{ "id": "1109.1661", "version": "v1", "published": "2011-09-08T08:52:29.000Z", "updated": "2011-09-08T08:52:29.000Z", "title": "Constraints on $Λ(t)$CDM models as holographic and agegraphic dark energy with the observational Hubble parameter data", "authors": [ "Zhong-Xu Zhai", "Tong-Jie Zhang", "Wen-Biao Liu" ], "comment": "20 pages, 10 figures, 3 tables", "journal": "JCAP 1108:019,2011", "doi": "10.1088/1475-7516/2011/08/019", "categories": [ "astro-ph.CO", "gr-qc" ], "abstract": "The newly released observational $H(z)$ data (OHD) is used to constrain $\\Lambda(t)$CDM models as holographic and agegraphic dark energy. By the use of the length scale and time scale as the IR cut-off including Hubble horizon (HH), future event horizon (FEH), age of the universe (AU), and conformal time (CT), we achieve four different $\\Lambda(t)$CDM models which can describe the present cosmological acceleration respectively. In order to get a comparison between such $\\Lambda(t)$CDM models and standard $\\Lambda$CDM model, we use the information criteria (IC), $Om(z)$ diagnostic, and statefinder diagnostic to measure the deviations. Furthermore, by simulating a larger Hubble parameter data sample in the redshift range of $0.1