{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2002:EO4OHLEQWTZCLBHVCWEFD6AEB3","short_pith_number":"pith:EO4OHLEQ","schema_version":"1.0","canonical_sha256":"23b8e3ac90b4f22584f5158851f8040ecf0c0b5c86d1e82f8c48fe1ccedf0058","source":{"kind":"arxiv","id":"hep-ph/0209277","version":1},"attestation_state":"computed","paper":{"title":"Detection Rates for Kaluza-Klein Dark Matter","license":"","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Debasish Majumdar","submitted_at":"2002-09-24T11:08:27Z","abstract_excerpt":"We consider the lightest Kaluza-Klein particle at N=1 mode (LKP) of universal extra dimension to be the candidate for Dark Matter and predict the detection rates for such particles for Germenium and NaI detectors. We have also calculated the nature of annual modulation for the signals in these two types of detectors for LKP Dark Matter. The rates with different values of speed of solar system in the Galactic rest frame are also evaluated."},"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/0209277","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"hep-ph","submitted_at":"2002-09-24T11:08:27Z","cross_cats_sorted":[],"title_canon_sha256":"ea5d8b0a6cf96fbbb2b9e1a4cb2adf0c2579b7f40949a014ec6633dabce78043","abstract_canon_sha256":"023861f8efda7a1c91b81a9d9392f3ba5c5e4438363342a5f671fca763c856be"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:34:21.124307Z","signature_b64":"CmWCkiu17cOLjDk756TOeh/zNamYHeOUFIlUpDV7fedBqJ9tEMqUApT3HEFMUMdrti4czEMu+koIviGXCISvAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"23b8e3ac90b4f22584f5158851f8040ecf0c0b5c86d1e82f8c48fe1ccedf0058","last_reissued_at":"2026-07-04T16:34:21.123968Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:34:21.123968Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Detection Rates for Kaluza-Klein Dark Matter","license":"","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Debasish Majumdar","submitted_at":"2002-09-24T11:08:27Z","abstract_excerpt":"We consider the lightest Kaluza-Klein particle at N=1 mode (LKP) of universal extra dimension to be the candidate for Dark Matter and predict the detection rates for such particles for Germenium and NaI detectors. We have also calculated the nature of annual modulation for the signals in these two types of detectors for LKP Dark Matter. The rates with different values of speed of solar system in the Galactic rest frame are also evaluated."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-ph/0209277","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/hep-ph/0209277/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/0209277","created_at":"2026-07-04T16:34:21.124028+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-ph/0209277v1","created_at":"2026-07-04T16:34:21.124028+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-ph/0209277","created_at":"2026-07-04T16:34:21.124028+00:00"},{"alias_kind":"pith_short_12","alias_value":"EO4OHLEQWTZC","created_at":"2026-07-04T16:34:21.124028+00:00"},{"alias_kind":"pith_short_16","alias_value":"EO4OHLEQWTZCLBHV","created_at":"2026-07-04T16:34:21.124028+00:00"},{"alias_kind":"pith_short_8","alias_value":"EO4OHLEQ","created_at":"2026-07-04T16:34:21.124028+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":40,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/EO4OHLEQWTZCLBHVCWEFD6AEB3","json":"https://pith.science/pith/EO4OHLEQWTZCLBHVCWEFD6AEB3.json","graph_json":"https://pith.science/api/pith-number/EO4OHLEQWTZCLBHVCWEFD6AEB3/graph.json","events_json":"https://pith.science/api/pith-number/EO4OHLEQWTZCLBHVCWEFD6AEB3/events.json","paper":"https://pith.science/paper/EO4OHLEQ"},"agent_actions":{"view_html":"https://pith.science/pith/EO4OHLEQWTZCLBHVCWEFD6AEB3","download_json":"https://pith.science/pith/EO4OHLEQWTZCLBHVCWEFD6AEB3.json","view_paper":"https://pith.science/paper/EO4OHLEQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-ph/0209277&json=true","fetch_graph":"https://pith.science/api/pith-number/EO4OHLEQWTZCLBHVCWEFD6AEB3/graph.json","fetch_events":"https://pith.science/api/pith-number/EO4OHLEQWTZCLBHVCWEFD6AEB3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EO4OHLEQWTZCLBHVCWEFD6AEB3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EO4OHLEQWTZCLBHVCWEFD6AEB3/action/storage_attestation","attest_author":"https://pith.science/pith/EO4OHLEQWTZCLBHVCWEFD6AEB3/action/author_attestation","sign_citation":"https://pith.science/pith/EO4OHLEQWTZCLBHVCWEFD6AEB3/action/citation_signature","submit_replication":"https://pith.science/pith/EO4OHLEQWTZCLBHVCWEFD6AEB3/action/replication_record"}},"created_at":"2026-07-04T16:34:21.124028+00:00","updated_at":"2026-07-04T16:34:21.124028+00:00"}