{"paper":{"title":"Reconstruction of new holographic scalar field models of dark energy in Brans-Dicke Universe","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"gr-qc","authors_text":"Dandan Zhang, Jian Li, Limin Song, Weiqiang Yang, Xiaogang Wang, Yabo Wu, Yangyang Su","submitted_at":"2013-11-22T03:07:03Z","abstract_excerpt":"Motivated by the work [K. Karami, J. Fehri, {{\\it Phys. Lett. B}} {\\bf 684}, 61 (2010)] and [A. Sheykhi, {{\\it Phys. Lett. B}} {\\bf 681}, 205 (2009)], we generalize their work to the new holographic dark energy model with $\\rho_D=\\frac{3\\phi^2}{4\\omega}(\\mu H^2+\\nu\\dot{H})$ in the framework of Brans-Dicke cosmology. Concretely, we study the correspondence between the quintessence, tachyon, K-essence, dilaton scalar field and Chaplygin gas model with the new holographic dark energy model in the non-flat Brans-Dicke universe. Furthermore, we reconstruct the potentials and dynamics for these mode"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1311.5884","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"}