{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:6TJGZNQPC3LSXS53X4JFX3C6LG","short_pith_number":"pith:6TJGZNQP","schema_version":"1.0","canonical_sha256":"f4d26cb60f16d72bcbbbbf125bec5e59987892c2f4cc12ccc4abe9d4906d189b","source":{"kind":"arxiv","id":"1310.2478","version":3},"attestation_state":"computed","paper":{"title":"Comprehensive Bayesian Analysis of Rare (Semi)leptonic and Radiative B Decays","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"hep-ph","authors_text":"Christoph Bobeth (Munich, Danny van Dyk (Siegen U.), Frederik Beaujean (Munich, Tech. U., TUM-IAS Munich), Universe, Universe)","submitted_at":"2013-10-09T13:35:44Z","abstract_excerpt":"The available data on $|\\Delta B| = |\\Delta S| = 1$ decays are in good agreement with the Standard Model when permitting subleading power corrections of about 15% at large hadronic recoil. Constraining new-physics effects in $\\mathcal{C}_7$, $\\mathcal{C}_9$, $\\mathcal{C}_{10}$, the data still demand the same size of power corrections as in the Standard Model. In the presence of chirality-flipped operators, all but one of the power corrections reduce substantially. The Bayes factors are in favor of the Standard Model. Using new lattice inputs for $B\\to K^*$ form factors, the evidence of models "},"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":"1310.2478","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2013-10-09T13:35:44Z","cross_cats_sorted":["hep-ex"],"title_canon_sha256":"ee0da471cf7058efbf8c738cca3473f433f706920cfe1c2f4abb6c6d417bba78","abstract_canon_sha256":"a6d16b97700c12d2114123029e1a6e85f715a39a1c2832f2ed07b25bd0c36bd3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:40:03.407718Z","signature_b64":"PyL8FUT72MM+/Vc6qbR2T3HFeVJdCDnwxzeF7YiL78SEImxSuwINdYQ2hE5PBzwDICHn1pQtbQyk2wUCgfvuAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f4d26cb60f16d72bcbbbbf125bec5e59987892c2f4cc12ccc4abe9d4906d189b","last_reissued_at":"2026-05-18T02:40:03.407205Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:40:03.407205Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Comprehensive Bayesian Analysis of Rare (Semi)leptonic and Radiative B Decays","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"hep-ph","authors_text":"Christoph Bobeth (Munich, Danny van Dyk (Siegen U.), Frederik Beaujean (Munich, Tech. U., TUM-IAS Munich), Universe, Universe)","submitted_at":"2013-10-09T13:35:44Z","abstract_excerpt":"The available data on $|\\Delta B| = |\\Delta S| = 1$ decays are in good agreement with the Standard Model when permitting subleading power corrections of about 15% at large hadronic recoil. Constraining new-physics effects in $\\mathcal{C}_7$, $\\mathcal{C}_9$, $\\mathcal{C}_{10}$, the data still demand the same size of power corrections as in the Standard Model. In the presence of chirality-flipped operators, all but one of the power corrections reduce substantially. The Bayes factors are in favor of the Standard Model. Using new lattice inputs for $B\\to K^*$ form factors, the evidence of models "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1310.2478","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":""},"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":"1310.2478","created_at":"2026-05-18T02:40:03.407290+00:00"},{"alias_kind":"arxiv_version","alias_value":"1310.2478v3","created_at":"2026-05-18T02:40:03.407290+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1310.2478","created_at":"2026-05-18T02:40:03.407290+00:00"},{"alias_kind":"pith_short_12","alias_value":"6TJGZNQPC3LS","created_at":"2026-05-18T12:27:36.564083+00:00"},{"alias_kind":"pith_short_16","alias_value":"6TJGZNQPC3LSXS53","created_at":"2026-05-18T12:27:36.564083+00:00"},{"alias_kind":"pith_short_8","alias_value":"6TJGZNQP","created_at":"2026-05-18T12:27:36.564083+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/6TJGZNQPC3LSXS53X4JFX3C6LG","json":"https://pith.science/pith/6TJGZNQPC3LSXS53X4JFX3C6LG.json","graph_json":"https://pith.science/api/pith-number/6TJGZNQPC3LSXS53X4JFX3C6LG/graph.json","events_json":"https://pith.science/api/pith-number/6TJGZNQPC3LSXS53X4JFX3C6LG/events.json","paper":"https://pith.science/paper/6TJGZNQP"},"agent_actions":{"view_html":"https://pith.science/pith/6TJGZNQPC3LSXS53X4JFX3C6LG","download_json":"https://pith.science/pith/6TJGZNQPC3LSXS53X4JFX3C6LG.json","view_paper":"https://pith.science/paper/6TJGZNQP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1310.2478&json=true","fetch_graph":"https://pith.science/api/pith-number/6TJGZNQPC3LSXS53X4JFX3C6LG/graph.json","fetch_events":"https://pith.science/api/pith-number/6TJGZNQPC3LSXS53X4JFX3C6LG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6TJGZNQPC3LSXS53X4JFX3C6LG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6TJGZNQPC3LSXS53X4JFX3C6LG/action/storage_attestation","attest_author":"https://pith.science/pith/6TJGZNQPC3LSXS53X4JFX3C6LG/action/author_attestation","sign_citation":"https://pith.science/pith/6TJGZNQPC3LSXS53X4JFX3C6LG/action/citation_signature","submit_replication":"https://pith.science/pith/6TJGZNQPC3LSXS53X4JFX3C6LG/action/replication_record"}},"created_at":"2026-05-18T02:40:03.407290+00:00","updated_at":"2026-05-18T02:40:03.407290+00:00"}