{"paper":{"title":"Diagnosing $\\Lambda$HDE model with statefinder hierarchy and fractional growth parameter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Lanjun Zhou, Shuang Wang","submitted_at":"2016-02-06T04:18:53Z","abstract_excerpt":"Recently, a new dark energy model called $\\Lambda$HDE was proposed. In this model, dark energy consists of two parts: cosmological constant $\\Lambda$ and holographic dark energy (HDE). Two key parameters of this model are the fractional density of cosmological constant $\\Omega_{\\Lambda0}$, and the dimensionless HDE parameter $c$. Since these two parameters determine the dynamical properties of DE and the destiny of universe, it is important to study the impacts of different values of $\\Omega_{\\Lambda0}$ and $c$ on the $\\Lambda$HDE model. In this paper, we apply various DE diagnostic tools to d"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1602.02213","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"}