{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2002:Z4MN6BD2C67HLHLKCCOCKVGA43","short_pith_number":"pith:Z4MN6BD2","schema_version":"1.0","canonical_sha256":"cf18df047a17be759d6a109c2554c0e6f4debf3d6bc990326d11754dec31e155","source":{"kind":"arxiv","id":"hep-ph/0212379","version":2},"attestation_state":"computed","paper":{"title":"Light Relic Neutralinos","license":"","headline":"","cross_cats":["astro-ph","hep-ex"],"primary_cat":"hep-ph","authors_text":"A. Bottino, INFN - Torino), N. Fornengo, S. Scopel (U. of Torino","submitted_at":"2002-12-27T16:54:23Z","abstract_excerpt":"The relic abundance and the scalar cross-section off nucleon for light neutralinos (of mass below about 45 GeV) are evaluated in an effective MSSM model without GUT-inspired relations among gaugino masses. It is shown that these neutralinos may provide a sizeable contribution to the matter density in the Universe and produce measurable effects in WIMP direct detection experiments. These properties are elucidated in terms of simple analytical arguments."},"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":"hep-ph/0212379","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"hep-ph","submitted_at":"2002-12-27T16:54:23Z","cross_cats_sorted":["astro-ph","hep-ex"],"title_canon_sha256":"adfce70bb323ce2d8a22bb5c8d48b2484cb13a5b6960c2d32251360fe5ac3a5e","abstract_canon_sha256":"7d2622ac8447d14f1685a5d4810cb87766e9e18399863598eb54b879ba73df95"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:26:42.923417Z","signature_b64":"8tL9tdxM3GoOEPL0ynbb1/mdU/EXK7jf7QwIW3jh5ibe+EPSwGuOIkxZnOBg+yKONUgh7882CGs3AMsNWah9Bg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"cf18df047a17be759d6a109c2554c0e6f4debf3d6bc990326d11754dec31e155","last_reissued_at":"2026-07-04T15:26:42.923024Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:26:42.923024Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Light Relic Neutralinos","license":"","headline":"","cross_cats":["astro-ph","hep-ex"],"primary_cat":"hep-ph","authors_text":"A. Bottino, INFN - Torino), N. Fornengo, S. Scopel (U. of Torino","submitted_at":"2002-12-27T16:54:23Z","abstract_excerpt":"The relic abundance and the scalar cross-section off nucleon for light neutralinos (of mass below about 45 GeV) are evaluated in an effective MSSM model without GUT-inspired relations among gaugino masses. It is shown that these neutralinos may provide a sizeable contribution to the matter density in the Universe and produce measurable effects in WIMP direct detection experiments. These properties are elucidated in terms of simple analytical arguments."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-ph/0212379","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/hep-ph/0212379/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":"hep-ph/0212379","created_at":"2026-07-04T15:26:42.923077+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-ph/0212379v2","created_at":"2026-07-04T15:26:42.923077+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-ph/0212379","created_at":"2026-07-04T15:26:42.923077+00:00"},{"alias_kind":"pith_short_12","alias_value":"Z4MN6BD2C67H","created_at":"2026-07-04T15:26:42.923077+00:00"},{"alias_kind":"pith_short_16","alias_value":"Z4MN6BD2C67HLHLK","created_at":"2026-07-04T15:26:42.923077+00:00"},{"alias_kind":"pith_short_8","alias_value":"Z4MN6BD2","created_at":"2026-07-04T15:26:42.923077+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2507.00359","citing_title":"Searching for long-lived light neutralinos from $B$-meson decays with baryonic R-parity violation at Belle II","ref_index":23,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/Z4MN6BD2C67HLHLKCCOCKVGA43","json":"https://pith.science/pith/Z4MN6BD2C67HLHLKCCOCKVGA43.json","graph_json":"https://pith.science/api/pith-number/Z4MN6BD2C67HLHLKCCOCKVGA43/graph.json","events_json":"https://pith.science/api/pith-number/Z4MN6BD2C67HLHLKCCOCKVGA43/events.json","paper":"https://pith.science/paper/Z4MN6BD2"},"agent_actions":{"view_html":"https://pith.science/pith/Z4MN6BD2C67HLHLKCCOCKVGA43","download_json":"https://pith.science/pith/Z4MN6BD2C67HLHLKCCOCKVGA43.json","view_paper":"https://pith.science/paper/Z4MN6BD2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-ph/0212379&json=true","fetch_graph":"https://pith.science/api/pith-number/Z4MN6BD2C67HLHLKCCOCKVGA43/graph.json","fetch_events":"https://pith.science/api/pith-number/Z4MN6BD2C67HLHLKCCOCKVGA43/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/Z4MN6BD2C67HLHLKCCOCKVGA43/action/timestamp_anchor","attest_storage":"https://pith.science/pith/Z4MN6BD2C67HLHLKCCOCKVGA43/action/storage_attestation","attest_author":"https://pith.science/pith/Z4MN6BD2C67HLHLKCCOCKVGA43/action/author_attestation","sign_citation":"https://pith.science/pith/Z4MN6BD2C67HLHLKCCOCKVGA43/action/citation_signature","submit_replication":"https://pith.science/pith/Z4MN6BD2C67HLHLKCCOCKVGA43/action/replication_record"}},"created_at":"2026-07-04T15:26:42.923077+00:00","updated_at":"2026-07-04T15:26:42.923077+00:00"}