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 · Astrophysical Journal

DOI:https://doi.org/10.3847/1538-4357/835/1/86· OSTI ID:22869365

Chen, Yun ^[1]; Kumar, Suresh ^[2]; Ratra, Bharat ^[3]

Key Laboratory for Computational Astrophysics, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100012 (China)
Department of Mathematics, BITS Pilani, Pilani Campus, Rajasthan-333031 (India)
Department of Physics, Kansas State University, 116 Cardwell Hall, Manhattan, KS 66506 (United States)

We use 28 measurements of the Hubble parameter, H(z), at intermediate redshifts 0.07⩽z⩽2.3 to determine the present-day Hubble constant H{sub 0} in four cosmological models. We measure H{sub 0}=68.3{sub −2.6}{sup +2.7},68.4{sub −3.3}{sup +2.9},65.0{sub −6.6}{sup +6.5}, and 67.9{sub −2.4}{sup +2.4} km s{sup −1} Mpc{sup −1} (1σ errors) in the ΛCDM (spatially flat and non-flat), ωCDM, and ϕCDM models, respectively. These measured H{sub 0} values are more consistent with the lower values determined from recent data on the cosmic microwave background and baryon acoustic oscillations, as well as with the value found from a median statistical analysis of Huchra’s compilation of H{sub 0} measurements, but include the higher local measurements of H{sub 0} within the 2σ confidence limits.

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OSTI ID:: 22869365

Journal Information:: Astrophysical Journal, Vol. 835, Issue 1; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 0004-637X

Country of Publication:: United States

Language:: English

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Inflation in a closed universe Ratra, Bharat arXiv https://doi.org/10.48550/arxiv.1707.03439	text	January 2017
Planck 2015 constraints on the non-flat XCDM inflation model Ooba, Junpei; Ratra, Bharat; Sugiyama, Naoshi arXiv https://doi.org/10.48550/arxiv.1710.03271	text	January 2017
Dynamical effects of the scale invariance of the empty space: The fall of dark matter ? Maeder, Andre arXiv https://doi.org/10.48550/arxiv.1710.11425	text	January 2017
Dark Energy Survey Year 1 Results: A Precise H0 Measurement from DES Y1, BAO, and D/H Data Collaboration, Des; Abbott, T. M. C.; Abdalla, F. B. arXiv https://doi.org/10.48550/arxiv.1711.00403	text	January 2017
$H_0$ from cosmic chronometers and Type Ia supernovae, with Gaussian Processes and the novel Weighted Polynomial Regression method Gómez-Valent, Adrià; Amendola, Luca arXiv https://doi.org/10.48550/arxiv.1802.01505	text	January 2018
Observational constraints on the tilted flat-XCDM and the untilted nonflat XCDM dynamical dark energy inflation parameterizations Park, Chan-Gyung; Ratra, Bharat arXiv https://doi.org/10.48550/arxiv.1803.05522	text	January 2018
Updated Bounds on Sum of Neutrino Masses in Various Cosmological Scenarios Choudhury, Shouvik Roy; Choubey, Sandhya arXiv https://doi.org/10.48550/arxiv.1806.10832	text	January 2018
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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