{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:ASFOUZCISIGO3QIHVJHAG2NO4G","short_pith_number":"pith:ASFOUZCI","schema_version":"1.0","canonical_sha256":"048aea6448920cedc107aa4e0369aee181c84355f91d846d6b072afb12fd5f26","source":{"kind":"arxiv","id":"2210.07305","version":1},"attestation_state":"computed","paper":{"title":"Dark matter - electron interactions in materials beyond the dark photon model","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Daniel Cole, Einar Urdshals, Marek Matas, Nicola Spaldin, Riccardo Catena, Timon Emken, Walter Tarantino","submitted_at":"2022-10-13T19:19:08Z","abstract_excerpt":"The search for sub-GeV dark matter (DM) particles via electronic transitions in underground detectors attracted much theoretical and experimental interest in the past few years. A still open question in this field is whether experimental results can in general be interpreted in a framework where the response of detector materials to an external DM probe is described by a single ionisation or crystal form factor, as expected for the so-called dark photon model. Here, ionisation and crystal form factors are examples of material response functions: interaction-specific integrals of the initial an"},"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":"2210.07305","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-ph","submitted_at":"2022-10-13T19:19:08Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"3001e04e5eb084c03e88033b6a034bc51fa805c67e6f1bdb8e3a863e7010edb7","abstract_canon_sha256":"62232a9c43b495a32072fa41ddebb0a1e1a4b3567b35a77dc5b1c213a1eca8af"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:57:57.732082Z","signature_b64":"g2DMCtwGoWg0tQUh2m6xpAv/QcTpo5VbVKDAPLtOK4EqYkepBp4EFIdRgq8sWXHVgApBCqn9mBafL9Ou+Pt6Bw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"048aea6448920cedc107aa4e0369aee181c84355f91d846d6b072afb12fd5f26","last_reissued_at":"2026-07-05T05:57:57.731628Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:57:57.731628Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dark matter - electron interactions in materials beyond the dark photon model","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Daniel Cole, Einar Urdshals, Marek Matas, Nicola Spaldin, Riccardo Catena, Timon Emken, Walter Tarantino","submitted_at":"2022-10-13T19:19:08Z","abstract_excerpt":"The search for sub-GeV dark matter (DM) particles via electronic transitions in underground detectors attracted much theoretical and experimental interest in the past few years. A still open question in this field is whether experimental results can in general be interpreted in a framework where the response of detector materials to an external DM probe is described by a single ionisation or crystal form factor, as expected for the so-called dark photon model. Here, ionisation and crystal form factors are examples of material response functions: interaction-specific integrals of the initial an"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2210.07305","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/2210.07305/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":"2210.07305","created_at":"2026-07-05T05:57:57.731688+00:00"},{"alias_kind":"arxiv_version","alias_value":"2210.07305v1","created_at":"2026-07-05T05:57:57.731688+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2210.07305","created_at":"2026-07-05T05:57:57.731688+00:00"},{"alias_kind":"pith_short_12","alias_value":"ASFOUZCISIGO","created_at":"2026-07-05T05:57:57.731688+00:00"},{"alias_kind":"pith_short_16","alias_value":"ASFOUZCISIGO3QIH","created_at":"2026-07-05T05:57:57.731688+00:00"},{"alias_kind":"pith_short_8","alias_value":"ASFOUZCI","created_at":"2026-07-05T05:57:57.731688+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.06929","citing_title":"Direct-detection constraints on inelastic dark matter with a scalar mediator","ref_index":60,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/ASFOUZCISIGO3QIHVJHAG2NO4G","json":"https://pith.science/pith/ASFOUZCISIGO3QIHVJHAG2NO4G.json","graph_json":"https://pith.science/api/pith-number/ASFOUZCISIGO3QIHVJHAG2NO4G/graph.json","events_json":"https://pith.science/api/pith-number/ASFOUZCISIGO3QIHVJHAG2NO4G/events.json","paper":"https://pith.science/paper/ASFOUZCI"},"agent_actions":{"view_html":"https://pith.science/pith/ASFOUZCISIGO3QIHVJHAG2NO4G","download_json":"https://pith.science/pith/ASFOUZCISIGO3QIHVJHAG2NO4G.json","view_paper":"https://pith.science/paper/ASFOUZCI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2210.07305&json=true","fetch_graph":"https://pith.science/api/pith-number/ASFOUZCISIGO3QIHVJHAG2NO4G/graph.json","fetch_events":"https://pith.science/api/pith-number/ASFOUZCISIGO3QIHVJHAG2NO4G/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ASFOUZCISIGO3QIHVJHAG2NO4G/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ASFOUZCISIGO3QIHVJHAG2NO4G/action/storage_attestation","attest_author":"https://pith.science/pith/ASFOUZCISIGO3QIHVJHAG2NO4G/action/author_attestation","sign_citation":"https://pith.science/pith/ASFOUZCISIGO3QIHVJHAG2NO4G/action/citation_signature","submit_replication":"https://pith.science/pith/ASFOUZCISIGO3QIHVJHAG2NO4G/action/replication_record"}},"created_at":"2026-07-05T05:57:57.731688+00:00","updated_at":"2026-07-05T05:57:57.731688+00:00"}