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• W2199601775 abstract "Dark energy affects the Hubble expansion rate (namely, the expansion history) $H(z)$ by an integral over $w(z)$. However, the usual observables are the luminosity distances or the angular diameter distances, which measure the distance-redshift relation. Actually, dark energy affects the distances (and the growth factor) by a further integration over functions of $H(z)$. Thus, the direct measurements of the Hubble parameter $H(z)$ at different redshifts are of great importance for constraining the properties of dark energy. In this paper, we show how the typical dark energy models, for example, the $Lambda$CDM, $w$CDM, CPL, and holographic dark energy (HDE) models, can be constrained by the current direct measurements of $H(z)$ (31 data in total, covering the redshift range of $zin [0.07,2.34]$). In fact, the future redshift-drift observations (also referred to as the Sandage-Loeb test) can also directly measure $H(z)$ at higher redshifts, covering the range of $zin [2,5]$. We thus discuss what role the redshift-drift observations can play in constraining dark energy with the Hubble parameter measurements. We show that the constraints on dark energy can be improved greatly with the $H(z)$ data from only a 10-year observation of redshift drift." @default.
• W2199601775 created "2016-06-24" @default.
• W2199601775 creator A5020810072 @default.
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• W2199601775 date "2016-03-01" @default.
• W2199601775 modified "2023-09-27" @default.
• W2199601775 title "Constraining dark energy with Hubble parameter measurements: an analysis including future redshift-drift observations" @default.
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• W2199601775 doi "https://doi.org/10.1140/epjc/s10052-016-4016-x" @default.
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