{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2002:HTJSJAUD4LRKWIGXGJWNJQYI2Q","short_pith_number":"pith:HTJSJAUD","schema_version":"1.0","canonical_sha256":"3cd3248283e2e2ab20d7326cd4c308d42c4dcf3d84b34ebc403dfb8c37a82668","source":{"kind":"arxiv","id":"hep-ph/0209262","version":4},"attestation_state":"computed","paper":{"title":"Elastic Scattering and Direct Detection of Kaluza-Klein Dark Matter","license":"","headline":"","cross_cats":["astro-ph"],"primary_cat":"hep-ph","authors_text":"Geraldine Servant, Tim M.P. Tait","submitted_at":"2002-09-23T16:55:05Z","abstract_excerpt":"Recently a new dark matter candidate has been proposed as a consequence of universal compact extra dimensions. It was found that to account for cosmological observations, the masses of the first Kaluza-Klein modes (and thus the approximate size of the extra dimension) should be in the range 600-1200 GeV when the lightest Kaluza-Klein particle (LKP) corresponds to the hypercharge boson and in the range 1 - 1.8 TeV when it corresponds to a neutrino. In this article, we compute the elastic scattering cross sections between Kaluza-Klein dark matter and nuclei both when the lightest Kaluza-Klein pa"},"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/0209262","kind":"arxiv","version":4},"metadata":{"license":"","primary_cat":"hep-ph","submitted_at":"2002-09-23T16:55:05Z","cross_cats_sorted":["astro-ph"],"title_canon_sha256":"4546877880a298af1710563fdb49ad24ee4ac15030e90564b38fb42c3c8c8b5a","abstract_canon_sha256":"ec947a0e801d713a62ba0340e061543ce8d9ca8973a6d28aee41a84684f6dacb"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:32:21.486737Z","signature_b64":"stIRY5g7NtzOYXBstue/8i8UmQuEkJGCjwq7Rsybv4A2f+mpUi5UfFYbOYKeqqn6nBBCzMOlMzGJWS9y6weeAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3cd3248283e2e2ab20d7326cd4c308d42c4dcf3d84b34ebc403dfb8c37a82668","last_reissued_at":"2026-07-04T15:32:21.486301Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:32:21.486301Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Elastic Scattering and Direct Detection of Kaluza-Klein Dark Matter","license":"","headline":"","cross_cats":["astro-ph"],"primary_cat":"hep-ph","authors_text":"Geraldine Servant, Tim M.P. Tait","submitted_at":"2002-09-23T16:55:05Z","abstract_excerpt":"Recently a new dark matter candidate has been proposed as a consequence of universal compact extra dimensions. It was found that to account for cosmological observations, the masses of the first Kaluza-Klein modes (and thus the approximate size of the extra dimension) should be in the range 600-1200 GeV when the lightest Kaluza-Klein particle (LKP) corresponds to the hypercharge boson and in the range 1 - 1.8 TeV when it corresponds to a neutrino. In this article, we compute the elastic scattering cross sections between Kaluza-Klein dark matter and nuclei both when the lightest Kaluza-Klein pa"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-ph/0209262","kind":"arxiv","version":4},"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/0209262/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/0209262","created_at":"2026-07-04T15:32:21.486366+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-ph/0209262v4","created_at":"2026-07-04T15:32:21.486366+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-ph/0209262","created_at":"2026-07-04T15:32:21.486366+00:00"},{"alias_kind":"pith_short_12","alias_value":"HTJSJAUD4LRK","created_at":"2026-07-04T15:32:21.486366+00:00"},{"alias_kind":"pith_short_16","alias_value":"HTJSJAUD4LRKWIGX","created_at":"2026-07-04T15:32:21.486366+00:00"},{"alias_kind":"pith_short_8","alias_value":"HTJSJAUD","created_at":"2026-07-04T15:32:21.486366+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2509.20027","citing_title":"Belle II Constraints on the Non-Minimal Universal Extra Dimensional Model","ref_index":37,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/HTJSJAUD4LRKWIGXGJWNJQYI2Q","json":"https://pith.science/pith/HTJSJAUD4LRKWIGXGJWNJQYI2Q.json","graph_json":"https://pith.science/api/pith-number/HTJSJAUD4LRKWIGXGJWNJQYI2Q/graph.json","events_json":"https://pith.science/api/pith-number/HTJSJAUD4LRKWIGXGJWNJQYI2Q/events.json","paper":"https://pith.science/paper/HTJSJAUD"},"agent_actions":{"view_html":"https://pith.science/pith/HTJSJAUD4LRKWIGXGJWNJQYI2Q","download_json":"https://pith.science/pith/HTJSJAUD4LRKWIGXGJWNJQYI2Q.json","view_paper":"https://pith.science/paper/HTJSJAUD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-ph/0209262&json=true","fetch_graph":"https://pith.science/api/pith-number/HTJSJAUD4LRKWIGXGJWNJQYI2Q/graph.json","fetch_events":"https://pith.science/api/pith-number/HTJSJAUD4LRKWIGXGJWNJQYI2Q/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HTJSJAUD4LRKWIGXGJWNJQYI2Q/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HTJSJAUD4LRKWIGXGJWNJQYI2Q/action/storage_attestation","attest_author":"https://pith.science/pith/HTJSJAUD4LRKWIGXGJWNJQYI2Q/action/author_attestation","sign_citation":"https://pith.science/pith/HTJSJAUD4LRKWIGXGJWNJQYI2Q/action/citation_signature","submit_replication":"https://pith.science/pith/HTJSJAUD4LRKWIGXGJWNJQYI2Q/action/replication_record"}},"created_at":"2026-07-04T15:32:21.486366+00:00","updated_at":"2026-07-04T15:32:21.486366+00:00"}