{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:MFJVJERRIR6YQY2TZUVQUGANCL","short_pith_number":"pith:MFJVJERR","schema_version":"1.0","canonical_sha256":"6153549231447d886353cd2b0a180d12e4fcb4d6861e4d8cb5834c6455fafb0f","source":{"kind":"arxiv","id":"1204.2373","version":1},"attestation_state":"computed","paper":{"title":"Mini--Review of Dark Matter: 2012","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Gilles Gerbier (Saclay), Manuel Drees (Bonn)","submitted_at":"2012-04-11T08:27:18Z","abstract_excerpt":"This is the mini-review on Dark Matter in the 2012 edition of the Particle Data Group's Review of Particle Properties. After briefly summarizing the arguments in favor of the existence of Dark Matter, we list possible candidates, ranging in mass from a fraction of an eV (e.g., axions) to many solar masses (e.g., primordial black holes), and discuss ways to detect them. The main emphasis is on Weakly Interacting Massive Particles (WIMPs). A large international effort is being made to detect them directly, or else to detect their annihilation products. We explain why we consider all claims to ha"},"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":"1204.2373","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2012-04-11T08:27:18Z","cross_cats_sorted":[],"title_canon_sha256":"d8307c932068aabff3734e777a73606bf6488983ff2af1cadd906d5a3c61a815","abstract_canon_sha256":"e2e64e30ea04f626efda996de8eb131026653f29decc9eac6b27558625fc0a64"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:58:05.473894Z","signature_b64":"4ePwawXdn3s7KgeLVmhRww/iV11lxttN+XM0EtXreLz71FcM9PHPpCClWBY2V8MyUh4XwctXukEanDFbTIENCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6153549231447d886353cd2b0a180d12e4fcb4d6861e4d8cb5834c6455fafb0f","last_reissued_at":"2026-05-18T03:58:05.473331Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:58:05.473331Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Mini--Review of Dark Matter: 2012","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Gilles Gerbier (Saclay), Manuel Drees (Bonn)","submitted_at":"2012-04-11T08:27:18Z","abstract_excerpt":"This is the mini-review on Dark Matter in the 2012 edition of the Particle Data Group's Review of Particle Properties. After briefly summarizing the arguments in favor of the existence of Dark Matter, we list possible candidates, ranging in mass from a fraction of an eV (e.g., axions) to many solar masses (e.g., primordial black holes), and discuss ways to detect them. The main emphasis is on Weakly Interacting Massive Particles (WIMPs). A large international effort is being made to detect them directly, or else to detect their annihilation products. We explain why we consider all claims to ha"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1204.2373","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":""},"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":"1204.2373","created_at":"2026-05-18T03:58:05.473407+00:00"},{"alias_kind":"arxiv_version","alias_value":"1204.2373v1","created_at":"2026-05-18T03:58:05.473407+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1204.2373","created_at":"2026-05-18T03:58:05.473407+00:00"},{"alias_kind":"pith_short_12","alias_value":"MFJVJERRIR6Y","created_at":"2026-05-18T12:27:14.488303+00:00"},{"alias_kind":"pith_short_16","alias_value":"MFJVJERRIR6YQY2T","created_at":"2026-05-18T12:27:14.488303+00:00"},{"alias_kind":"pith_short_8","alias_value":"MFJVJERR","created_at":"2026-05-18T12:27:14.488303+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2507.13518","citing_title":"Exploring Direct Detection of Massive Particles Using Wave Propagation from Gravitational Coupling with a Wire Under Tension","ref_index":4,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/MFJVJERRIR6YQY2TZUVQUGANCL","json":"https://pith.science/pith/MFJVJERRIR6YQY2TZUVQUGANCL.json","graph_json":"https://pith.science/api/pith-number/MFJVJERRIR6YQY2TZUVQUGANCL/graph.json","events_json":"https://pith.science/api/pith-number/MFJVJERRIR6YQY2TZUVQUGANCL/events.json","paper":"https://pith.science/paper/MFJVJERR"},"agent_actions":{"view_html":"https://pith.science/pith/MFJVJERRIR6YQY2TZUVQUGANCL","download_json":"https://pith.science/pith/MFJVJERRIR6YQY2TZUVQUGANCL.json","view_paper":"https://pith.science/paper/MFJVJERR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1204.2373&json=true","fetch_graph":"https://pith.science/api/pith-number/MFJVJERRIR6YQY2TZUVQUGANCL/graph.json","fetch_events":"https://pith.science/api/pith-number/MFJVJERRIR6YQY2TZUVQUGANCL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MFJVJERRIR6YQY2TZUVQUGANCL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MFJVJERRIR6YQY2TZUVQUGANCL/action/storage_attestation","attest_author":"https://pith.science/pith/MFJVJERRIR6YQY2TZUVQUGANCL/action/author_attestation","sign_citation":"https://pith.science/pith/MFJVJERRIR6YQY2TZUVQUGANCL/action/citation_signature","submit_replication":"https://pith.science/pith/MFJVJERRIR6YQY2TZUVQUGANCL/action/replication_record"}},"created_at":"2026-05-18T03:58:05.473407+00:00","updated_at":"2026-05-18T03:58:05.473407+00:00"}