{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:TKGP5KJWTC6HVRTCJ57IAA35WO","short_pith_number":"pith:TKGP5KJW","schema_version":"1.0","canonical_sha256":"9a8cfea93698bc7ac6624f7e80037db3afe64d9a3e0b46bc9ea4c25fadc84078","source":{"kind":"arxiv","id":"1504.05755","version":2},"attestation_state":"computed","paper":{"title":"A Model of Neutrino Mass and Dark Matter with an Accidental Symmetry","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Amine Ahriche, Kristian L. McDonald, Salah Nasri, Takashi Toma","submitted_at":"2015-04-22T12:27:15Z","abstract_excerpt":"We present a model of radiative neutrino mass that automatically contains an accidental $Z_2$ symmetry and thus provides a stable dark matter candidate. This allows a common framework for the origin of neutrino mass and dark matter without invoking any symmetries beyond those of the Standard Model. The model can be probed by direct-detection experiments and $\\mu\\rightarrow e+\\gamma$ searches, and predicts a charged scalar that can appear at the TeV scale, within reach of collider experiments."},"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":"1504.05755","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2015-04-22T12:27:15Z","cross_cats_sorted":[],"title_canon_sha256":"2f6f1f0d36bfbbb32c0cf73edd18e4a897ba87f7da3a8ceb9b0e92bdf2a77fcc","abstract_canon_sha256":"3daa13d832eb6b129fe354a6d547235bd29942c7b3be50ead04255949d2fcdc1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:27:31.772733Z","signature_b64":"JMcrHOW8IttvEmg4HLdhKkPHlxTgmmsgHTpNUTkybSEquXdx36r4YMuN6b8XP/sMpkfYHLldDe+SL6/c8vllDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9a8cfea93698bc7ac6624f7e80037db3afe64d9a3e0b46bc9ea4c25fadc84078","last_reissued_at":"2026-05-18T01:27:31.772312Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:27:31.772312Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A Model of Neutrino Mass and Dark Matter with an Accidental Symmetry","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Amine Ahriche, Kristian L. McDonald, Salah Nasri, Takashi Toma","submitted_at":"2015-04-22T12:27:15Z","abstract_excerpt":"We present a model of radiative neutrino mass that automatically contains an accidental $Z_2$ symmetry and thus provides a stable dark matter candidate. This allows a common framework for the origin of neutrino mass and dark matter without invoking any symmetries beyond those of the Standard Model. The model can be probed by direct-detection experiments and $\\mu\\rightarrow e+\\gamma$ searches, and predicts a charged scalar that can appear at the TeV scale, within reach of collider experiments."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1504.05755","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":"1504.05755","created_at":"2026-05-18T01:27:31.772382+00:00"},{"alias_kind":"arxiv_version","alias_value":"1504.05755v2","created_at":"2026-05-18T01:27:31.772382+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1504.05755","created_at":"2026-05-18T01:27:31.772382+00:00"},{"alias_kind":"pith_short_12","alias_value":"TKGP5KJWTC6H","created_at":"2026-05-18T12:29:42.218222+00:00"},{"alias_kind":"pith_short_16","alias_value":"TKGP5KJWTC6HVRTC","created_at":"2026-05-18T12:29:42.218222+00:00"},{"alias_kind":"pith_short_8","alias_value":"TKGP5KJW","created_at":"2026-05-18T12:29:42.218222+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2511.16762","citing_title":"Radiative neutrino mass generation and dark matter through vectorlike leptons","ref_index":16,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TKGP5KJWTC6HVRTCJ57IAA35WO","json":"https://pith.science/pith/TKGP5KJWTC6HVRTCJ57IAA35WO.json","graph_json":"https://pith.science/api/pith-number/TKGP5KJWTC6HVRTCJ57IAA35WO/graph.json","events_json":"https://pith.science/api/pith-number/TKGP5KJWTC6HVRTCJ57IAA35WO/events.json","paper":"https://pith.science/paper/TKGP5KJW"},"agent_actions":{"view_html":"https://pith.science/pith/TKGP5KJWTC6HVRTCJ57IAA35WO","download_json":"https://pith.science/pith/TKGP5KJWTC6HVRTCJ57IAA35WO.json","view_paper":"https://pith.science/paper/TKGP5KJW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1504.05755&json=true","fetch_graph":"https://pith.science/api/pith-number/TKGP5KJWTC6HVRTCJ57IAA35WO/graph.json","fetch_events":"https://pith.science/api/pith-number/TKGP5KJWTC6HVRTCJ57IAA35WO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TKGP5KJWTC6HVRTCJ57IAA35WO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TKGP5KJWTC6HVRTCJ57IAA35WO/action/storage_attestation","attest_author":"https://pith.science/pith/TKGP5KJWTC6HVRTCJ57IAA35WO/action/author_attestation","sign_citation":"https://pith.science/pith/TKGP5KJWTC6HVRTCJ57IAA35WO/action/citation_signature","submit_replication":"https://pith.science/pith/TKGP5KJWTC6HVRTCJ57IAA35WO/action/replication_record"}},"created_at":"2026-05-18T01:27:31.772382+00:00","updated_at":"2026-05-18T01:27:31.772382+00:00"}