{"paper":{"title":"The largest virialized dark halo in the universe","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Li Chen, Tong-Jie Zhang, Wei Zhou, Xiang-Tao He, Yu-Mei Huang","submitted_at":"2002-04-29T05:12:43Z","abstract_excerpt":"Using semi-analytic approach, we present an estimate of the properties of the largest virialized dark halos in the present universe for three different scenarios of structure formation: SCDM, LCDM and OCDM models. The resulting virial mass and temperature increase from the lowest values of $1.6 \\times 10^{15}h^{-1}M_{\\odot}$ and 9.8 keV in OCDM, the mid-range values of $9.0 \\times 10^{15}h^{-1}M_{\\odot}$ and 31 keV in LCDM, to the highest values of $20.9 \\times 10^{15}h^{-1}M_{\\odot}$, 65 keV in SCDM. As compared with the largest virialized object seen in the universe, the richest clusters of "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0204480","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/astro-ph/0204480/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"}