{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:JFAVWNA2I577MHDVKDKQJ5AV66","short_pith_number":"pith:JFAVWNA2","schema_version":"1.0","canonical_sha256":"49415b341a477ff61c7550d504f415f7a93c40ae0873052f496940b2e1566430","source":{"kind":"arxiv","id":"1012.4671","version":1},"attestation_state":"computed","paper":{"title":"Light Cone Sum Rules for the pi0-gamma*-gamma Form Factor Revisited","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"hep-ph","authors_text":"F.A. Porkert, N. Offen, S.S. Agaev, V.M. Braun","submitted_at":"2010-12-21T14:29:38Z","abstract_excerpt":"We provide a theoretical update of the calculations of the pi0-gamma*-gamma form factor in the LCSR framework, including up to six polynomials in the conformal expansion of the pion distribution amplitude and taking into account twist-six corrections related to the photon emission at large distances. The results are compared with the calculations of the B-> pi l nu decay and pion electromagnetic form factors in the same framework. Our conclusion is that the recent BaBar measurements of the pi0-gamma*-gamma form factor at large momentum transfers are consistent with QCD, although they do sugges"},"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":"1012.4671","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2010-12-21T14:29:38Z","cross_cats_sorted":["hep-ex"],"title_canon_sha256":"a8dcbbd5efd705bf28d8d20dfdc03820ba2c58686e484edd9dbf19d2c22bbba9","abstract_canon_sha256":"4f50d670909834c1b87bec754767e8b759104f23e971f34d2afe1ab1d2012f68"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:26:22.727838Z","signature_b64":"0Q1xzqy1cHePfAIpy9ydu5l/6okbbnGfFS/gjAGylkU+0UkkRqrSSmlBcl2CS+HSjDVibi/zwiUZSDmwVKbvCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"49415b341a477ff61c7550d504f415f7a93c40ae0873052f496940b2e1566430","last_reissued_at":"2026-05-18T04:26:22.727406Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:26:22.727406Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Light Cone Sum Rules for the pi0-gamma*-gamma Form Factor Revisited","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"hep-ph","authors_text":"F.A. Porkert, N. Offen, S.S. Agaev, V.M. Braun","submitted_at":"2010-12-21T14:29:38Z","abstract_excerpt":"We provide a theoretical update of the calculations of the pi0-gamma*-gamma form factor in the LCSR framework, including up to six polynomials in the conformal expansion of the pion distribution amplitude and taking into account twist-six corrections related to the photon emission at large distances. The results are compared with the calculations of the B-> pi l nu decay and pion electromagnetic form factors in the same framework. Our conclusion is that the recent BaBar measurements of the pi0-gamma*-gamma form factor at large momentum transfers are consistent with QCD, although they do sugges"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1012.4671","kind":"arxiv","version":1},"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":"1012.4671","created_at":"2026-05-18T04:26:22.727473+00:00"},{"alias_kind":"arxiv_version","alias_value":"1012.4671v1","created_at":"2026-05-18T04:26:22.727473+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1012.4671","created_at":"2026-05-18T04:26:22.727473+00:00"},{"alias_kind":"pith_short_12","alias_value":"JFAVWNA2I577","created_at":"2026-05-18T12:26:09.077623+00:00"},{"alias_kind":"pith_short_16","alias_value":"JFAVWNA2I577MHDV","created_at":"2026-05-18T12:26:09.077623+00:00"},{"alias_kind":"pith_short_8","alias_value":"JFAVWNA2","created_at":"2026-05-18T12:26:09.077623+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2510.00378","citing_title":"$\\bar{B}_{s,d}^{0} \\to J/\\psi \\mu^{+}\\mu^{-}$ Decays in QCD Factorization","ref_index":81,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/JFAVWNA2I577MHDVKDKQJ5AV66","json":"https://pith.science/pith/JFAVWNA2I577MHDVKDKQJ5AV66.json","graph_json":"https://pith.science/api/pith-number/JFAVWNA2I577MHDVKDKQJ5AV66/graph.json","events_json":"https://pith.science/api/pith-number/JFAVWNA2I577MHDVKDKQJ5AV66/events.json","paper":"https://pith.science/paper/JFAVWNA2"},"agent_actions":{"view_html":"https://pith.science/pith/JFAVWNA2I577MHDVKDKQJ5AV66","download_json":"https://pith.science/pith/JFAVWNA2I577MHDVKDKQJ5AV66.json","view_paper":"https://pith.science/paper/JFAVWNA2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1012.4671&json=true","fetch_graph":"https://pith.science/api/pith-number/JFAVWNA2I577MHDVKDKQJ5AV66/graph.json","fetch_events":"https://pith.science/api/pith-number/JFAVWNA2I577MHDVKDKQJ5AV66/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JFAVWNA2I577MHDVKDKQJ5AV66/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JFAVWNA2I577MHDVKDKQJ5AV66/action/storage_attestation","attest_author":"https://pith.science/pith/JFAVWNA2I577MHDVKDKQJ5AV66/action/author_attestation","sign_citation":"https://pith.science/pith/JFAVWNA2I577MHDVKDKQJ5AV66/action/citation_signature","submit_replication":"https://pith.science/pith/JFAVWNA2I577MHDVKDKQJ5AV66/action/replication_record"}},"created_at":"2026-05-18T04:26:22.727473+00:00","updated_at":"2026-05-18T04:26:22.727473+00:00"}