{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:RDO36DM52YHMKH2FJ5ED2UN7SQ","short_pith_number":"pith:RDO36DM5","schema_version":"1.0","canonical_sha256":"88ddbf0d9dd60ec51f454f483d51bf942fb7221a60ae28bb9b6ff24948cd8eb2","source":{"kind":"arxiv","id":"1312.3326","version":2},"attestation_state":"computed","paper":{"title":"LUX Constraints on Magnetic Dark Matter in the $S\\bar{E} \\chi$y Model with(out) Naturality","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Francesco Sannino, Ian M. Shoemaker, Mads T. Frandsen, Ole Svendsen","submitted_at":"2013-12-11T21:00:13Z","abstract_excerpt":"We study phenomenological constraints in a simple $S\\bar{E} \\chi$y extension of the Standard Model (SM) with a 125 GeV Higgs, a vector-like heavy electron $(E)$, a complex scalar electron $(S)$ and a standard model singlet Dirac fermion $(\\chi)$. The interactions among the dark matter candidate $\\chi$ and the standard model particles occur via loop-induced processes involving the Yukawa interaction $S\\bar{E} \\chi$y. The model is an explicit perturbative realization of so-called magnetic dark matter. The field content allows for a cancelation of quadratic divergences in the scalar masses at one"},"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":"1312.3326","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2013-12-11T21:00:13Z","cross_cats_sorted":[],"title_canon_sha256":"0c4fa5546bea3f82b6d4b0b732eb224d9038786dd9a4025b4d7cab0d07f94f32","abstract_canon_sha256":"05b4cfe891904b94e8f676936e85a1cd2ed919b68c2203d6d58507388b32193e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:54:46.642372Z","signature_b64":"qLrMnd1L+dF4/1wIlgOmiadO4UNfz2xcOVtszeItlM4Ax7jwNvD+wd4Jyi5Sn4DBbQ3cELhZkOcPs0ORTxE4DA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"88ddbf0d9dd60ec51f454f483d51bf942fb7221a60ae28bb9b6ff24948cd8eb2","last_reissued_at":"2026-05-18T02:54:46.641979Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:54:46.641979Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"LUX Constraints on Magnetic Dark Matter in the $S\\bar{E} \\chi$y Model with(out) Naturality","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Francesco Sannino, Ian M. Shoemaker, Mads T. Frandsen, Ole Svendsen","submitted_at":"2013-12-11T21:00:13Z","abstract_excerpt":"We study phenomenological constraints in a simple $S\\bar{E} \\chi$y extension of the Standard Model (SM) with a 125 GeV Higgs, a vector-like heavy electron $(E)$, a complex scalar electron $(S)$ and a standard model singlet Dirac fermion $(\\chi)$. The interactions among the dark matter candidate $\\chi$ and the standard model particles occur via loop-induced processes involving the Yukawa interaction $S\\bar{E} \\chi$y. The model is an explicit perturbative realization of so-called magnetic dark matter. The field content allows for a cancelation of quadratic divergences in the scalar masses at one"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1312.3326","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":"1312.3326","created_at":"2026-05-18T02:54:46.642038+00:00"},{"alias_kind":"arxiv_version","alias_value":"1312.3326v2","created_at":"2026-05-18T02:54:46.642038+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1312.3326","created_at":"2026-05-18T02:54:46.642038+00:00"},{"alias_kind":"pith_short_12","alias_value":"RDO36DM52YHM","created_at":"2026-05-18T12:27:57.521954+00:00"},{"alias_kind":"pith_short_16","alias_value":"RDO36DM52YHMKH2F","created_at":"2026-05-18T12:27:57.521954+00:00"},{"alias_kind":"pith_short_8","alias_value":"RDO36DM5","created_at":"2026-05-18T12:27:57.521954+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/RDO36DM52YHMKH2FJ5ED2UN7SQ","json":"https://pith.science/pith/RDO36DM52YHMKH2FJ5ED2UN7SQ.json","graph_json":"https://pith.science/api/pith-number/RDO36DM52YHMKH2FJ5ED2UN7SQ/graph.json","events_json":"https://pith.science/api/pith-number/RDO36DM52YHMKH2FJ5ED2UN7SQ/events.json","paper":"https://pith.science/paper/RDO36DM5"},"agent_actions":{"view_html":"https://pith.science/pith/RDO36DM52YHMKH2FJ5ED2UN7SQ","download_json":"https://pith.science/pith/RDO36DM52YHMKH2FJ5ED2UN7SQ.json","view_paper":"https://pith.science/paper/RDO36DM5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1312.3326&json=true","fetch_graph":"https://pith.science/api/pith-number/RDO36DM52YHMKH2FJ5ED2UN7SQ/graph.json","fetch_events":"https://pith.science/api/pith-number/RDO36DM52YHMKH2FJ5ED2UN7SQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RDO36DM52YHMKH2FJ5ED2UN7SQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RDO36DM52YHMKH2FJ5ED2UN7SQ/action/storage_attestation","attest_author":"https://pith.science/pith/RDO36DM52YHMKH2FJ5ED2UN7SQ/action/author_attestation","sign_citation":"https://pith.science/pith/RDO36DM52YHMKH2FJ5ED2UN7SQ/action/citation_signature","submit_replication":"https://pith.science/pith/RDO36DM52YHMKH2FJ5ED2UN7SQ/action/replication_record"}},"created_at":"2026-05-18T02:54:46.642038+00:00","updated_at":"2026-05-18T02:54:46.642038+00:00"}