{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2004:OKAGE4U6SRBSU7XOFSCKOTMVP6","short_pith_number":"pith:OKAGE4U6","schema_version":"1.0","canonical_sha256":"728062729e94432a7eee2c84a74d957f9d2bb8fa946100bc59eea4594897e448","source":{"kind":"arxiv","id":"hep-ph/0408241","version":2},"attestation_state":"computed","paper":{"title":"Gravitational clustering of relic neutrinos and implications for their detection","license":"","headline":"","cross_cats":["astro-ph","hep-ex"],"primary_cat":"hep-ph","authors_text":"Andreas Ringwald, Yvonne Y. Y. Wong","submitted_at":"2004-08-23T12:55:16Z","abstract_excerpt":"We study the gravitational clustering of big bang relic neutrinos onto existing cold dark matter (CDM) and baryonic structures within the flat $\\Lambda$CDM model, using both numerical simulations and a semi-analytical linear technique, with the aim of understanding the neutrinos' clustering properties for direct detection purposes. In a comparative analysis, we find that the linear technique systematically underestimates the amount of clustering for a wide range of CDM halo and neutrino masses. This invalidates earlier claims of the technique's applicability. We then compute the exact phase sp"},"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/0408241","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"hep-ph","submitted_at":"2004-08-23T12:55:16Z","cross_cats_sorted":["astro-ph","hep-ex"],"title_canon_sha256":"8b7073bff3caa12ceb7dac6efab6df2a581909b72ee45ddc2c036c3edf61850f","abstract_canon_sha256":"6e286ebc0f044e59319cb1cf4a852d70561c7bedd380428561cdbbc98d99ff08"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:48:28.555293Z","signature_b64":"VteiIWImsfQexYYMT7QQaxc0sxzpvb/IV1z4yy9bhY9dy1+l5Z5MONVvHU966shrdRfhvrs1b/h2fvzHCywAAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"728062729e94432a7eee2c84a74d957f9d2bb8fa946100bc59eea4594897e448","last_reissued_at":"2026-07-04T16:48:28.554823Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:48:28.554823Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gravitational clustering of relic neutrinos and implications for their detection","license":"","headline":"","cross_cats":["astro-ph","hep-ex"],"primary_cat":"hep-ph","authors_text":"Andreas Ringwald, Yvonne Y. Y. Wong","submitted_at":"2004-08-23T12:55:16Z","abstract_excerpt":"We study the gravitational clustering of big bang relic neutrinos onto existing cold dark matter (CDM) and baryonic structures within the flat $\\Lambda$CDM model, using both numerical simulations and a semi-analytical linear technique, with the aim of understanding the neutrinos' clustering properties for direct detection purposes. In a comparative analysis, we find that the linear technique systematically underestimates the amount of clustering for a wide range of CDM halo and neutrino masses. This invalidates earlier claims of the technique's applicability. We then compute the exact phase sp"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-ph/0408241","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/0408241/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/0408241","created_at":"2026-07-04T16:48:28.554885+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-ph/0408241v2","created_at":"2026-07-04T16:48:28.554885+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-ph/0408241","created_at":"2026-07-04T16:48:28.554885+00:00"},{"alias_kind":"pith_short_12","alias_value":"OKAGE4U6SRBS","created_at":"2026-07-04T16:48:28.554885+00:00"},{"alias_kind":"pith_short_16","alias_value":"OKAGE4U6SRBSU7XO","created_at":"2026-07-04T16:48:28.554885+00:00"},{"alias_kind":"pith_short_8","alias_value":"OKAGE4U6","created_at":"2026-07-04T16:48:28.554885+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2607.05221","citing_title":"Pathways and impediments towards a detection of the relic neutrino wind","ref_index":47,"is_internal_anchor":true},{"citing_arxiv_id":"2605.11956","citing_title":"Probing the small-scale primordial power spectrum via relic neutrinos and acoustic reheating","ref_index":60,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/OKAGE4U6SRBSU7XOFSCKOTMVP6","json":"https://pith.science/pith/OKAGE4U6SRBSU7XOFSCKOTMVP6.json","graph_json":"https://pith.science/api/pith-number/OKAGE4U6SRBSU7XOFSCKOTMVP6/graph.json","events_json":"https://pith.science/api/pith-number/OKAGE4U6SRBSU7XOFSCKOTMVP6/events.json","paper":"https://pith.science/paper/OKAGE4U6"},"agent_actions":{"view_html":"https://pith.science/pith/OKAGE4U6SRBSU7XOFSCKOTMVP6","download_json":"https://pith.science/pith/OKAGE4U6SRBSU7XOFSCKOTMVP6.json","view_paper":"https://pith.science/paper/OKAGE4U6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-ph/0408241&json=true","fetch_graph":"https://pith.science/api/pith-number/OKAGE4U6SRBSU7XOFSCKOTMVP6/graph.json","fetch_events":"https://pith.science/api/pith-number/OKAGE4U6SRBSU7XOFSCKOTMVP6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OKAGE4U6SRBSU7XOFSCKOTMVP6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OKAGE4U6SRBSU7XOFSCKOTMVP6/action/storage_attestation","attest_author":"https://pith.science/pith/OKAGE4U6SRBSU7XOFSCKOTMVP6/action/author_attestation","sign_citation":"https://pith.science/pith/OKAGE4U6SRBSU7XOFSCKOTMVP6/action/citation_signature","submit_replication":"https://pith.science/pith/OKAGE4U6SRBSU7XOFSCKOTMVP6/action/replication_record"}},"created_at":"2026-07-04T16:48:28.554885+00:00","updated_at":"2026-07-04T16:48:28.554885+00:00"}