{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:RDHIKORQ3GHNFRQRWFVJPDM26Y","short_pith_number":"pith:RDHIKORQ","schema_version":"1.0","canonical_sha256":"88ce853a30d98ed2c611b16a978d9af605bc0984c3531f78807540b573d526f7","source":{"kind":"arxiv","id":"2104.03245","version":1},"attestation_state":"computed","paper":{"title":"Dark matter, fine-tuning and $(g-2)_{\\mu}$ in the pMSSM","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Jeremy de Wit, Marrit Schutten, Melissa van Beekveld, Wim Beenakker","submitted_at":"2021-04-07T16:48:35Z","abstract_excerpt":"In this paper we analyze spectra in the phenomenological supersymmetric Standard Model that simultaneously result in the right dark-matter relic density $\\Omega_{\\rm DM} h^2$, offer an explanation for the $(g-2)_{\\mu}$ discrepancy $\\Delta a_{\\mu}$ and are minimally fine-tuned. We discuss the LHC phenomenology resulting from these spectra and the sensitivity of dark-matter direct detection experiments to these spectra. We find that the latter type of experiments with sensitivity to the spin-dependent dark-matter-nucleon scattering cross section $\\sigma_{\\rm SD,p}$ will probe all of our found so"},"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":"2104.03245","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-ph","submitted_at":"2021-04-07T16:48:35Z","cross_cats_sorted":[],"title_canon_sha256":"211c30cb6243373bfa1f570e1c0b9d80127b8d2a18bf833bbcbc052290f4aa7f","abstract_canon_sha256":"47c6214d2dae855982c10d4f69490f4b468aae0a9928ca6e75da0bfa8e334b8b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:30:09.337215Z","signature_b64":"/sINpFxZgSg9pEte9aihBFQYZiNmLaCj5LZYMwq9qyabP6L3kciH0EQmeI5+ZUwXt9B4JkCzyRygyZyh4z0XCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"88ce853a30d98ed2c611b16a978d9af605bc0984c3531f78807540b573d526f7","last_reissued_at":"2026-07-05T02:30:09.336660Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:30:09.336660Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dark matter, fine-tuning and $(g-2)_{\\mu}$ in the pMSSM","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Jeremy de Wit, Marrit Schutten, Melissa van Beekveld, Wim Beenakker","submitted_at":"2021-04-07T16:48:35Z","abstract_excerpt":"In this paper we analyze spectra in the phenomenological supersymmetric Standard Model that simultaneously result in the right dark-matter relic density $\\Omega_{\\rm DM} h^2$, offer an explanation for the $(g-2)_{\\mu}$ discrepancy $\\Delta a_{\\mu}$ and are minimally fine-tuned. We discuss the LHC phenomenology resulting from these spectra and the sensitivity of dark-matter direct detection experiments to these spectra. We find that the latter type of experiments with sensitivity to the spin-dependent dark-matter-nucleon scattering cross section $\\sigma_{\\rm SD,p}$ will probe all of our found so"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2104.03245","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2104.03245/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2104.03245","created_at":"2026-07-05T02:30:09.336721+00:00"},{"alias_kind":"arxiv_version","alias_value":"2104.03245v1","created_at":"2026-07-05T02:30:09.336721+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2104.03245","created_at":"2026-07-05T02:30:09.336721+00:00"},{"alias_kind":"pith_short_12","alias_value":"RDHIKORQ3GHN","created_at":"2026-07-05T02:30:09.336721+00:00"},{"alias_kind":"pith_short_16","alias_value":"RDHIKORQ3GHNFRQR","created_at":"2026-07-05T02:30:09.336721+00:00"},{"alias_kind":"pith_short_8","alias_value":"RDHIKORQ","created_at":"2026-07-05T02:30:09.336721+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2501.12039","citing_title":"The Light Neutralino Dark Matter in the Generalized Minimal Supergravity (GmSUGRA)","ref_index":32,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/RDHIKORQ3GHNFRQRWFVJPDM26Y","json":"https://pith.science/pith/RDHIKORQ3GHNFRQRWFVJPDM26Y.json","graph_json":"https://pith.science/api/pith-number/RDHIKORQ3GHNFRQRWFVJPDM26Y/graph.json","events_json":"https://pith.science/api/pith-number/RDHIKORQ3GHNFRQRWFVJPDM26Y/events.json","paper":"https://pith.science/paper/RDHIKORQ"},"agent_actions":{"view_html":"https://pith.science/pith/RDHIKORQ3GHNFRQRWFVJPDM26Y","download_json":"https://pith.science/pith/RDHIKORQ3GHNFRQRWFVJPDM26Y.json","view_paper":"https://pith.science/paper/RDHIKORQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2104.03245&json=true","fetch_graph":"https://pith.science/api/pith-number/RDHIKORQ3GHNFRQRWFVJPDM26Y/graph.json","fetch_events":"https://pith.science/api/pith-number/RDHIKORQ3GHNFRQRWFVJPDM26Y/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RDHIKORQ3GHNFRQRWFVJPDM26Y/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RDHIKORQ3GHNFRQRWFVJPDM26Y/action/storage_attestation","attest_author":"https://pith.science/pith/RDHIKORQ3GHNFRQRWFVJPDM26Y/action/author_attestation","sign_citation":"https://pith.science/pith/RDHIKORQ3GHNFRQRWFVJPDM26Y/action/citation_signature","submit_replication":"https://pith.science/pith/RDHIKORQ3GHNFRQRWFVJPDM26Y/action/replication_record"}},"created_at":"2026-07-05T02:30:09.336721+00:00","updated_at":"2026-07-05T02:30:09.336721+00:00"}