{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:NJPSICLQXFHEAE7RYBIW23GNDB","short_pith_number":"pith:NJPSICLQ","schema_version":"1.0","canonical_sha256":"6a5f240970b94e4013f1c0516d6ccd187cade4b65c02e622a54f156aadd68dd6","source":{"kind":"arxiv","id":"2405.03975","version":2},"attestation_state":"computed","paper":{"title":"Baryonic thermal screening mass at NLO","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-lat"],"primary_cat":"hep-ph","authors_text":"Davide Laudicina, Leonardo Giusti, Michele Pepe, M. Laine, Pietro Rescigno","submitted_at":"2024-05-07T03:18:47Z","abstract_excerpt":"We determine the resummed 1-loop correction to a baryonic thermal screening mass. The calculation is carried out in the framework of a dimensionally reduced effective theory, where quarks are heavy fields due to their non-zero Matsubara frequencies. The correction due to interactions is computed at O($g^2_{ }$) in the coupling constant. In order to solve a 3-body Schr\\\"odinger equation, we exploit a two-dimensional generalization of the hyperspherical harmonics method. At electroweak scale temperatures, the NLO correction represents a $\\sim 4.6 \\%$ increase of the free-theory value $3\\pi T$ of"},"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":"2405.03975","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2024-05-07T03:18:47Z","cross_cats_sorted":["hep-lat"],"title_canon_sha256":"f44151941ef45f10217bd6bde7858f7319e79c8718a16a7deb37f160714aa2f8","abstract_canon_sha256":"80c6a26e2d847fe5ac0d23bcb6741e8aee7ed8137f28fbd096fad32b61099f90"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:40:17.363237Z","signature_b64":"eqzC3dB0tJP94C/KEsTSnMGSg7wxp7K33miwi7k5X8gzh38JJ36VieshdimKWevGeulM3gUmbE8CF6ivDrLPDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6a5f240970b94e4013f1c0516d6ccd187cade4b65c02e622a54f156aadd68dd6","last_reissued_at":"2026-07-05T08:40:17.362693Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:40:17.362693Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Baryonic thermal screening mass at NLO","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-lat"],"primary_cat":"hep-ph","authors_text":"Davide Laudicina, Leonardo Giusti, Michele Pepe, M. Laine, Pietro Rescigno","submitted_at":"2024-05-07T03:18:47Z","abstract_excerpt":"We determine the resummed 1-loop correction to a baryonic thermal screening mass. The calculation is carried out in the framework of a dimensionally reduced effective theory, where quarks are heavy fields due to their non-zero Matsubara frequencies. The correction due to interactions is computed at O($g^2_{ }$) in the coupling constant. In order to solve a 3-body Schr\\\"odinger equation, we exploit a two-dimensional generalization of the hyperspherical harmonics method. At electroweak scale temperatures, the NLO correction represents a $\\sim 4.6 \\%$ increase of the free-theory value $3\\pi T$ of"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2405.03975","kind":"arxiv","version":2},"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/2405.03975/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":"2405.03975","created_at":"2026-07-05T08:40:17.362778+00:00"},{"alias_kind":"arxiv_version","alias_value":"2405.03975v2","created_at":"2026-07-05T08:40:17.362778+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2405.03975","created_at":"2026-07-05T08:40:17.362778+00:00"},{"alias_kind":"pith_short_12","alias_value":"NJPSICLQXFHE","created_at":"2026-07-05T08:40:17.362778+00:00"},{"alias_kind":"pith_short_16","alias_value":"NJPSICLQXFHEAE7R","created_at":"2026-07-05T08:40:17.362778+00:00"},{"alias_kind":"pith_short_8","alias_value":"NJPSICLQ","created_at":"2026-07-05T08:40:17.362778+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2411.14127","citing_title":"Non-perturbative thermal QCD at very high temperatures: computational strategy and hadronic screening masses","ref_index":10,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/NJPSICLQXFHEAE7RYBIW23GNDB","json":"https://pith.science/pith/NJPSICLQXFHEAE7RYBIW23GNDB.json","graph_json":"https://pith.science/api/pith-number/NJPSICLQXFHEAE7RYBIW23GNDB/graph.json","events_json":"https://pith.science/api/pith-number/NJPSICLQXFHEAE7RYBIW23GNDB/events.json","paper":"https://pith.science/paper/NJPSICLQ"},"agent_actions":{"view_html":"https://pith.science/pith/NJPSICLQXFHEAE7RYBIW23GNDB","download_json":"https://pith.science/pith/NJPSICLQXFHEAE7RYBIW23GNDB.json","view_paper":"https://pith.science/paper/NJPSICLQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2405.03975&json=true","fetch_graph":"https://pith.science/api/pith-number/NJPSICLQXFHEAE7RYBIW23GNDB/graph.json","fetch_events":"https://pith.science/api/pith-number/NJPSICLQXFHEAE7RYBIW23GNDB/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NJPSICLQXFHEAE7RYBIW23GNDB/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NJPSICLQXFHEAE7RYBIW23GNDB/action/storage_attestation","attest_author":"https://pith.science/pith/NJPSICLQXFHEAE7RYBIW23GNDB/action/author_attestation","sign_citation":"https://pith.science/pith/NJPSICLQXFHEAE7RYBIW23GNDB/action/citation_signature","submit_replication":"https://pith.science/pith/NJPSICLQXFHEAE7RYBIW23GNDB/action/replication_record"}},"created_at":"2026-07-05T08:40:17.362778+00:00","updated_at":"2026-07-05T08:40:17.362778+00:00"}