{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:DBXPDJLLJYIKMRTTN3F6WL3IPM","short_pith_number":"pith:DBXPDJLL","schema_version":"1.0","canonical_sha256":"186ef1a56b4e10a646736ecbeb2f687b0d3d97d97ef7ccd7b19f73fd42bc0db3","source":{"kind":"arxiv","id":"1704.05287","version":2},"attestation_state":"computed","paper":{"title":"Probing minimal SUSY scenarios in the light of muon $g-2$ and dark matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Keisuke Yanagi, Koichi Hamaguchi, Motoi Endo, Sho Iwamoto","submitted_at":"2017-04-18T11:59:24Z","abstract_excerpt":"We study supersymmetric (SUSY) models in which the muon $g-2$ discrepancy and the dark matter relic abundance are simultaneously explained. The muon $g-2$ discrepancy, or a 3$\\sigma$ deviation between the experimental and theoretical results of the muon anomalous magnetic moment, can be resolved by SUSY models, which implies at least three SUSY multiplets have masses of $\\mathop{\\mathcal{O}}(100)\\, \\mathrm{GeV}$. In particular, models with the bino, higgsino and slepton having $\\mathop{\\mathcal{O}}(100)\\, \\mathrm{GeV}$ masses are not only capable to explain the muon $g-2$ discrepancy but natur"},"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":"1704.05287","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2017-04-18T11:59:24Z","cross_cats_sorted":[],"title_canon_sha256":"9f60334f82592cfbee5bba626da6320f5c1111bd916b8a8a5b10bdb71027065b","abstract_canon_sha256":"6c8acd02119ac6f9a277873aefd0588be8e862a1f5d8ab1ba7dca725706b1714"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:42:43.609892Z","signature_b64":"zufsgAvjefmSjgw6xUZksUcjFwOp7u4JCfB9AaFIEbPWVwTP2UmzdyOf6qiZFH+cEHDxXi8fZkGdCF5ywhCgDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"186ef1a56b4e10a646736ecbeb2f687b0d3d97d97ef7ccd7b19f73fd42bc0db3","last_reissued_at":"2026-05-18T00:42:43.609165Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:42:43.609165Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Probing minimal SUSY scenarios in the light of muon $g-2$ and dark matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Keisuke Yanagi, Koichi Hamaguchi, Motoi Endo, Sho Iwamoto","submitted_at":"2017-04-18T11:59:24Z","abstract_excerpt":"We study supersymmetric (SUSY) models in which the muon $g-2$ discrepancy and the dark matter relic abundance are simultaneously explained. The muon $g-2$ discrepancy, or a 3$\\sigma$ deviation between the experimental and theoretical results of the muon anomalous magnetic moment, can be resolved by SUSY models, which implies at least three SUSY multiplets have masses of $\\mathop{\\mathcal{O}}(100)\\, \\mathrm{GeV}$. In particular, models with the bino, higgsino and slepton having $\\mathop{\\mathcal{O}}(100)\\, \\mathrm{GeV}$ masses are not only capable to explain the muon $g-2$ discrepancy but natur"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1704.05287","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":"1704.05287","created_at":"2026-05-18T00:42:43.609279+00:00"},{"alias_kind":"arxiv_version","alias_value":"1704.05287v2","created_at":"2026-05-18T00:42:43.609279+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1704.05287","created_at":"2026-05-18T00:42:43.609279+00:00"},{"alias_kind":"pith_short_12","alias_value":"DBXPDJLLJYIK","created_at":"2026-05-18T12:31:10.602751+00:00"},{"alias_kind":"pith_short_16","alias_value":"DBXPDJLLJYIKMRTT","created_at":"2026-05-18T12:31:10.602751+00:00"},{"alias_kind":"pith_short_8","alias_value":"DBXPDJLL","created_at":"2026-05-18T12:31:10.602751+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/DBXPDJLLJYIKMRTTN3F6WL3IPM","json":"https://pith.science/pith/DBXPDJLLJYIKMRTTN3F6WL3IPM.json","graph_json":"https://pith.science/api/pith-number/DBXPDJLLJYIKMRTTN3F6WL3IPM/graph.json","events_json":"https://pith.science/api/pith-number/DBXPDJLLJYIKMRTTN3F6WL3IPM/events.json","paper":"https://pith.science/paper/DBXPDJLL"},"agent_actions":{"view_html":"https://pith.science/pith/DBXPDJLLJYIKMRTTN3F6WL3IPM","download_json":"https://pith.science/pith/DBXPDJLLJYIKMRTTN3F6WL3IPM.json","view_paper":"https://pith.science/paper/DBXPDJLL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1704.05287&json=true","fetch_graph":"https://pith.science/api/pith-number/DBXPDJLLJYIKMRTTN3F6WL3IPM/graph.json","fetch_events":"https://pith.science/api/pith-number/DBXPDJLLJYIKMRTTN3F6WL3IPM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DBXPDJLLJYIKMRTTN3F6WL3IPM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DBXPDJLLJYIKMRTTN3F6WL3IPM/action/storage_attestation","attest_author":"https://pith.science/pith/DBXPDJLLJYIKMRTTN3F6WL3IPM/action/author_attestation","sign_citation":"https://pith.science/pith/DBXPDJLLJYIKMRTTN3F6WL3IPM/action/citation_signature","submit_replication":"https://pith.science/pith/DBXPDJLLJYIKMRTTN3F6WL3IPM/action/replication_record"}},"created_at":"2026-05-18T00:42:43.609279+00:00","updated_at":"2026-05-18T00:42:43.609279+00:00"}