Determining the Hubble Constant from Hubble Parameter Measurements

Chen, Yun; Kumar, Suresh; Ratra, Bharat

doi:10.3847/1538-4357/835/1/86

Title: Determining the Hubble Constant from Hubble Parameter Measurements

Journal Article · Fri Jan 20 00:00:00 EST 2017 · The Astrophysical Journal (Online)

DOI:https://doi.org/10.3847/1538-4357/835/1/86· OSTI ID:1532969

^[1];

^[2]; Ratra, Bharat ^[3]

Chinese Academy of Sciences, Beijing (China). National Astronomical Observatories, Key Lab. for Computational Astrophysics
Birla Institute of Technology and Science (BITS) Pilani, Rajasthan (India). Dept. of Mathematics
Kansas State Univ., Manhattan, KS (United States). Dept. of Physics

We use 28 Hubble parameter, H($$z$$), measurements at intermediate redshifts 0.07 $$\leqslant z \leqslant$$ 2.3 to determine the present-day Hubble constant H₀ in four cosmological models. We measure H₀ = 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 ( σ errors) in the ΛCDM (spatially flat and non-flat), ωCDM and ΦCDM models, respectively. These measured H₀ 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 H₀ measurements, but include the higher local measurements of H₀ within the 2σ confidence limits.

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Research Organization:: Kansas State Univ., Manhattan, KS (United States)

Sponsoring Organization:: USDOE Office of Science (SC)

Grant/Contract Number:: FG03-99ER41093

OSTI ID:: 1532969

Journal Information:: The Astrophysical Journal (Online), Vol. 835, Issue 1; ISSN 1538-4357

Publisher:: Institute of Physics (IOP)Copyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 96 works

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Constraints on quintessence scalar field models using cosmological observations Yang, Weiqiang; Shahalam, M.; Pal, Barun arXiv https://doi.org/10.48550/arxiv.1810.08586	text	January 2018
CMB tensions with low-redshift $H_0$ and $S_8$ measurements: impact of a redshift-dependent type-Ia supernovae intrinsic luminosity Martinelli, Matteo; Tutusaus, Isaac arXiv https://doi.org/10.48550/arxiv.1906.09189	text	January 2019
Quasar X-ray and UV flux, baryon acoustic oscillation, and Hubble parameter measurement constraints on cosmological model parameters Khadka, Narayan; Ratra, Bharat arXiv https://doi.org/10.48550/arxiv.1909.01400	text	January 2019

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79 ASTRONOMY AND ASTROPHYSICS
astronomy & astrophysics
cosmological parameters
dark energy

Title: Determining the Hubble Constant from Hubble Parameter Measurements

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