{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:KQQPLJ6JZLLVBAFR5DM4IP5Y5E","short_pith_number":"pith:KQQPLJ6J","schema_version":"1.0","canonical_sha256":"5420f5a7c9cad75080b1e8d9c43fb8e925234b0f0b810e207b9b8d1eef548166","source":{"kind":"arxiv","id":"1104.5040","version":1},"attestation_state":"computed","paper":{"title":"The abundance of galaxy clusters in MOND: Cosmological simulations with massive neutrinos","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Antonaldo Diaferio, Garry W. Angus","submitted_at":"2011-04-26T22:18:31Z","abstract_excerpt":"We present a new Particle-Mesh cosmological N-body code for accurately solving the modified Poisson equation of the Quasi Linear formulation of MOND. We generate initial conditions for the Angus (2009) cosmological model, which is identical to LCDM except that the cold dark matter is switched for a single species of thermal sterile neutrinos. We set the initial conditions at z=250 for a (512 Mpc/h)^3 box with 256^3 particles and we evolve them down to z=0. We clearly demonstrate the necessity of MOND for developing the large scale structure in a hot dark matter cosmology and contradict the nai"},"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":"1104.5040","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2011-04-26T22:18:31Z","cross_cats_sorted":[],"title_canon_sha256":"c687e1731cd356a65cac31dc52c621a28f977e6b481ee1281a992beab32383f7","abstract_canon_sha256":"eb894b5c09b881ca86d9a4e0c6b5a054478172a5b5fbd348d5619b60de008c66"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:02:14.455851Z","signature_b64":"VtjIOtlF2X7fAz/lFPoYW00lemSYt8auRIjclisg+To4p4tSQgSfzO583elTkier+kLyrh4Qf4ABsuIuz6v0Dw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5420f5a7c9cad75080b1e8d9c43fb8e925234b0f0b810e207b9b8d1eef548166","last_reissued_at":"2026-05-18T02:02:14.454834Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:02:14.454834Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The abundance of galaxy clusters in MOND: Cosmological simulations with massive neutrinos","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Antonaldo Diaferio, Garry W. Angus","submitted_at":"2011-04-26T22:18:31Z","abstract_excerpt":"We present a new Particle-Mesh cosmological N-body code for accurately solving the modified Poisson equation of the Quasi Linear formulation of MOND. We generate initial conditions for the Angus (2009) cosmological model, which is identical to LCDM except that the cold dark matter is switched for a single species of thermal sterile neutrinos. We set the initial conditions at z=250 for a (512 Mpc/h)^3 box with 256^3 particles and we evolve them down to z=0. We clearly demonstrate the necessity of MOND for developing the large scale structure in a hot dark matter cosmology and contradict the nai"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1104.5040","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":"1104.5040","created_at":"2026-05-18T02:02:14.455002+00:00"},{"alias_kind":"arxiv_version","alias_value":"1104.5040v1","created_at":"2026-05-18T02:02:14.455002+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1104.5040","created_at":"2026-05-18T02:02:14.455002+00:00"},{"alias_kind":"pith_short_12","alias_value":"KQQPLJ6JZLLV","created_at":"2026-05-18T12:26:34.985390+00:00"},{"alias_kind":"pith_short_16","alias_value":"KQQPLJ6JZLLVBAFR","created_at":"2026-05-18T12:26:34.985390+00:00"},{"alias_kind":"pith_short_8","alias_value":"KQQPLJ6J","created_at":"2026-05-18T12:26:34.985390+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/KQQPLJ6JZLLVBAFR5DM4IP5Y5E","json":"https://pith.science/pith/KQQPLJ6JZLLVBAFR5DM4IP5Y5E.json","graph_json":"https://pith.science/api/pith-number/KQQPLJ6JZLLVBAFR5DM4IP5Y5E/graph.json","events_json":"https://pith.science/api/pith-number/KQQPLJ6JZLLVBAFR5DM4IP5Y5E/events.json","paper":"https://pith.science/paper/KQQPLJ6J"},"agent_actions":{"view_html":"https://pith.science/pith/KQQPLJ6JZLLVBAFR5DM4IP5Y5E","download_json":"https://pith.science/pith/KQQPLJ6JZLLVBAFR5DM4IP5Y5E.json","view_paper":"https://pith.science/paper/KQQPLJ6J","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1104.5040&json=true","fetch_graph":"https://pith.science/api/pith-number/KQQPLJ6JZLLVBAFR5DM4IP5Y5E/graph.json","fetch_events":"https://pith.science/api/pith-number/KQQPLJ6JZLLVBAFR5DM4IP5Y5E/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KQQPLJ6JZLLVBAFR5DM4IP5Y5E/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KQQPLJ6JZLLVBAFR5DM4IP5Y5E/action/storage_attestation","attest_author":"https://pith.science/pith/KQQPLJ6JZLLVBAFR5DM4IP5Y5E/action/author_attestation","sign_citation":"https://pith.science/pith/KQQPLJ6JZLLVBAFR5DM4IP5Y5E/action/citation_signature","submit_replication":"https://pith.science/pith/KQQPLJ6JZLLVBAFR5DM4IP5Y5E/action/replication_record"}},"created_at":"2026-05-18T02:02:14.455002+00:00","updated_at":"2026-05-18T02:02:14.455002+00:00"}