{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2004:UMYJJGMOQEC6LD6WENW5TTHDVM","short_pith_number":"pith:UMYJJGMO","schema_version":"1.0","canonical_sha256":"a33094998e8105e58fd6236dd9cce3ab3532b9af2a370075c9a9a98c19d6512f","source":{"kind":"arxiv","id":"hep-ph/0412210","version":3},"attestation_state":"computed","paper":{"title":"Chiral radiative corrections and D_s(2317)/D(2308) mass puzzle","license":"","headline":"","cross_cats":["hep-ex"],"primary_cat":"hep-ph","authors_text":"Byung-Yoon Park, D.P. Min, Ian Woo Lee, Taekoon Lee","submitted_at":"2004-12-15T11:55:44Z","abstract_excerpt":"We show that one loop chiral corrections for heavy-light mesons in potential model can explain the small mass of D_s(2317) as well as the small mass gap between D_s(2317) and D(2308)."},"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/0412210","kind":"arxiv","version":3},"metadata":{"license":"","primary_cat":"hep-ph","submitted_at":"2004-12-15T11:55:44Z","cross_cats_sorted":["hep-ex"],"title_canon_sha256":"b966d269db8a5a668ec5bc63277ebd1d0cc1c48d82d53f4aefc6529e74cd7232","abstract_canon_sha256":"7d520423cf9fd7a93270f7f75cfc63e6eed158690e1e2ef2bcc03bc85fb4bafd"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:38:36.504725Z","signature_b64":"IO7+Sq7e304dMY9Z5rU4rfey/gNsSSuluL9WOOp7QMjy/+RXnnKrKNkYY/wbbtl111YqclpnzHMF8MKUSLT4Cw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a33094998e8105e58fd6236dd9cce3ab3532b9af2a370075c9a9a98c19d6512f","last_reissued_at":"2026-05-18T04:38:36.504068Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:38:36.504068Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Chiral radiative corrections and D_s(2317)/D(2308) mass puzzle","license":"","headline":"","cross_cats":["hep-ex"],"primary_cat":"hep-ph","authors_text":"Byung-Yoon Park, D.P. Min, Ian Woo Lee, Taekoon Lee","submitted_at":"2004-12-15T11:55:44Z","abstract_excerpt":"We show that one loop chiral corrections for heavy-light mesons in potential model can explain the small mass of D_s(2317) as well as the small mass gap between D_s(2317) and D(2308)."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-ph/0412210","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":"hep-ph/0412210","created_at":"2026-05-18T04:38:36.504179+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-ph/0412210v3","created_at":"2026-05-18T04:38:36.504179+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-ph/0412210","created_at":"2026-05-18T04:38:36.504179+00:00"},{"alias_kind":"pith_short_12","alias_value":"UMYJJGMOQEC6","created_at":"2026-05-18T12:25:52.687210+00:00"},{"alias_kind":"pith_short_16","alias_value":"UMYJJGMOQEC6LD6W","created_at":"2026-05-18T12:25:52.687210+00:00"},{"alias_kind":"pith_short_8","alias_value":"UMYJJGMO","created_at":"2026-05-18T12:25:52.687210+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2608.01272","citing_title":"Properties of the $D_{s0}^*(2317)^\\pm$ in hot and dense nuclear matter","ref_index":19,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/UMYJJGMOQEC6LD6WENW5TTHDVM","json":"https://pith.science/pith/UMYJJGMOQEC6LD6WENW5TTHDVM.json","graph_json":"https://pith.science/api/pith-number/UMYJJGMOQEC6LD6WENW5TTHDVM/graph.json","events_json":"https://pith.science/api/pith-number/UMYJJGMOQEC6LD6WENW5TTHDVM/events.json","paper":"https://pith.science/paper/UMYJJGMO"},"agent_actions":{"view_html":"https://pith.science/pith/UMYJJGMOQEC6LD6WENW5TTHDVM","download_json":"https://pith.science/pith/UMYJJGMOQEC6LD6WENW5TTHDVM.json","view_paper":"https://pith.science/paper/UMYJJGMO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-ph/0412210&json=true","fetch_graph":"https://pith.science/api/pith-number/UMYJJGMOQEC6LD6WENW5TTHDVM/graph.json","fetch_events":"https://pith.science/api/pith-number/UMYJJGMOQEC6LD6WENW5TTHDVM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UMYJJGMOQEC6LD6WENW5TTHDVM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UMYJJGMOQEC6LD6WENW5TTHDVM/action/storage_attestation","attest_author":"https://pith.science/pith/UMYJJGMOQEC6LD6WENW5TTHDVM/action/author_attestation","sign_citation":"https://pith.science/pith/UMYJJGMOQEC6LD6WENW5TTHDVM/action/citation_signature","submit_replication":"https://pith.science/pith/UMYJJGMOQEC6LD6WENW5TTHDVM/action/replication_record"}},"created_at":"2026-05-18T04:38:36.504179+00:00","updated_at":"2026-05-18T04:38:36.504179+00:00"}