{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:4OTNXTYO5QCW6AAOOQPFTAJ4J7","short_pith_number":"pith:4OTNXTYO","schema_version":"1.0","canonical_sha256":"e3a6dbcf0eec056f000e741e59813c4fcfb5ec6659ed1e69df64e657939900ca","source":{"kind":"arxiv","id":"1903.10932","version":3},"attestation_state":"computed","paper":{"title":"Implications for New Physics in $b\\to s \\mu\\mu$ transitions after recent measurements by Belle and LHCb","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Dinesh Kumar, Enrico Maria Sessolo, Kamila Kowalska","submitted_at":"2019-03-26T14:52:06Z","abstract_excerpt":"We present a Bayesian analysis of the implications for new physics in semileptonic $b\\to s$ transitions after including new measurements of $R_K$ at LHCb and new determinations of $R_{K^*}$ and $R_{K^{*+}}$ at Belle. We perform global fits with 1, 2, 4, and 8 input Wilson coefficients, plus one CKM nuisance parameter to take into account uncertainties that are not factorizable. We infer the 68% and 95.4% credibility regions of the marginalized posterior probability density for all scenarios and perform comparisons of models in pairs by calculating the Bayes factor given a common data set. We t"},"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":"1903.10932","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2019-03-26T14:52:06Z","cross_cats_sorted":[],"title_canon_sha256":"122e8bbf62e02ee46a2c9a41bd2f18c98218f3129e29507a50d3e77f8bcfa1f2","abstract_canon_sha256":"60754e2a65362833dcee87ca6da90549d632197ef4323f1c1e8788554aadc168"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:11:33.045127Z","signature_b64":"6ccOEqchtWyN9yIMdw6RZCwAfhkApfNNMpKnjUGPqu3TTdFnKL8R8N6w096G7pCOivl/0ACykGX+t6TyMJX4Dw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e3a6dbcf0eec056f000e741e59813c4fcfb5ec6659ed1e69df64e657939900ca","last_reissued_at":"2026-07-05T00:11:33.044675Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:11:33.044675Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Implications for New Physics in $b\\to s \\mu\\mu$ transitions after recent measurements by Belle and LHCb","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Dinesh Kumar, Enrico Maria Sessolo, Kamila Kowalska","submitted_at":"2019-03-26T14:52:06Z","abstract_excerpt":"We present a Bayesian analysis of the implications for new physics in semileptonic $b\\to s$ transitions after including new measurements of $R_K$ at LHCb and new determinations of $R_{K^*}$ and $R_{K^{*+}}$ at Belle. We perform global fits with 1, 2, 4, and 8 input Wilson coefficients, plus one CKM nuisance parameter to take into account uncertainties that are not factorizable. We infer the 68% and 95.4% credibility regions of the marginalized posterior probability density for all scenarios and perform comparisons of models in pairs by calculating the Bayes factor given a common data set. We t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1903.10932","kind":"arxiv","version":3},"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/1903.10932/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":"1903.10932","created_at":"2026-07-05T00:11:33.044723+00:00"},{"alias_kind":"arxiv_version","alias_value":"1903.10932v3","created_at":"2026-07-05T00:11:33.044723+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1903.10932","created_at":"2026-07-05T00:11:33.044723+00:00"},{"alias_kind":"pith_short_12","alias_value":"4OTNXTYO5QCW","created_at":"2026-07-05T00:11:33.044723+00:00"},{"alias_kind":"pith_short_16","alias_value":"4OTNXTYO5QCW6AAO","created_at":"2026-07-05T00:11:33.044723+00:00"},{"alias_kind":"pith_short_8","alias_value":"4OTNXTYO","created_at":"2026-07-05T00:11:33.044723+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"1906.08596","citing_title":"Global Bayesian Analysis of new physics in $b \\to s \\mu\\mu$ transitions after Moriond-2019","ref_index":14,"is_internal_anchor":false},{"citing_arxiv_id":"1907.05158","citing_title":"Flavour anomalies and (fundamental) partial compositeness","ref_index":32,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/4OTNXTYO5QCW6AAOOQPFTAJ4J7","json":"https://pith.science/pith/4OTNXTYO5QCW6AAOOQPFTAJ4J7.json","graph_json":"https://pith.science/api/pith-number/4OTNXTYO5QCW6AAOOQPFTAJ4J7/graph.json","events_json":"https://pith.science/api/pith-number/4OTNXTYO5QCW6AAOOQPFTAJ4J7/events.json","paper":"https://pith.science/paper/4OTNXTYO"},"agent_actions":{"view_html":"https://pith.science/pith/4OTNXTYO5QCW6AAOOQPFTAJ4J7","download_json":"https://pith.science/pith/4OTNXTYO5QCW6AAOOQPFTAJ4J7.json","view_paper":"https://pith.science/paper/4OTNXTYO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1903.10932&json=true","fetch_graph":"https://pith.science/api/pith-number/4OTNXTYO5QCW6AAOOQPFTAJ4J7/graph.json","fetch_events":"https://pith.science/api/pith-number/4OTNXTYO5QCW6AAOOQPFTAJ4J7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4OTNXTYO5QCW6AAOOQPFTAJ4J7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4OTNXTYO5QCW6AAOOQPFTAJ4J7/action/storage_attestation","attest_author":"https://pith.science/pith/4OTNXTYO5QCW6AAOOQPFTAJ4J7/action/author_attestation","sign_citation":"https://pith.science/pith/4OTNXTYO5QCW6AAOOQPFTAJ4J7/action/citation_signature","submit_replication":"https://pith.science/pith/4OTNXTYO5QCW6AAOOQPFTAJ4J7/action/replication_record"}},"created_at":"2026-07-05T00:11:33.044723+00:00","updated_at":"2026-07-05T00:11:33.044723+00:00"}