{"paper":{"title":"The large-scale structure in a universe dominated by cold plus hot dark matter","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"G. Boerner, H.J. Mo, L.Z. Fang, Y.P. Jing","submitted_at":"1993-08-12T21:45:58Z","abstract_excerpt":"Using numerical simulations, we investigate the large-scale gravitational clustering in a flat universe dominated by cold plus hot dark matter (i.e., $\\Omega_0=\\ocdm+\\ohdm+\\obaryon=1$). Primordial density fluctuation spectrum is taken to have the Zel'dovich-Harrison form. Three models are studied, with Model I having $\\ocdm=0.69$, $\\obaryon=0.01$, and $\\ohdm=0.30$ in one flavor of neutrinos; Model II having $\\ocdm=0.60$, $\\obaryon=0.10$, and $\\ohdm=0.30$ in one flavor of neutrinos; Model III having $\\ocdm=0.69$, $\\obaryon=0.01$, and $\\ohdm=0.30$ in three flavors of neutrinos. The initial densi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/9308017","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"}