{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:BWQOLXGNTQBVXQ5ZQNIPFKZQW4","short_pith_number":"pith:BWQOLXGN","schema_version":"1.0","canonical_sha256":"0da0e5dccd9c035bc3b98350f2ab30b73b41f355faaef691555e0c6d1f5303a0","source":{"kind":"arxiv","id":"1307.8134","version":2},"attestation_state":"computed","paper":{"title":"WIMP dark matter as radiative neutrino mass messenger","license":"http://creativecommons.org/licenses/by/3.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"J. Palacio, J. W. F. Valle, M. Hirsch, N. Rojas, R. A. Lineros, S. Morisi","submitted_at":"2013-07-30T20:11:08Z","abstract_excerpt":"The minimal seesaw extension of the Standard SU(3) x SU(2) x U(1) Model requires two electroweak singlet fermions in order to accommodate the neutrino oscillation parameters at tree level. Here we consider a next to minimal extension where light neutrino masses are generated radiatively by two electroweak fermions: one singlet and one triplet under SU(2). These should be odd under a parity symmetry and their mixing gives rise to a stable weakly interactive massive particle (WIMP) dark matter candidate. For mass in the GeV-TeV range, it reproduces the correct relic density, and provides an obse"},"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":"1307.8134","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/3.0/","primary_cat":"hep-ph","submitted_at":"2013-07-30T20:11:08Z","cross_cats_sorted":[],"title_canon_sha256":"54c97505e5cc0fa976cab43b369fb07a0832d84a1b1a2e86e8b63db17babd56b","abstract_canon_sha256":"793456b0f389a5c8f73291c80e773b1789b87260008c294dc3bba381ffad4bd3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:08:06.837491Z","signature_b64":"MiKIsReQeFvvIL8doM81gCSmoF6gz2CvnK5Mg/Gc3F5IBIRRCtcEJrMLmRbsUmqpIh7dLV4gXJxntuArgQ+XBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0da0e5dccd9c035bc3b98350f2ab30b73b41f355faaef691555e0c6d1f5303a0","last_reissued_at":"2026-05-18T03:08:06.836657Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:08:06.836657Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"WIMP dark matter as radiative neutrino mass messenger","license":"http://creativecommons.org/licenses/by/3.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"J. Palacio, J. W. F. Valle, M. Hirsch, N. Rojas, R. A. Lineros, S. Morisi","submitted_at":"2013-07-30T20:11:08Z","abstract_excerpt":"The minimal seesaw extension of the Standard SU(3) x SU(2) x U(1) Model requires two electroweak singlet fermions in order to accommodate the neutrino oscillation parameters at tree level. Here we consider a next to minimal extension where light neutrino masses are generated radiatively by two electroweak fermions: one singlet and one triplet under SU(2). These should be odd under a parity symmetry and their mixing gives rise to a stable weakly interactive massive particle (WIMP) dark matter candidate. For mass in the GeV-TeV range, it reproduces the correct relic density, and provides an obse"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1307.8134","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":""},"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":"1307.8134","created_at":"2026-05-18T03:08:06.836817+00:00"},{"alias_kind":"arxiv_version","alias_value":"1307.8134v2","created_at":"2026-05-18T03:08:06.836817+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1307.8134","created_at":"2026-05-18T03:08:06.836817+00:00"},{"alias_kind":"pith_short_12","alias_value":"BWQOLXGNTQBV","created_at":"2026-05-18T12:27:40.988391+00:00"},{"alias_kind":"pith_short_16","alias_value":"BWQOLXGNTQBVXQ5Z","created_at":"2026-05-18T12:27:40.988391+00:00"},{"alias_kind":"pith_short_8","alias_value":"BWQOLXGN","created_at":"2026-05-18T12:27:40.988391+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.11097","citing_title":"Two-loop neutrino mass model with modular $S_4$ symmetry","ref_index":16,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/BWQOLXGNTQBVXQ5ZQNIPFKZQW4","json":"https://pith.science/pith/BWQOLXGNTQBVXQ5ZQNIPFKZQW4.json","graph_json":"https://pith.science/api/pith-number/BWQOLXGNTQBVXQ5ZQNIPFKZQW4/graph.json","events_json":"https://pith.science/api/pith-number/BWQOLXGNTQBVXQ5ZQNIPFKZQW4/events.json","paper":"https://pith.science/paper/BWQOLXGN"},"agent_actions":{"view_html":"https://pith.science/pith/BWQOLXGNTQBVXQ5ZQNIPFKZQW4","download_json":"https://pith.science/pith/BWQOLXGNTQBVXQ5ZQNIPFKZQW4.json","view_paper":"https://pith.science/paper/BWQOLXGN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1307.8134&json=true","fetch_graph":"https://pith.science/api/pith-number/BWQOLXGNTQBVXQ5ZQNIPFKZQW4/graph.json","fetch_events":"https://pith.science/api/pith-number/BWQOLXGNTQBVXQ5ZQNIPFKZQW4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BWQOLXGNTQBVXQ5ZQNIPFKZQW4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BWQOLXGNTQBVXQ5ZQNIPFKZQW4/action/storage_attestation","attest_author":"https://pith.science/pith/BWQOLXGNTQBVXQ5ZQNIPFKZQW4/action/author_attestation","sign_citation":"https://pith.science/pith/BWQOLXGNTQBVXQ5ZQNIPFKZQW4/action/citation_signature","submit_replication":"https://pith.science/pith/BWQOLXGNTQBVXQ5ZQNIPFKZQW4/action/replication_record"}},"created_at":"2026-05-18T03:08:06.836817+00:00","updated_at":"2026-05-18T03:08:06.836817+00:00"}