{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:FGJIQNYAGRBTBOQGCVC4VLFXZA","short_pith_number":"pith:FGJIQNYA","schema_version":"1.0","canonical_sha256":"2992883700344330ba061545caacb7c82799bb9194078e914a4a6bf0d8a4e66a","source":{"kind":"arxiv","id":"2203.09997","version":1},"attestation_state":"computed","paper":{"title":"Semileptonic $B_{s}\\to K_0^*(1430)$ transitions with the light-cone sum rules","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"R. Khosravi","submitted_at":"2022-03-18T14:50:29Z","abstract_excerpt":"In the $\\rm SU(3)_F$ symmetry limit, using two- and three-particle distribution amplitudes of $B^{\\pm}$-meson for $B_s$, the transition form factors of semileptonic $B_{s}\\to K_{0}^*(1430)$ decays are calculated in the framework of the light-cone sum rules. The two-particle distribution amplitudes, $\\varphi_{_{+}}(\\omega)$ and $\\varphi_{_{-}}(\\omega)$ have the most important contribution in estimation of the form factors $f_{+}(q^2)$, $f_{-}(q^2)$ and $f_{T}(q^2)$. The knowledge of the behavior of $\\varphi_{_+}(\\omega)$ is still rather limited. Therefore, we consider three different parametriz"},"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":"2203.09997","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-ph","submitted_at":"2022-03-18T14:50:29Z","cross_cats_sorted":[],"title_canon_sha256":"f24fdd9ac2be2f0cc06cd226f2dca34c384f95bcea716e979f35275fa7e914fa","abstract_canon_sha256":"602486c97dc54afee67afa3bcd031adb9df300d02532b6af28aae82b8dd9e2d6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:36:48.022301Z","signature_b64":"p2gMfQBoLq8Z9/fwyncHRIYNAiUdhlJFDyfBnI5Xkxvm6+dAEKeM5cHc5UwpoU2OPHWBfYc18ehRqfi8nJDcBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2992883700344330ba061545caacb7c82799bb9194078e914a4a6bf0d8a4e66a","last_reissued_at":"2026-07-05T04:36:48.021901Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:36:48.021901Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Semileptonic $B_{s}\\to K_0^*(1430)$ transitions with the light-cone sum rules","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"R. Khosravi","submitted_at":"2022-03-18T14:50:29Z","abstract_excerpt":"In the $\\rm SU(3)_F$ symmetry limit, using two- and three-particle distribution amplitudes of $B^{\\pm}$-meson for $B_s$, the transition form factors of semileptonic $B_{s}\\to K_{0}^*(1430)$ decays are calculated in the framework of the light-cone sum rules. The two-particle distribution amplitudes, $\\varphi_{_{+}}(\\omega)$ and $\\varphi_{_{-}}(\\omega)$ have the most important contribution in estimation of the form factors $f_{+}(q^2)$, $f_{-}(q^2)$ and $f_{T}(q^2)$. The knowledge of the behavior of $\\varphi_{_+}(\\omega)$ is still rather limited. Therefore, we consider three different parametriz"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2203.09997","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/2203.09997/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":"2203.09997","created_at":"2026-07-05T04:36:48.021951+00:00"},{"alias_kind":"arxiv_version","alias_value":"2203.09997v1","created_at":"2026-07-05T04:36:48.021951+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2203.09997","created_at":"2026-07-05T04:36:48.021951+00:00"},{"alias_kind":"pith_short_12","alias_value":"FGJIQNYAGRBT","created_at":"2026-07-05T04:36:48.021951+00:00"},{"alias_kind":"pith_short_16","alias_value":"FGJIQNYAGRBTBOQG","created_at":"2026-07-05T04:36:48.021951+00:00"},{"alias_kind":"pith_short_8","alias_value":"FGJIQNYA","created_at":"2026-07-05T04:36:48.021951+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2501.15121","citing_title":"Study on the Distribution Amplitude of the Scalar Meson $K_0^*(1430)$","ref_index":15,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/FGJIQNYAGRBTBOQGCVC4VLFXZA","json":"https://pith.science/pith/FGJIQNYAGRBTBOQGCVC4VLFXZA.json","graph_json":"https://pith.science/api/pith-number/FGJIQNYAGRBTBOQGCVC4VLFXZA/graph.json","events_json":"https://pith.science/api/pith-number/FGJIQNYAGRBTBOQGCVC4VLFXZA/events.json","paper":"https://pith.science/paper/FGJIQNYA"},"agent_actions":{"view_html":"https://pith.science/pith/FGJIQNYAGRBTBOQGCVC4VLFXZA","download_json":"https://pith.science/pith/FGJIQNYAGRBTBOQGCVC4VLFXZA.json","view_paper":"https://pith.science/paper/FGJIQNYA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2203.09997&json=true","fetch_graph":"https://pith.science/api/pith-number/FGJIQNYAGRBTBOQGCVC4VLFXZA/graph.json","fetch_events":"https://pith.science/api/pith-number/FGJIQNYAGRBTBOQGCVC4VLFXZA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FGJIQNYAGRBTBOQGCVC4VLFXZA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FGJIQNYAGRBTBOQGCVC4VLFXZA/action/storage_attestation","attest_author":"https://pith.science/pith/FGJIQNYAGRBTBOQGCVC4VLFXZA/action/author_attestation","sign_citation":"https://pith.science/pith/FGJIQNYAGRBTBOQGCVC4VLFXZA/action/citation_signature","submit_replication":"https://pith.science/pith/FGJIQNYAGRBTBOQGCVC4VLFXZA/action/replication_record"}},"created_at":"2026-07-05T04:36:48.021951+00:00","updated_at":"2026-07-05T04:36:48.021951+00:00"}