{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1995:5WBMZFFQ5AQUZFZXWWKDUFCYPI","short_pith_number":"pith:5WBMZFFQ","schema_version":"1.0","canonical_sha256":"ed82cc94b0e8214c9737b5943a14587a31b2da3c00314dff0034cbeb38ca07e0","source":{"kind":"arxiv","id":"hep-ph/9507300","version":1},"attestation_state":"computed","paper":{"title":"Three-body relativistic flux tube model from QCD Wilson-loop approach","license":"","headline":"","cross_cats":["hep-th"],"primary_cat":"hep-ph","authors_text":"A. Vairo, G. M. Prosperi, N. Brambilla","submitted_at":"1995-07-13T12:06:42Z","abstract_excerpt":"First we review the derivation of the relativistic flux tube model for a quark-antiquark system from Wilson area law as we have given in a preceding paper. Then we extend the method to the three-quark case and obtain a Lagrangian corresponding to a star flux tube configuration.\n  A Hamiltonian can be explicitly constructed as an expansion in $1 / m^2$ or in the string tension $\\sigma$. In the first case it reproduces the Wilson loop three-quark semirelativistic potential; in the second one, very complicated in general, but it reproduces known string models for slowly rotating quarks."},"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/9507300","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"hep-ph","submitted_at":"1995-07-13T12:06:42Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"d3c6752b44aa702d286d2cec6444c07a8285661a9dc25125a16a8d4625d3c89c","abstract_canon_sha256":"cb91137e2842e536e2298872f4fae1438ea99f8fab67e7b38a85ca22184fa0a0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:06:30.132586Z","signature_b64":"5Af4CjKnnycZE/mj8Q+AqG9HQLIW1pTmaydI8iu2RA7ZZ1Q9okx6ZY+4MJEZbInOi8oWL8hwJ8QAnWlyZvPvCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ed82cc94b0e8214c9737b5943a14587a31b2da3c00314dff0034cbeb38ca07e0","last_reissued_at":"2026-05-18T01:06:30.131937Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:06:30.131937Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Three-body relativistic flux tube model from QCD Wilson-loop approach","license":"","headline":"","cross_cats":["hep-th"],"primary_cat":"hep-ph","authors_text":"A. Vairo, G. M. Prosperi, N. Brambilla","submitted_at":"1995-07-13T12:06:42Z","abstract_excerpt":"First we review the derivation of the relativistic flux tube model for a quark-antiquark system from Wilson area law as we have given in a preceding paper. Then we extend the method to the three-quark case and obtain a Lagrangian corresponding to a star flux tube configuration.\n  A Hamiltonian can be explicitly constructed as an expansion in $1 / m^2$ or in the string tension $\\sigma$. In the first case it reproduces the Wilson loop three-quark semirelativistic potential; in the second one, very complicated in general, but it reproduces known string models for slowly rotating quarks."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-ph/9507300","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":"hep-ph/9507300","created_at":"2026-05-18T01:06:30.132032+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-ph/9507300v1","created_at":"2026-05-18T01:06:30.132032+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-ph/9507300","created_at":"2026-05-18T01:06:30.132032+00:00"},{"alias_kind":"pith_short_12","alias_value":"5WBMZFFQ5AQU","created_at":"2026-05-18T12:25:47.102015+00:00"},{"alias_kind":"pith_short_16","alias_value":"5WBMZFFQ5AQUZFZX","created_at":"2026-05-18T12:25:47.102015+00:00"},{"alias_kind":"pith_short_8","alias_value":"5WBMZFFQ","created_at":"2026-05-18T12:25:47.102015+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/5WBMZFFQ5AQUZFZXWWKDUFCYPI","json":"https://pith.science/pith/5WBMZFFQ5AQUZFZXWWKDUFCYPI.json","graph_json":"https://pith.science/api/pith-number/5WBMZFFQ5AQUZFZXWWKDUFCYPI/graph.json","events_json":"https://pith.science/api/pith-number/5WBMZFFQ5AQUZFZXWWKDUFCYPI/events.json","paper":"https://pith.science/paper/5WBMZFFQ"},"agent_actions":{"view_html":"https://pith.science/pith/5WBMZFFQ5AQUZFZXWWKDUFCYPI","download_json":"https://pith.science/pith/5WBMZFFQ5AQUZFZXWWKDUFCYPI.json","view_paper":"https://pith.science/paper/5WBMZFFQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-ph/9507300&json=true","fetch_graph":"https://pith.science/api/pith-number/5WBMZFFQ5AQUZFZXWWKDUFCYPI/graph.json","fetch_events":"https://pith.science/api/pith-number/5WBMZFFQ5AQUZFZXWWKDUFCYPI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5WBMZFFQ5AQUZFZXWWKDUFCYPI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5WBMZFFQ5AQUZFZXWWKDUFCYPI/action/storage_attestation","attest_author":"https://pith.science/pith/5WBMZFFQ5AQUZFZXWWKDUFCYPI/action/author_attestation","sign_citation":"https://pith.science/pith/5WBMZFFQ5AQUZFZXWWKDUFCYPI/action/citation_signature","submit_replication":"https://pith.science/pith/5WBMZFFQ5AQUZFZXWWKDUFCYPI/action/replication_record"}},"created_at":"2026-05-18T01:06:30.132032+00:00","updated_at":"2026-05-18T01:06:30.132032+00:00"}