{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:AFSGHNDCBJD2TZRPA26UY34NPO","short_pith_number":"pith:AFSGHNDC","schema_version":"1.0","canonical_sha256":"016463b4620a47a9e62f06bd4c6f8d7b8045569cb4272607de651ef94f220c11","source":{"kind":"arxiv","id":"1501.02020","version":1},"attestation_state":"computed","paper":{"title":"A three-loop radiative neutrino mass model with dark matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Fei Zhang, Li-gang Jin, Rui Tang","submitted_at":"2015-01-09T02:46:39Z","abstract_excerpt":"We present a model that generates small neutrino masses at three-loop level due to the existence of Majorana fermionic dark matter, which is stabilized by a Z2 symmetry. The model predicts that the lightest neutrino is massless. We show a prototypical parameter choice allowed by relevant experimental data, which favors the case of normal neutrino mass spectrum and the dark matter with m \\sim 50-135 GeV and a sizable Yukawa coupling. It means that new particles can be searched for in future e+e- collisions."},"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":"1501.02020","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2015-01-09T02:46:39Z","cross_cats_sorted":[],"title_canon_sha256":"434333344bf57fd156a666acc735d0382bf03e015b1cb06acc2db777b345e155","abstract_canon_sha256":"21d880ea8d0974fe02616d9cbc9696a4b43d50d4edb7a67026000dad329bff01"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:16:34.163097Z","signature_b64":"S2ww0bw4d5tSLGW1L15VX3j6dFM02OcrWt9In6zN6s92EMWY2emv5oi00WYGQxhCxluTN+0sXs4GDAihxaebCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"016463b4620a47a9e62f06bd4c6f8d7b8045569cb4272607de651ef94f220c11","last_reissued_at":"2026-05-18T00:16:34.162557Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:16:34.162557Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A three-loop radiative neutrino mass model with dark matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Fei Zhang, Li-gang Jin, Rui Tang","submitted_at":"2015-01-09T02:46:39Z","abstract_excerpt":"We present a model that generates small neutrino masses at three-loop level due to the existence of Majorana fermionic dark matter, which is stabilized by a Z2 symmetry. The model predicts that the lightest neutrino is massless. We show a prototypical parameter choice allowed by relevant experimental data, which favors the case of normal neutrino mass spectrum and the dark matter with m \\sim 50-135 GeV and a sizable Yukawa coupling. It means that new particles can be searched for in future e+e- collisions."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1501.02020","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":""},"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":"1501.02020","created_at":"2026-05-18T00:16:34.162646+00:00"},{"alias_kind":"arxiv_version","alias_value":"1501.02020v1","created_at":"2026-05-18T00:16:34.162646+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1501.02020","created_at":"2026-05-18T00:16:34.162646+00:00"},{"alias_kind":"pith_short_12","alias_value":"AFSGHNDCBJD2","created_at":"2026-05-18T12:29:10.953037+00:00"},{"alias_kind":"pith_short_16","alias_value":"AFSGHNDCBJD2TZRP","created_at":"2026-05-18T12:29:10.953037+00:00"},{"alias_kind":"pith_short_8","alias_value":"AFSGHNDC","created_at":"2026-05-18T12:29:10.953037+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":22,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/AFSGHNDCBJD2TZRPA26UY34NPO","json":"https://pith.science/pith/AFSGHNDCBJD2TZRPA26UY34NPO.json","graph_json":"https://pith.science/api/pith-number/AFSGHNDCBJD2TZRPA26UY34NPO/graph.json","events_json":"https://pith.science/api/pith-number/AFSGHNDCBJD2TZRPA26UY34NPO/events.json","paper":"https://pith.science/paper/AFSGHNDC"},"agent_actions":{"view_html":"https://pith.science/pith/AFSGHNDCBJD2TZRPA26UY34NPO","download_json":"https://pith.science/pith/AFSGHNDCBJD2TZRPA26UY34NPO.json","view_paper":"https://pith.science/paper/AFSGHNDC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1501.02020&json=true","fetch_graph":"https://pith.science/api/pith-number/AFSGHNDCBJD2TZRPA26UY34NPO/graph.json","fetch_events":"https://pith.science/api/pith-number/AFSGHNDCBJD2TZRPA26UY34NPO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AFSGHNDCBJD2TZRPA26UY34NPO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AFSGHNDCBJD2TZRPA26UY34NPO/action/storage_attestation","attest_author":"https://pith.science/pith/AFSGHNDCBJD2TZRPA26UY34NPO/action/author_attestation","sign_citation":"https://pith.science/pith/AFSGHNDCBJD2TZRPA26UY34NPO/action/citation_signature","submit_replication":"https://pith.science/pith/AFSGHNDCBJD2TZRPA26UY34NPO/action/replication_record"}},"created_at":"2026-05-18T00:16:34.162646+00:00","updated_at":"2026-05-18T00:16:34.162646+00:00"}