{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2008:7IFDDZXKOPMYAFDN4CIGBYANJO","short_pith_number":"pith:7IFDDZXK","schema_version":"1.0","canonical_sha256":"fa0a31e6ea73d980146de09060e00d4b8019dbc34af6de57f45317b11d574412","source":{"kind":"arxiv","id":"0805.1244","version":2},"attestation_state":"computed","paper":{"title":"Clumps and streams in the local dark matter distribution","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph","authors_text":"B. Moore, D. Potter, J. Diemand, J. Stadel, M. Kuhlen, M. Zemp, P. Madau","submitted_at":"2008-05-08T21:27:53Z","abstract_excerpt":"In cold dark matter cosmological models, structures form and grow by merging of smaller units. Numerical simulations have shown that such merging is incomplete; the inner cores of halos survive and orbit as \"subhalos\" within their hosts. Here we report a simulation that resolves such substructure even in the very inner regions of the Galactic halo. We find hundreds of very concentrated dark matter clumps surviving near the solar circle, as well as numerous cold streams. The simulation reveals the fractal nature of dark matter clustering: Isolated halos and subhalos contain the same relative am"},"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":"0805.1244","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph","submitted_at":"2008-05-08T21:27:53Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"3415f12b9017f725d5ae8d670c20349cc46be7f9156d38cc2d1e810991b9c856","abstract_canon_sha256":"6b645b177f9932a64c6f360d1df2473b3c0a039e2beea3edbec356feb96b6491"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T17:24:59.440403Z","signature_b64":"ooGmy/1fuWxJqRtqpROGU4clsf9/JGB4gX02R2xY5TW0Z6PvH6stUW4TO/w01VDt75vHrcSdyxAOcvnaX4kZAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"fa0a31e6ea73d980146de09060e00d4b8019dbc34af6de57f45317b11d574412","last_reissued_at":"2026-07-04T17:24:59.439895Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T17:24:59.439895Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Clumps and streams in the local dark matter distribution","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph","authors_text":"B. Moore, D. Potter, J. Diemand, J. Stadel, M. Kuhlen, M. Zemp, P. Madau","submitted_at":"2008-05-08T21:27:53Z","abstract_excerpt":"In cold dark matter cosmological models, structures form and grow by merging of smaller units. Numerical simulations have shown that such merging is incomplete; the inner cores of halos survive and orbit as \"subhalos\" within their hosts. Here we report a simulation that resolves such substructure even in the very inner regions of the Galactic halo. We find hundreds of very concentrated dark matter clumps surviving near the solar circle, as well as numerous cold streams. The simulation reveals the fractal nature of dark matter clustering: Isolated halos and subhalos contain the same relative am"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0805.1244","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/0805.1244/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":"0805.1244","created_at":"2026-07-04T17:24:59.439973+00:00"},{"alias_kind":"arxiv_version","alias_value":"0805.1244v2","created_at":"2026-07-04T17:24:59.439973+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0805.1244","created_at":"2026-07-04T17:24:59.439973+00:00"},{"alias_kind":"pith_short_12","alias_value":"7IFDDZXKOPMY","created_at":"2026-07-04T17:24:59.439973+00:00"},{"alias_kind":"pith_short_16","alias_value":"7IFDDZXKOPMYAFDN","created_at":"2026-07-04T17:24:59.439973+00:00"},{"alias_kind":"pith_short_8","alias_value":"7IFDDZXK","created_at":"2026-07-04T17:24:59.439973+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":5,"internal_anchor_count":3,"sample":[{"citing_arxiv_id":"2607.00077","citing_title":"Hot or Cold? Radial Redistribution of Stars in FIRE Simulations of Milky Way-Mass Galaxies and the Asymmetry of Inward versus Outward Migrators","ref_index":287,"is_internal_anchor":true},{"citing_arxiv_id":"1906.11896","citing_title":"Unidentified Gamma-ray Sources as Targets for Indirect Dark Matter Detection with the Fermi-Large Area Telescope","ref_index":7,"is_internal_anchor":true},{"citing_arxiv_id":"2601.05351","citing_title":"Dipole Radiation and Kinetic Mixing from Dark Photon Solitons","ref_index":102,"is_internal_anchor":true},{"citing_arxiv_id":"2604.26072","citing_title":"Caught in the Cosmic Web: Environmental Impacts on the Halo Substructure Boosts to Dark Matter Annihilation Signals","ref_index":40,"is_internal_anchor":false},{"citing_arxiv_id":"2604.13930","citing_title":"Bayesian Analysis of Gravitational Wave Microlensing Effects from Galactic Double White Dwarfs","ref_index":60,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/7IFDDZXKOPMYAFDN4CIGBYANJO","json":"https://pith.science/pith/7IFDDZXKOPMYAFDN4CIGBYANJO.json","graph_json":"https://pith.science/api/pith-number/7IFDDZXKOPMYAFDN4CIGBYANJO/graph.json","events_json":"https://pith.science/api/pith-number/7IFDDZXKOPMYAFDN4CIGBYANJO/events.json","paper":"https://pith.science/paper/7IFDDZXK"},"agent_actions":{"view_html":"https://pith.science/pith/7IFDDZXKOPMYAFDN4CIGBYANJO","download_json":"https://pith.science/pith/7IFDDZXKOPMYAFDN4CIGBYANJO.json","view_paper":"https://pith.science/paper/7IFDDZXK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0805.1244&json=true","fetch_graph":"https://pith.science/api/pith-number/7IFDDZXKOPMYAFDN4CIGBYANJO/graph.json","fetch_events":"https://pith.science/api/pith-number/7IFDDZXKOPMYAFDN4CIGBYANJO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7IFDDZXKOPMYAFDN4CIGBYANJO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7IFDDZXKOPMYAFDN4CIGBYANJO/action/storage_attestation","attest_author":"https://pith.science/pith/7IFDDZXKOPMYAFDN4CIGBYANJO/action/author_attestation","sign_citation":"https://pith.science/pith/7IFDDZXKOPMYAFDN4CIGBYANJO/action/citation_signature","submit_replication":"https://pith.science/pith/7IFDDZXKOPMYAFDN4CIGBYANJO/action/replication_record"}},"created_at":"2026-07-04T17:24:59.439973+00:00","updated_at":"2026-07-04T17:24:59.439973+00:00"}