{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:PIJEXHCXPBJEJUDPGPNAF4VZIW","short_pith_number":"pith:PIJEXHCX","schema_version":"1.0","canonical_sha256":"7a124b9c57785244d06f33da02f2b945a657f2f5d3194047ddcbc58bd90db75d","source":{"kind":"arxiv","id":"1104.2607","version":2},"attestation_state":"computed","paper":{"title":"Theoretical dark matter halo substructure","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Alberto Manrique, Eduard Salvador-Sol\\'e, Sinue Serra","submitted_at":"2011-04-13T20:09:13Z","abstract_excerpt":"In two previous papers (Salvador-Sol\\'e 2012a,b), it was shown that: i) the typical structural and kinematic properties of haloes in (bottom-up) hierarchical cosmologies endowed with random Gaussian density perturbations of dissipationless collisionless dark matter emerge naturally from the typical properties of peaks in the primordial density field and ii) halo statistics are well described by the peak formalism. In the present paper, we use these results to model halo substructure. Specifically, making use of the peak formalism and the fact that accreting haloes evolve from the inside-out, w"},"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":"1104.2607","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2011-04-13T20:09:13Z","cross_cats_sorted":[],"title_canon_sha256":"e548562a03ccfcf979efaf394974632a30f1aa71673a0968a93c70c82500c85c","abstract_canon_sha256":"c05f41fda71b27a89c7206f7f9106479a38b9084f597e97d35ac0f8e44fc1281"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:59:49.567527Z","signature_b64":"dlRWZ8QFoGsz/hj04q8s5GVkCKElddFQ3LaUUqoUsIyRm8LkSngd6OuC2ZXedE9qIqgYXRBjgxjvDIJluczWCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7a124b9c57785244d06f33da02f2b945a657f2f5d3194047ddcbc58bd90db75d","last_reissued_at":"2026-05-18T03:59:49.567080Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:59:49.567080Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Theoretical dark matter halo substructure","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Alberto Manrique, Eduard Salvador-Sol\\'e, Sinue Serra","submitted_at":"2011-04-13T20:09:13Z","abstract_excerpt":"In two previous papers (Salvador-Sol\\'e 2012a,b), it was shown that: i) the typical structural and kinematic properties of haloes in (bottom-up) hierarchical cosmologies endowed with random Gaussian density perturbations of dissipationless collisionless dark matter emerge naturally from the typical properties of peaks in the primordial density field and ii) halo statistics are well described by the peak formalism. In the present paper, we use these results to model halo substructure. Specifically, making use of the peak formalism and the fact that accreting haloes evolve from the inside-out, w"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1104.2607","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":""},"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":"1104.2607","created_at":"2026-05-18T03:59:49.567149+00:00"},{"alias_kind":"arxiv_version","alias_value":"1104.2607v2","created_at":"2026-05-18T03:59:49.567149+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1104.2607","created_at":"2026-05-18T03:59:49.567149+00:00"},{"alias_kind":"pith_short_12","alias_value":"PIJEXHCXPBJE","created_at":"2026-05-18T12:26:39.201973+00:00"},{"alias_kind":"pith_short_16","alias_value":"PIJEXHCXPBJEJUDP","created_at":"2026-05-18T12:26:39.201973+00:00"},{"alias_kind":"pith_short_8","alias_value":"PIJEXHCX","created_at":"2026-05-18T12:26:39.201973+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/PIJEXHCXPBJEJUDPGPNAF4VZIW","json":"https://pith.science/pith/PIJEXHCXPBJEJUDPGPNAF4VZIW.json","graph_json":"https://pith.science/api/pith-number/PIJEXHCXPBJEJUDPGPNAF4VZIW/graph.json","events_json":"https://pith.science/api/pith-number/PIJEXHCXPBJEJUDPGPNAF4VZIW/events.json","paper":"https://pith.science/paper/PIJEXHCX"},"agent_actions":{"view_html":"https://pith.science/pith/PIJEXHCXPBJEJUDPGPNAF4VZIW","download_json":"https://pith.science/pith/PIJEXHCXPBJEJUDPGPNAF4VZIW.json","view_paper":"https://pith.science/paper/PIJEXHCX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1104.2607&json=true","fetch_graph":"https://pith.science/api/pith-number/PIJEXHCXPBJEJUDPGPNAF4VZIW/graph.json","fetch_events":"https://pith.science/api/pith-number/PIJEXHCXPBJEJUDPGPNAF4VZIW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PIJEXHCXPBJEJUDPGPNAF4VZIW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PIJEXHCXPBJEJUDPGPNAF4VZIW/action/storage_attestation","attest_author":"https://pith.science/pith/PIJEXHCXPBJEJUDPGPNAF4VZIW/action/author_attestation","sign_citation":"https://pith.science/pith/PIJEXHCXPBJEJUDPGPNAF4VZIW/action/citation_signature","submit_replication":"https://pith.science/pith/PIJEXHCXPBJEJUDPGPNAF4VZIW/action/replication_record"}},"created_at":"2026-05-18T03:59:49.567149+00:00","updated_at":"2026-05-18T03:59:49.567149+00:00"}