{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1994:F4IRUM7JA6D4HVF23PJKYT5IYS","short_pith_number":"pith:F4IRUM7J","schema_version":"1.0","canonical_sha256":"2f111a33e90787c3d4badbd2ac4fa8c49e49c47dd001f0f624b1eff6509fd626","source":{"kind":"arxiv","id":"hep-ph/9411311","version":1},"attestation_state":"computed","paper":{"title":"Semileptonic Kaon Decays","license":"","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"G. Colangelo, G. Ecker, J. Bijnens, J. Gasser","submitted_at":"1994-11-16T11:47:58Z","abstract_excerpt":"We present the matrix elements for the semileptonic kaon decays $K_{l2\\gamma}$ , $K_{l2l^+l^-}$, $K_{l2l'^+l'^-}$,$K_{l3}$, $K_{l3\\gamma}$ and $K_{l4}$ at next-to-leading order, and $K_{e5}$ at leading order in Chiral Perturbation Theory and compare the predictions with experimental data. For $K_{l4}$ decays we estimate yet higher orders in order to reduce theoretical uncertainties in the comparison with the data. Monte Carlo event generators are used to calculate the corresponding rates at DA$\\Phi$NE. We discuss the possibilities to improve our knowledge of the low-energy structure of the Sta"},"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/9411311","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"hep-ph","submitted_at":"1994-11-16T11:47:58Z","cross_cats_sorted":[],"title_canon_sha256":"13e6f413bebc57ae69c186f35b304ef748ee9f47a93cf37c5b8312dca026057b","abstract_canon_sha256":"d54974f7ae7bfc3b6f32f0df1fddf6ac60674b99528c5d28ffeadd5ac0466c2c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:50:50.178946Z","signature_b64":"PJznPP2LyeX/DAVmCcF/RCpjtZOhawDEKp0xV3rFrZnoHXR2x/WG3gwAImj4RjYN7hVCuIubWBcT+Kkc8XsXAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2f111a33e90787c3d4badbd2ac4fa8c49e49c47dd001f0f624b1eff6509fd626","last_reissued_at":"2026-07-04T15:50:50.178533Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:50:50.178533Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Semileptonic Kaon Decays","license":"","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"G. Colangelo, G. Ecker, J. Bijnens, J. Gasser","submitted_at":"1994-11-16T11:47:58Z","abstract_excerpt":"We present the matrix elements for the semileptonic kaon decays $K_{l2\\gamma}$ , $K_{l2l^+l^-}$, $K_{l2l'^+l'^-}$,$K_{l3}$, $K_{l3\\gamma}$ and $K_{l4}$ at next-to-leading order, and $K_{e5}$ at leading order in Chiral Perturbation Theory and compare the predictions with experimental data. For $K_{l4}$ decays we estimate yet higher orders in order to reduce theoretical uncertainties in the comparison with the data. Monte Carlo event generators are used to calculate the corresponding rates at DA$\\Phi$NE. We discuss the possibilities to improve our knowledge of the low-energy structure of the Sta"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-ph/9411311","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/hep-ph/9411311/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":"hep-ph/9411311","created_at":"2026-07-04T15:50:50.178598+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-ph/9411311v1","created_at":"2026-07-04T15:50:50.178598+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-ph/9411311","created_at":"2026-07-04T15:50:50.178598+00:00"},{"alias_kind":"pith_short_12","alias_value":"F4IRUM7JA6D4","created_at":"2026-07-04T15:50:50.178598+00:00"},{"alias_kind":"pith_short_16","alias_value":"F4IRUM7JA6D4HVF2","created_at":"2026-07-04T15:50:50.178598+00:00"},{"alias_kind":"pith_short_8","alias_value":"F4IRUM7J","created_at":"2026-07-04T15:50:50.178598+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.27521","citing_title":"From WIMP to FIMP during reheating: collider vs non-collider probes for p-wave annihilation","ref_index":164,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/F4IRUM7JA6D4HVF23PJKYT5IYS","json":"https://pith.science/pith/F4IRUM7JA6D4HVF23PJKYT5IYS.json","graph_json":"https://pith.science/api/pith-number/F4IRUM7JA6D4HVF23PJKYT5IYS/graph.json","events_json":"https://pith.science/api/pith-number/F4IRUM7JA6D4HVF23PJKYT5IYS/events.json","paper":"https://pith.science/paper/F4IRUM7J"},"agent_actions":{"view_html":"https://pith.science/pith/F4IRUM7JA6D4HVF23PJKYT5IYS","download_json":"https://pith.science/pith/F4IRUM7JA6D4HVF23PJKYT5IYS.json","view_paper":"https://pith.science/paper/F4IRUM7J","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-ph/9411311&json=true","fetch_graph":"https://pith.science/api/pith-number/F4IRUM7JA6D4HVF23PJKYT5IYS/graph.json","fetch_events":"https://pith.science/api/pith-number/F4IRUM7JA6D4HVF23PJKYT5IYS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/F4IRUM7JA6D4HVF23PJKYT5IYS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/F4IRUM7JA6D4HVF23PJKYT5IYS/action/storage_attestation","attest_author":"https://pith.science/pith/F4IRUM7JA6D4HVF23PJKYT5IYS/action/author_attestation","sign_citation":"https://pith.science/pith/F4IRUM7JA6D4HVF23PJKYT5IYS/action/citation_signature","submit_replication":"https://pith.science/pith/F4IRUM7JA6D4HVF23PJKYT5IYS/action/replication_record"}},"created_at":"2026-07-04T15:50:50.178598+00:00","updated_at":"2026-07-04T15:50:50.178598+00:00"}