masses","ref_index":28,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/BQURUZAYC6TMDOLF2FFJ6NGDRD","json":"https://pith.science/pith/BQURUZAYC6TMDOLF2FFJ6NGDRD.json","graph_json":"https://pith.science/api/pith-number/BQURUZAYC6TMDOLF2FFJ6NGDRD/graph.json","events_json":"https://pith.science/api/pith-number/BQURUZAYC6TMDOLF2FFJ6NGDRD/events.json","paper":"https://pith.science/paper/BQURUZAY"},"agent_actions":{"view_html":"https://pith.science/pith/BQURUZAYC6TMDOLF2FFJ6NGDRD","download_json":"https://pith.science/pith/BQURUZAYC6TMDOLF2FFJ6NGDRD.json","view_paper":"https://pith.science/paper/BQURUZAY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2206.01674&json=true","fetch_graph":"https://pith.science/api/pith-number/BQURUZAYC6TMDOLF2FFJ6NGDRD/graph.json","fetch_events":"https://pith.science/api/pith-number/BQURUZAYC6TMDOLF2FFJ6NGDRD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BQURUZAYC6TMDOLF2FFJ6NGDRD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BQURUZAYC6TMDOLF2FFJ6NGDRD/action/storage_attestation","attest_author":"https://pith.science/pith/BQURUZAYC6TMDOLF2FFJ6NGDRD/action/author_attestation","sign_citation":"https://pith.science/pith/BQURUZAYC6TMDOLF2FFJ6NGDRD/action/citation_signature","submit_replication":"https://pith.science/pith/BQURUZAYC6TMDOLF2FFJ6NGDRD/action/replication_record"}},"created_at":"2026-07-05T07:11:12.125966+00:00","updated_at":"2026-07-05T07:11:12.125966+00:00"}