{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:A3BILZB25H36MWYT5MCIYHC7MT","short_pith_number":"pith:A3BILZB2","schema_version":"1.0","canonical_sha256":"06c285e43ae9f7e65b13eb048c1c5f64e8aa91e8e330255ba3abf26768e1d61a","source":{"kind":"arxiv","id":"2503.14291","version":1},"attestation_state":"computed","paper":{"title":"The infrared-safe Minkowskian Curci-Ferrari model","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"hep-ph","authors_text":"Marcela Pel\\'aez, Santiago Oribe, Urko Reinosa","submitted_at":"2025-03-18T14:31:49Z","abstract_excerpt":"We discuss the existence of Landau-pole-free renormalization group trajectories in the Minkowskian version of the Curci-Ferrari model as a function of a running parameter $q^2$ associated to the four-vector $q$ at which renormalization conditions are imposed, and which can take both space-like ($\\smash{q^2<0}$) and time-like ($\\smash{q^2>0}$) values. We discuss two possible extensions of the infrared-safe scheme defined in Ref. [Phys. Rev. D, 84, 045018, 2011] for the Euclidean version of the model, which coincide with the latter in the space-like region upon identifying $\\smash{Q^2\\equiv-q^2}"},"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":"2503.14291","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2025-03-18T14:31:49Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"932c4f75f6aa0c1494728d6fff888be8f4a58f4aba27d63cc0ef603d7816babb","abstract_canon_sha256":"130faad615c2ec480c159ff2afd785e1385925eae7d6d8e7ade8d0d74acc474f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:33:59.452579Z","signature_b64":"w/fQGitOvW5EG9MFQX3NSq5qIZM20NJJ8NaeegFhfE74sp/85jiFUDNKAfe7OcHN/fGuhnr31SKI+q+wDCI4CA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"06c285e43ae9f7e65b13eb048c1c5f64e8aa91e8e330255ba3abf26768e1d61a","last_reissued_at":"2026-07-05T10:33:59.452084Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:33:59.452084Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The infrared-safe Minkowskian Curci-Ferrari model","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"hep-ph","authors_text":"Marcela Pel\\'aez, Santiago Oribe, Urko Reinosa","submitted_at":"2025-03-18T14:31:49Z","abstract_excerpt":"We discuss the existence of Landau-pole-free renormalization group trajectories in the Minkowskian version of the Curci-Ferrari model as a function of a running parameter $q^2$ associated to the four-vector $q$ at which renormalization conditions are imposed, and which can take both space-like ($\\smash{q^2<0}$) and time-like ($\\smash{q^2>0}$) values. We discuss two possible extensions of the infrared-safe scheme defined in Ref. [Phys. Rev. D, 84, 045018, 2011] for the Euclidean version of the model, which coincide with the latter in the space-like region upon identifying $\\smash{Q^2\\equiv-q^2}"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2503.14291","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/2503.14291/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":"2503.14291","created_at":"2026-07-05T10:33:59.452146+00:00"},{"alias_kind":"arxiv_version","alias_value":"2503.14291v1","created_at":"2026-07-05T10:33:59.452146+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2503.14291","created_at":"2026-07-05T10:33:59.452146+00:00"},{"alias_kind":"pith_short_12","alias_value":"A3BILZB25H36","created_at":"2026-07-05T10:33:59.452146+00:00"},{"alias_kind":"pith_short_16","alias_value":"A3BILZB25H36MWYT","created_at":"2026-07-05T10:33:59.452146+00:00"},{"alias_kind":"pith_short_8","alias_value":"A3BILZB2","created_at":"2026-07-05T10:33:59.452146+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2509.07256","citing_title":"Non-Abelian Casimir energy in the Curci-Ferrari model through a functional approach","ref_index":36,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/A3BILZB25H36MWYT5MCIYHC7MT","json":"https://pith.science/pith/A3BILZB25H36MWYT5MCIYHC7MT.json","graph_json":"https://pith.science/api/pith-number/A3BILZB25H36MWYT5MCIYHC7MT/graph.json","events_json":"https://pith.science/api/pith-number/A3BILZB25H36MWYT5MCIYHC7MT/events.json","paper":"https://pith.science/paper/A3BILZB2"},"agent_actions":{"view_html":"https://pith.science/pith/A3BILZB25H36MWYT5MCIYHC7MT","download_json":"https://pith.science/pith/A3BILZB25H36MWYT5MCIYHC7MT.json","view_paper":"https://pith.science/paper/A3BILZB2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2503.14291&json=true","fetch_graph":"https://pith.science/api/pith-number/A3BILZB25H36MWYT5MCIYHC7MT/graph.json","fetch_events":"https://pith.science/api/pith-number/A3BILZB25H36MWYT5MCIYHC7MT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/A3BILZB25H36MWYT5MCIYHC7MT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/A3BILZB25H36MWYT5MCIYHC7MT/action/storage_attestation","attest_author":"https://pith.science/pith/A3BILZB25H36MWYT5MCIYHC7MT/action/author_attestation","sign_citation":"https://pith.science/pith/A3BILZB25H36MWYT5MCIYHC7MT/action/citation_signature","submit_replication":"https://pith.science/pith/A3BILZB25H36MWYT5MCIYHC7MT/action/replication_record"}},"created_at":"2026-07-05T10:33:59.452146+00:00","updated_at":"2026-07-05T10:33:59.452146+00:00"}