Prospect for Cosmological Parameter Estimation Using Future Hubble Parameter Measurements**Supported by the National Natural Science Foundation of China under Grant Nos. 11522540, 11690021, 11375153, 11675145, and the National Program for Support of Top-Notch Young Professionals, and the 2016 Program for Postdoctoral Fellowship of Zhejiang Province

Abstract

We constrain cosmological parameters using only Hubble parameter data and quantify the impact of future Hubble parameter measurements on parameter estimation for the most typical dark energy models. We first constrain cosmological parameters using 52 current Hubble parameter data including the Hubble constant measurement from the Hubble Space Telescope. Then we simulate the baryon acoustic oscillation signals from WFIRST (Wide-Field Infrared Survey Telescope) covering the redshift range of z ∈ [0.5, 2] and the redshift drift data from E-ELT (European Extremely Large Telescope) in the redshift range of z ∈ [2,5]. It is shown that solely using the current Hubble parameter data could give fairly good constraints on cosmological parameters. Compared to the current Hubble parameter data, with the WFIRST observation the H(z) constraints on dark energy would be improved slightly, while with the E-ELT observation the H(z) constraints on dark energy is enormously improved.