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arXiv · 1606.07316

Determining the Hubble constant from Hubble parameter measurements

Yun Chen·Suresh Kumar·Bharat Ratra
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Abstract

We use 28 Hubble parameter, $H(z)$, measurements at intermediate redshifts $0.07 \leq z \leq 2.3$ to determine the present-day Hubble constant $H_0$ in four cosmological models. We measure $H_0 = 68.3^{ +2.7}_{ -2.6 }, 68.4^{ +2.9 }_{ -3.3 }, 65.0^{ +6.5 }_{ -6.6 }$ and $ 67.9^{ +2.4}_{-2.4}$ km s${}^{-1}$ Mpc${}^{-1}$ (1$\sigma$ errors) in the $\Lambda$CDM (spatially flat and non-flat), $\omega$CDM and $\phi$CDM models, respectively. These measured $H_0$ values are more consistent with the lower values determined from recent cosmic microwave background and baryon acoustic oscillation data, as well as with that found from a median statistics analysis of Huchra's compilation of $H_0$ measurements,but include the higher local measurements of $H_0$ within the 2$\sigma$ confidence limits.

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Yun Chen, Suresh Kumar, Bharat Ratra. 2016-06-23. Determining the Hubble constant from Hubble parameter measurements. https://doi.org/10.3847/1538-4357%2F835%2F1%2F86

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