{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:QZCCYWJVRHBO73ZOH62GRGNL36","short_pith_number":"pith:QZCCYWJV","schema_version":"1.0","canonical_sha256":"86442c593589c2efef2e3fb46899abdfb25f978e57b5e010e61528ce5c5ef9a9","source":{"kind":"arxiv","id":"1105.0583","version":1},"attestation_state":"computed","paper":{"title":"Spectroscopy and Regge trajectories of heavy baryons in the relativistic quark-diquark picture","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"hep-ph","authors_text":"D. Ebert, R. N. Faustov, V. O. Galkin","submitted_at":"2011-05-03T13:46:04Z","abstract_excerpt":"Mass spectra of heavy baryons are calculated in the heavy-quark--light-diquark picture in the framework of the QCD-motivated relativistic quark model. The dynamics of light quarks in the diquark as well as the dynamics of the heavy quark and light diquark in the baryon are treated completely relativistically without application of nonrelativistic v/c and heavy quark 1/m_Q expansions. Such approach allows us to get predictions for the heavy baryon masses for rather high orbital and radial excitations. On this basis the Regge trajectories of heavy baryons for orbital and radial excitations are c"},"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":"1105.0583","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2011-05-03T13:46:04Z","cross_cats_sorted":["hep-ex"],"title_canon_sha256":"fd344f14bba106b4ec281d87045931d91cc0d3fce796b8e42fd6deb14c784c62","abstract_canon_sha256":"12c74853e3e1b5518132ce4f2e644022d6ea1306cac20d03be038ac6e23e0633"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:16:01.634162Z","signature_b64":"tWWb6mt3Ea8OBo3EacA6LbAGF4lBx7BF20M812C1VPFUTkxxdlrEVJd+enrC5gzDFnJL55Htzs8xeDnTjuEhDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"86442c593589c2efef2e3fb46899abdfb25f978e57b5e010e61528ce5c5ef9a9","last_reissued_at":"2026-05-18T04:16:01.633644Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:16:01.633644Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Spectroscopy and Regge trajectories of heavy baryons in the relativistic quark-diquark picture","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"hep-ph","authors_text":"D. Ebert, R. N. Faustov, V. O. Galkin","submitted_at":"2011-05-03T13:46:04Z","abstract_excerpt":"Mass spectra of heavy baryons are calculated in the heavy-quark--light-diquark picture in the framework of the QCD-motivated relativistic quark model. The dynamics of light quarks in the diquark as well as the dynamics of the heavy quark and light diquark in the baryon are treated completely relativistically without application of nonrelativistic v/c and heavy quark 1/m_Q expansions. Such approach allows us to get predictions for the heavy baryon masses for rather high orbital and radial excitations. On this basis the Regge trajectories of heavy baryons for orbital and radial excitations are c"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1105.0583","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":"1105.0583","created_at":"2026-05-18T04:16:01.633726+00:00"},{"alias_kind":"arxiv_version","alias_value":"1105.0583v1","created_at":"2026-05-18T04:16:01.633726+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1105.0583","created_at":"2026-05-18T04:16:01.633726+00:00"},{"alias_kind":"pith_short_12","alias_value":"QZCCYWJVRHBO","created_at":"2026-05-18T12:26:39.201973+00:00"},{"alias_kind":"pith_short_16","alias_value":"QZCCYWJVRHBO73ZO","created_at":"2026-05-18T12:26:39.201973+00:00"},{"alias_kind":"pith_short_8","alias_value":"QZCCYWJV","created_at":"2026-05-18T12:26:39.201973+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2605.17322","citing_title":"Investigating the mass spectra of $1F$-wave singly heavy $\\Sigma_{Q}$, $\\Xi^{\\prime}_{Q}$, and $\\Omega_{Q}$ baryons","ref_index":38,"is_internal_anchor":true},{"citing_arxiv_id":"2603.01037","citing_title":"Quark-diquark effective mass formalism for heavy baryon spectroscopy","ref_index":42,"is_internal_anchor":true},{"citing_arxiv_id":"2604.18796","citing_title":"Mass spectrum, magnetic moments and Regge trajectories of $\\Omega_{ccb}$ and $\\Omega_{cbb}$ baryons in the nonrelativistic quark--diquark model","ref_index":79,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/QZCCYWJVRHBO73ZOH62GRGNL36","json":"https://pith.science/pith/QZCCYWJVRHBO73ZOH62GRGNL36.json","graph_json":"https://pith.science/api/pith-number/QZCCYWJVRHBO73ZOH62GRGNL36/graph.json","events_json":"https://pith.science/api/pith-number/QZCCYWJVRHBO73ZOH62GRGNL36/events.json","paper":"https://pith.science/paper/QZCCYWJV"},"agent_actions":{"view_html":"https://pith.science/pith/QZCCYWJVRHBO73ZOH62GRGNL36","download_json":"https://pith.science/pith/QZCCYWJVRHBO73ZOH62GRGNL36.json","view_paper":"https://pith.science/paper/QZCCYWJV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1105.0583&json=true","fetch_graph":"https://pith.science/api/pith-number/QZCCYWJVRHBO73ZOH62GRGNL36/graph.json","fetch_events":"https://pith.science/api/pith-number/QZCCYWJVRHBO73ZOH62GRGNL36/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QZCCYWJVRHBO73ZOH62GRGNL36/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QZCCYWJVRHBO73ZOH62GRGNL36/action/storage_attestation","attest_author":"https://pith.science/pith/QZCCYWJVRHBO73ZOH62GRGNL36/action/author_attestation","sign_citation":"https://pith.science/pith/QZCCYWJVRHBO73ZOH62GRGNL36/action/citation_signature","submit_replication":"https://pith.science/pith/QZCCYWJVRHBO73ZOH62GRGNL36/action/replication_record"}},"created_at":"2026-05-18T04:16:01.633726+00:00","updated_at":"2026-05-18T04:16:01.633726+00:00"}