{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:EQPLNANE6YBYCBTVWO67YYI47S","short_pith_number":"pith:EQPLNANE","schema_version":"1.0","canonical_sha256":"241eb681a4f603810675b3bdfc611cfcbcd92a54b01f4b6078c7c3570650ddc3","source":{"kind":"arxiv","id":"2504.01893","version":1},"attestation_state":"computed","paper":{"title":"A minimal Pati-Salam theory: from cosmic defects to gravitational waves and colliders","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO","hep-ex"],"primary_cat":"hep-ph","authors_text":"Goran Senjanovi\\'c, Michael Zantedeschi","submitted_at":"2025-04-02T16:53:52Z","abstract_excerpt":"We discuss a minimal renormalizable Pati-Salam theory based on the $SU(4)_{\\rm C}\\,\\times\\,SU(2)_{\\rm L}\\,\\times\\,SU(2)_{\\rm R}$ gauge group, with unification scale Higgs multiplets taken as $SU(2)_{\\rm L}$ and $SU(2)_{\\rm R}$ doublets, which lead to neutrino Dirac picture. Although a number of scalar particles could be light, even lying at the LHC energies, the unification scale is hopelessly out of reach in any foreseeable future. Moreover, phase transition in the early Universe leads to the production of magnetic monopoles and domain walls, both incompatible with the standard cosmological m"},"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":"2504.01893","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-ph","submitted_at":"2025-04-02T16:53:52Z","cross_cats_sorted":["astro-ph.CO","hep-ex"],"title_canon_sha256":"e71b3919f60a9f330e7838b264d462bbc3e38518dea7f9daa60d55344c4db6e9","abstract_canon_sha256":"ab6463e9cee58f5b888365d587bcb0df145efc52c092513e1e2bbc4c51b7764b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:43:31.355017Z","signature_b64":"Jha6ROvSAqNzNxu5Y3eyfJrjMTXNAPlo6FqqEIaljjNuv38LROwGjb2JsWOBuqeWKLBEgqhUUA8TPo2wZYCgBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"241eb681a4f603810675b3bdfc611cfcbcd92a54b01f4b6078c7c3570650ddc3","last_reissued_at":"2026-07-05T10:43:31.354546Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:43:31.354546Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A minimal Pati-Salam theory: from cosmic defects to gravitational waves and colliders","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO","hep-ex"],"primary_cat":"hep-ph","authors_text":"Goran Senjanovi\\'c, Michael Zantedeschi","submitted_at":"2025-04-02T16:53:52Z","abstract_excerpt":"We discuss a minimal renormalizable Pati-Salam theory based on the $SU(4)_{\\rm C}\\,\\times\\,SU(2)_{\\rm L}\\,\\times\\,SU(2)_{\\rm R}$ gauge group, with unification scale Higgs multiplets taken as $SU(2)_{\\rm L}$ and $SU(2)_{\\rm R}$ doublets, which lead to neutrino Dirac picture. Although a number of scalar particles could be light, even lying at the LHC energies, the unification scale is hopelessly out of reach in any foreseeable future. Moreover, phase transition in the early Universe leads to the production of magnetic monopoles and domain walls, both incompatible with the standard cosmological m"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2504.01893","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/2504.01893/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":"2504.01893","created_at":"2026-07-05T10:43:31.354602+00:00"},{"alias_kind":"arxiv_version","alias_value":"2504.01893v1","created_at":"2026-07-05T10:43:31.354602+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2504.01893","created_at":"2026-07-05T10:43:31.354602+00:00"},{"alias_kind":"pith_short_12","alias_value":"EQPLNANE6YBY","created_at":"2026-07-05T10:43:31.354602+00:00"},{"alias_kind":"pith_short_16","alias_value":"EQPLNANE6YBYCBTV","created_at":"2026-07-05T10:43:31.354602+00:00"},{"alias_kind":"pith_short_8","alias_value":"EQPLNANE","created_at":"2026-07-05T10:43:31.354602+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.14996","citing_title":"Domain walls and magnetic monopoles in Grand Unified Models","ref_index":16,"is_internal_anchor":false},{"citing_arxiv_id":"2605.21281","citing_title":"Self-Consistent Parker Bound on Magnetic Monopoles","ref_index":20,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/EQPLNANE6YBYCBTVWO67YYI47S","json":"https://pith.science/pith/EQPLNANE6YBYCBTVWO67YYI47S.json","graph_json":"https://pith.science/api/pith-number/EQPLNANE6YBYCBTVWO67YYI47S/graph.json","events_json":"https://pith.science/api/pith-number/EQPLNANE6YBYCBTVWO67YYI47S/events.json","paper":"https://pith.science/paper/EQPLNANE"},"agent_actions":{"view_html":"https://pith.science/pith/EQPLNANE6YBYCBTVWO67YYI47S","download_json":"https://pith.science/pith/EQPLNANE6YBYCBTVWO67YYI47S.json","view_paper":"https://pith.science/paper/EQPLNANE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2504.01893&json=true","fetch_graph":"https://pith.science/api/pith-number/EQPLNANE6YBYCBTVWO67YYI47S/graph.json","fetch_events":"https://pith.science/api/pith-number/EQPLNANE6YBYCBTVWO67YYI47S/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EQPLNANE6YBYCBTVWO67YYI47S/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EQPLNANE6YBYCBTVWO67YYI47S/action/storage_attestation","attest_author":"https://pith.science/pith/EQPLNANE6YBYCBTVWO67YYI47S/action/author_attestation","sign_citation":"https://pith.science/pith/EQPLNANE6YBYCBTVWO67YYI47S/action/citation_signature","submit_replication":"https://pith.science/pith/EQPLNANE6YBYCBTVWO67YYI47S/action/replication_record"}},"created_at":"2026-07-05T10:43:31.354602+00:00","updated_at":"2026-07-05T10:43:31.354602+00:00"}