{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2002:QGLMLYHMN5CFXKXMVEMXMNLQIE","short_pith_number":"pith:QGLMLYHM","schema_version":"1.0","canonical_sha256":"8196c5e0ec6f445baaeca9197635704135ee755ee5132aed73554ad4ab9b7c3c","source":{"kind":"arxiv","id":"hep-ph/0206242","version":2},"attestation_state":"computed","paper":{"title":"Implications of B -> rho gamma measurements in the Standard Model and Supersymmetric Theories","license":"","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Ahmed Ali, Enrico Lunghi","submitted_at":"2002-06-25T18:09:08Z","abstract_excerpt":"We study the implications of the recently improved upper limits on the branching ratios for the decays B -> rho gamma, expressed as R(rho gamma/K^* gamma) = BR(B -> rho gamma)/BR(B -> K^* gamma) <0.047. We work out the constraints that the current bound on R(rho gamma/K^* gamma) implies on the parameters of the quark mixing matrix in the standard model (SM). Using the present profile of the unitarity triangle, we predict this ratio to be R(rho gamma/K^* gamma) = 0.023 +/- 0.012. We also work out the correlations involving R(rho gamma/K^* gamma), the isospin-violating ratio Delta (rho gamma), a"},"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/0206242","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"hep-ph","submitted_at":"2002-06-25T18:09:08Z","cross_cats_sorted":[],"title_canon_sha256":"eb34362313536099bcc9135363e234bae9b153920f4d5f864b47803417b33334","abstract_canon_sha256":"c5da2482b621d209a68582f75b95fc31e74a1bddbaf2bec3e22cf2e5b9e69262"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:26:11.093372Z","signature_b64":"/pLPglVdOtspmHfLPUHGwjYVC0QWurZRXpUV+cuQDK8SH4jG+TKfrvl58rQ+HC0+FkNTYFz9ENSvvVs+WoDNBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8196c5e0ec6f445baaeca9197635704135ee755ee5132aed73554ad4ab9b7c3c","last_reissued_at":"2026-05-18T04:26:11.092924Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:26:11.092924Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Implications of B -> rho gamma measurements in the Standard Model and Supersymmetric Theories","license":"","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Ahmed Ali, Enrico Lunghi","submitted_at":"2002-06-25T18:09:08Z","abstract_excerpt":"We study the implications of the recently improved upper limits on the branching ratios for the decays B -> rho gamma, expressed as R(rho gamma/K^* gamma) = BR(B -> rho gamma)/BR(B -> K^* gamma) <0.047. We work out the constraints that the current bound on R(rho gamma/K^* gamma) implies on the parameters of the quark mixing matrix in the standard model (SM). Using the present profile of the unitarity triangle, we predict this ratio to be R(rho gamma/K^* gamma) = 0.023 +/- 0.012. We also work out the correlations involving R(rho gamma/K^* gamma), the isospin-violating ratio Delta (rho gamma), a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-ph/0206242","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":"hep-ph/0206242","created_at":"2026-05-18T04:26:11.092985+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-ph/0206242v2","created_at":"2026-05-18T04:26:11.092985+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-ph/0206242","created_at":"2026-05-18T04:26:11.092985+00:00"},{"alias_kind":"pith_short_12","alias_value":"QGLMLYHMN5CF","created_at":"2026-05-18T12:25:51.375804+00:00"},{"alias_kind":"pith_short_16","alias_value":"QGLMLYHMN5CFXKXM","created_at":"2026-05-18T12:25:51.375804+00:00"},{"alias_kind":"pith_short_8","alias_value":"QGLMLYHM","created_at":"2026-05-18T12:25:51.375804+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2601.03083","citing_title":"First evidence of the $B_s^0\\rightarrow K^-\\pi^+\\gamma$ decay","ref_index":3,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/QGLMLYHMN5CFXKXMVEMXMNLQIE","json":"https://pith.science/pith/QGLMLYHMN5CFXKXMVEMXMNLQIE.json","graph_json":"https://pith.science/api/pith-number/QGLMLYHMN5CFXKXMVEMXMNLQIE/graph.json","events_json":"https://pith.science/api/pith-number/QGLMLYHMN5CFXKXMVEMXMNLQIE/events.json","paper":"https://pith.science/paper/QGLMLYHM"},"agent_actions":{"view_html":"https://pith.science/pith/QGLMLYHMN5CFXKXMVEMXMNLQIE","download_json":"https://pith.science/pith/QGLMLYHMN5CFXKXMVEMXMNLQIE.json","view_paper":"https://pith.science/paper/QGLMLYHM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-ph/0206242&json=true","fetch_graph":"https://pith.science/api/pith-number/QGLMLYHMN5CFXKXMVEMXMNLQIE/graph.json","fetch_events":"https://pith.science/api/pith-number/QGLMLYHMN5CFXKXMVEMXMNLQIE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QGLMLYHMN5CFXKXMVEMXMNLQIE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QGLMLYHMN5CFXKXMVEMXMNLQIE/action/storage_attestation","attest_author":"https://pith.science/pith/QGLMLYHMN5CFXKXMVEMXMNLQIE/action/author_attestation","sign_citation":"https://pith.science/pith/QGLMLYHMN5CFXKXMVEMXMNLQIE/action/citation_signature","submit_replication":"https://pith.science/pith/QGLMLYHMN5CFXKXMVEMXMNLQIE/action/replication_record"}},"created_at":"2026-05-18T04:26:11.092985+00:00","updated_at":"2026-05-18T04:26:11.092985+00:00"}