{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2006:N6UL6QHD5U5UOO46ASVGVFX6XW","short_pith_number":"pith:N6UL6QHD","schema_version":"1.0","canonical_sha256":"6fa8bf40e3ed3b473b9e04aa6a96febd82ebf088d01c48b9e2807572f67de80b","source":{"kind":"arxiv","id":"astro-ph/0611930","version":1},"attestation_state":"computed","paper":{"title":"The Asymptotic Form of Cosmic Structure: Small Scale Power and Accretion History","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"August E. Evrard, Fred C. Adams (University of Michigan), Michael T. Busha","submitted_at":"2006-11-30T19:56:28Z","abstract_excerpt":"We explore the effects of small scale structure on the formation and equilibrium of dark matter halos in a universe dominated by vacuum energy. We present the results of a suite of four N-body simulations, two with a LCDM initial power spectrum and two with WDM-like spectra that suppress the early formation of small structures. All simulations are run into to far future when the universe is 64Gyr/h old, long enough for halos to essentially reach dynamical equilibrium. We quantify the importance of hierarchical merging on the halo mass accretion history, the substructure population, and the equ"},"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":"astro-ph/0611930","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2006-11-30T19:56:28Z","cross_cats_sorted":[],"title_canon_sha256":"839f3254bd0cdec60710ed445574f428d01e01372840cc6ba6233db3b7cf4427","abstract_canon_sha256":"79350fb990fe4c38ba98d871ece38c4f9a5bf0fb2a46afff86323e0f6f3e7b5c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:29:15.142252Z","signature_b64":"Sm3PW+s+2PFZp4//Nx2yGM9K1W5ORsfHMoQoGi/Y/x8sUpywv4Ddj6ztsaAgGBYc8b2EvCUt4pKvtyHUydu2DA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6fa8bf40e3ed3b473b9e04aa6a96febd82ebf088d01c48b9e2807572f67de80b","last_reissued_at":"2026-05-18T04:29:15.141563Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:29:15.141563Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Asymptotic Form of Cosmic Structure: Small Scale Power and Accretion History","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"August E. Evrard, Fred C. Adams (University of Michigan), Michael T. Busha","submitted_at":"2006-11-30T19:56:28Z","abstract_excerpt":"We explore the effects of small scale structure on the formation and equilibrium of dark matter halos in a universe dominated by vacuum energy. We present the results of a suite of four N-body simulations, two with a LCDM initial power spectrum and two with WDM-like spectra that suppress the early formation of small structures. All simulations are run into to far future when the universe is 64Gyr/h old, long enough for halos to essentially reach dynamical equilibrium. We quantify the importance of hierarchical merging on the halo mass accretion history, the substructure population, and the equ"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0611930","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":""},"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":"astro-ph/0611930","created_at":"2026-05-18T04:29:15.141681+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0611930v1","created_at":"2026-05-18T04:29:15.141681+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0611930","created_at":"2026-05-18T04:29:15.141681+00:00"},{"alias_kind":"pith_short_12","alias_value":"N6UL6QHD5U5U","created_at":"2026-05-18T12:25:54.717736+00:00"},{"alias_kind":"pith_short_16","alias_value":"N6UL6QHD5U5UOO46","created_at":"2026-05-18T12:25:54.717736+00:00"},{"alias_kind":"pith_short_8","alias_value":"N6UL6QHD","created_at":"2026-05-18T12:25:54.717736+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/N6UL6QHD5U5UOO46ASVGVFX6XW","json":"https://pith.science/pith/N6UL6QHD5U5UOO46ASVGVFX6XW.json","graph_json":"https://pith.science/api/pith-number/N6UL6QHD5U5UOO46ASVGVFX6XW/graph.json","events_json":"https://pith.science/api/pith-number/N6UL6QHD5U5UOO46ASVGVFX6XW/events.json","paper":"https://pith.science/paper/N6UL6QHD"},"agent_actions":{"view_html":"https://pith.science/pith/N6UL6QHD5U5UOO46ASVGVFX6XW","download_json":"https://pith.science/pith/N6UL6QHD5U5UOO46ASVGVFX6XW.json","view_paper":"https://pith.science/paper/N6UL6QHD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0611930&json=true","fetch_graph":"https://pith.science/api/pith-number/N6UL6QHD5U5UOO46ASVGVFX6XW/graph.json","fetch_events":"https://pith.science/api/pith-number/N6UL6QHD5U5UOO46ASVGVFX6XW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/N6UL6QHD5U5UOO46ASVGVFX6XW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/N6UL6QHD5U5UOO46ASVGVFX6XW/action/storage_attestation","attest_author":"https://pith.science/pith/N6UL6QHD5U5UOO46ASVGVFX6XW/action/author_attestation","sign_citation":"https://pith.science/pith/N6UL6QHD5U5UOO46ASVGVFX6XW/action/citation_signature","submit_replication":"https://pith.science/pith/N6UL6QHD5U5UOO46ASVGVFX6XW/action/replication_record"}},"created_at":"2026-05-18T04:29:15.141681+00:00","updated_at":"2026-05-18T04:29:15.141681+00:00"}