{"paper":{"title":"Reexploration of interacting holographic dark energy model: Cases of interaction term excluding the Hubble parameter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Hai-Li Li, Jing-Fei Zhang, Lu Feng, Xin Zhang","submitted_at":"2017-11-15T10:23:27Z","abstract_excerpt":"In this paper, we make a deep analysis for the five typical interacting holographic dark energy models with the interaction terms $Q=3\\beta H_{0}\\rho_{\\rm{de}}$, $Q=3\\beta H_{0}\\rho_{\\rm{c}}$, $Q=3\\beta H_{0}(\\rho_{\\rm{de}}+\\rho_{\\rm c})$, $Q=3\\beta H_{0}\\sqrt{\\rho_{\\rm{de}}\\rho_{\\rm c}}$, and $Q=3\\beta H_{0}\\frac{\\rho_{\\rm{de}}\\rho_{c}}{\\rho_{\\rm{de}}+\\rho_{\\rm c}}$, respectively. We obtain observational constraints on these models by using the type Ia supernova data (the Joint Light-curve Analysis sample), the cosmic microwave background data (Planck 2015 distance priors), the baryon acousti"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.06159","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"}