{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:TFJSRVEDOVE7BZDUJECU24E57C","short_pith_number":"pith:TFJSRVED","schema_version":"1.0","canonical_sha256":"995328d4837549f0e47449054d709df8b9528100b5598de9c5d9dbe386f60ef0","source":{"kind":"arxiv","id":"1806.06036","version":2},"attestation_state":"computed","paper":{"title":"Flavor anomalies and dark matter in SUSY with an extra U(1)","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ex"],"primary_cat":"hep-ph","authors_text":"Enrico Maria Sessolo, Kamila Kowalska, Leszek Roszkowski, Luc Darm\\'e","submitted_at":"2018-06-15T16:23:29Z","abstract_excerpt":"Motivated by the recent anomalies in $b\\rightarrow s$ transitions that emerged at LHCb, we consider a model with an $L_\\mu - L_\\tau$ gauge symmetry and additional vector-like fermions. We find that by introducing supersymmetry the model can be made consistent with the long-standing deviation in the measured value of the anomalous magnetic moment of the muon, $g-2$, and neutralino dark matter of broad mass ranges and properties. In particular, dark matter candidates include the well-known 1 TeV higgsino, which in the MSSM is typically not compatible with solutions to the $g-2$ puzzle. Moreover,"},"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":"1806.06036","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2018-06-15T16:23:29Z","cross_cats_sorted":["astro-ph.CO","hep-ex"],"title_canon_sha256":"3e9cc33e23cd86851b909352173540a763d72fae4affdbc97f9d8a9a9afeed37","abstract_canon_sha256":"965fe888f74253001fbd67966e92c35cb722562dcf2f63a12f641040c1202231"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:03:24.396727Z","signature_b64":"mtCGYU/Lsz5mXCDRPvhli/d+hM6H9tHcFadrU2M6Gx4Aos8gyKKiXPfvoX+GPX+/kWaCvIz9h0Abx7u9NXfPCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"995328d4837549f0e47449054d709df8b9528100b5598de9c5d9dbe386f60ef0","last_reissued_at":"2026-05-18T00:03:24.396362Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:03:24.396362Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Flavor anomalies and dark matter in SUSY with an extra U(1)","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ex"],"primary_cat":"hep-ph","authors_text":"Enrico Maria Sessolo, Kamila Kowalska, Leszek Roszkowski, Luc Darm\\'e","submitted_at":"2018-06-15T16:23:29Z","abstract_excerpt":"Motivated by the recent anomalies in $b\\rightarrow s$ transitions that emerged at LHCb, we consider a model with an $L_\\mu - L_\\tau$ gauge symmetry and additional vector-like fermions. We find that by introducing supersymmetry the model can be made consistent with the long-standing deviation in the measured value of the anomalous magnetic moment of the muon, $g-2$, and neutralino dark matter of broad mass ranges and properties. In particular, dark matter candidates include the well-known 1 TeV higgsino, which in the MSSM is typically not compatible with solutions to the $g-2$ puzzle. Moreover,"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1806.06036","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":"1806.06036","created_at":"2026-05-18T00:03:24.396421+00:00"},{"alias_kind":"arxiv_version","alias_value":"1806.06036v2","created_at":"2026-05-18T00:03:24.396421+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1806.06036","created_at":"2026-05-18T00:03:24.396421+00:00"},{"alias_kind":"pith_short_12","alias_value":"TFJSRVEDOVE7","created_at":"2026-05-18T12:32:53.628368+00:00"},{"alias_kind":"pith_short_16","alias_value":"TFJSRVEDOVE7BZDU","created_at":"2026-05-18T12:32:53.628368+00:00"},{"alias_kind":"pith_short_8","alias_value":"TFJSRVED","created_at":"2026-05-18T12:32:53.628368+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"1906.08596","citing_title":"Global Bayesian Analysis of new physics in $b \\to s \\mu\\mu$ transitions after Moriond-2019","ref_index":19,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TFJSRVEDOVE7BZDUJECU24E57C","json":"https://pith.science/pith/TFJSRVEDOVE7BZDUJECU24E57C.json","graph_json":"https://pith.science/api/pith-number/TFJSRVEDOVE7BZDUJECU24E57C/graph.json","events_json":"https://pith.science/api/pith-number/TFJSRVEDOVE7BZDUJECU24E57C/events.json","paper":"https://pith.science/paper/TFJSRVED"},"agent_actions":{"view_html":"https://pith.science/pith/TFJSRVEDOVE7BZDUJECU24E57C","download_json":"https://pith.science/pith/TFJSRVEDOVE7BZDUJECU24E57C.json","view_paper":"https://pith.science/paper/TFJSRVED","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1806.06036&json=true","fetch_graph":"https://pith.science/api/pith-number/TFJSRVEDOVE7BZDUJECU24E57C/graph.json","fetch_events":"https://pith.science/api/pith-number/TFJSRVEDOVE7BZDUJECU24E57C/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TFJSRVEDOVE7BZDUJECU24E57C/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TFJSRVEDOVE7BZDUJECU24E57C/action/storage_attestation","attest_author":"https://pith.science/pith/TFJSRVEDOVE7BZDUJECU24E57C/action/author_attestation","sign_citation":"https://pith.science/pith/TFJSRVEDOVE7BZDUJECU24E57C/action/citation_signature","submit_replication":"https://pith.science/pith/TFJSRVEDOVE7BZDUJECU24E57C/action/replication_record"}},"created_at":"2026-05-18T00:03:24.396421+00:00","updated_at":"2026-05-18T00:03:24.396421+00:00"}