{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2002:MWG7W33B7MHW6RM6HYHKPHADKM","short_pith_number":"pith:MWG7W33B","schema_version":"1.0","canonical_sha256":"658dfb6f61fb0f6f459e3e0ea79c0353133964a9b54bd9f31d243003b9e755fd","source":{"kind":"arxiv","id":"hep-ph/0206071","version":2},"attestation_state":"computed","paper":{"title":"Is the Lightest Kaluza-Klein Particle a Viable Dark Matter Candidate?","license":"","headline":"","cross_cats":["astro-ph","hep-th"],"primary_cat":"hep-ph","authors_text":"Geraldine Servant, Tim M.P. Tait","submitted_at":"2002-06-06T16:59:25Z","abstract_excerpt":"In models with universal extra dimensions (i.e. in which all Standard Model fields, including fermions, propagate into compact extra dimensions) momentum conservation in the extra dimensions leads to the conservation of Kaluza--Klein (KK) number at each vertex. KK number is violated by loop effects because of the orbifold imposed to reproduce the chiral Standard Model with zero modes, however, a KK parity remains at any order in perturbation theory which leads to the existence of a stable lightest KK particle (LKP). In addition, the degeneracy in the KK spectrum is lifted by radiative correcti"},"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/0206071","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"hep-ph","submitted_at":"2002-06-06T16:59:25Z","cross_cats_sorted":["astro-ph","hep-th"],"title_canon_sha256":"623ad0a087ff7ba0b2580eee6e885007735ab1ccee0ddf3bca60f9c05ebdf107","abstract_canon_sha256":"fd3897abde26debc8dd737d7d216db26495e8ffacddc9714608c639520c6b068"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:32:21.010308Z","signature_b64":"tA4U/vIlnm7p1EAL06eTCoFZJzCB3O1C8ZU+bWFW3d8PxBNNr5t2lQG6gR2j7/KrwjR+SYxbwSjCSUKeSL+hDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"658dfb6f61fb0f6f459e3e0ea79c0353133964a9b54bd9f31d243003b9e755fd","last_reissued_at":"2026-07-04T15:32:21.009900Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:32:21.009900Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Is the Lightest Kaluza-Klein Particle a Viable Dark Matter Candidate?","license":"","headline":"","cross_cats":["astro-ph","hep-th"],"primary_cat":"hep-ph","authors_text":"Geraldine Servant, Tim M.P. Tait","submitted_at":"2002-06-06T16:59:25Z","abstract_excerpt":"In models with universal extra dimensions (i.e. in which all Standard Model fields, including fermions, propagate into compact extra dimensions) momentum conservation in the extra dimensions leads to the conservation of Kaluza--Klein (KK) number at each vertex. KK number is violated by loop effects because of the orbifold imposed to reproduce the chiral Standard Model with zero modes, however, a KK parity remains at any order in perturbation theory which leads to the existence of a stable lightest KK particle (LKP). In addition, the degeneracy in the KK spectrum is lifted by radiative correcti"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-ph/0206071","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/0206071/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/0206071","created_at":"2026-07-04T15:32:21.009959+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-ph/0206071v2","created_at":"2026-07-04T15:32:21.009959+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-ph/0206071","created_at":"2026-07-04T15:32:21.009959+00:00"},{"alias_kind":"pith_short_12","alias_value":"MWG7W33B7MHW","created_at":"2026-07-04T15:32:21.009959+00:00"},{"alias_kind":"pith_short_16","alias_value":"MWG7W33B7MHW6RM6","created_at":"2026-07-04T15:32:21.009959+00:00"},{"alias_kind":"pith_short_8","alias_value":"MWG7W33B","created_at":"2026-07-04T15:32:21.009959+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":4,"sample":[{"citing_arxiv_id":"1907.08010","citing_title":"Cosmological searches for the neutrino mass scale and mass ordering","ref_index":208,"is_internal_anchor":true},{"citing_arxiv_id":"2507.13432","citing_title":"INTEGRAL, eROSITA and Voyager Constraints on Light Bosonic Dark Matter: ALPs, Dark Photons, Scalars, $B-L$ and $L_{i}-L_{j}$ Vectors","ref_index":78,"is_internal_anchor":true},{"citing_arxiv_id":"2509.20027","citing_title":"Belle II Constraints on the Non-Minimal Universal Extra Dimensional Model","ref_index":38,"is_internal_anchor":true},{"citing_arxiv_id":"2510.18958","citing_title":"Sensitivity forecasts for gravitational-wave detectors to dark matter decaying into gravitons","ref_index":3,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/MWG7W33B7MHW6RM6HYHKPHADKM","json":"https://pith.science/pith/MWG7W33B7MHW6RM6HYHKPHADKM.json","graph_json":"https://pith.science/api/pith-number/MWG7W33B7MHW6RM6HYHKPHADKM/graph.json","events_json":"https://pith.science/api/pith-number/MWG7W33B7MHW6RM6HYHKPHADKM/events.json","paper":"https://pith.science/paper/MWG7W33B"},"agent_actions":{"view_html":"https://pith.science/pith/MWG7W33B7MHW6RM6HYHKPHADKM","download_json":"https://pith.science/pith/MWG7W33B7MHW6RM6HYHKPHADKM.json","view_paper":"https://pith.science/paper/MWG7W33B","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-ph/0206071&json=true","fetch_graph":"https://pith.science/api/pith-number/MWG7W33B7MHW6RM6HYHKPHADKM/graph.json","fetch_events":"https://pith.science/api/pith-number/MWG7W33B7MHW6RM6HYHKPHADKM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MWG7W33B7MHW6RM6HYHKPHADKM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MWG7W33B7MHW6RM6HYHKPHADKM/action/storage_attestation","attest_author":"https://pith.science/pith/MWG7W33B7MHW6RM6HYHKPHADKM/action/author_attestation","sign_citation":"https://pith.science/pith/MWG7W33B7MHW6RM6HYHKPHADKM/action/citation_signature","submit_replication":"https://pith.science/pith/MWG7W33B7MHW6RM6HYHKPHADKM/action/replication_record"}},"created_at":"2026-07-04T15:32:21.009959+00:00","updated_at":"2026-07-04T15:32:21.009959+00:00"}