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Title: Baryon acoustic oscillation, Hubble parameter, and angular size measurement constraints on the Hubble constant, dark energy dynamics, and spatial curvature

Journal Article · · Monthly Notices of the Royal Astronomical Society
 [1];  [2];  [1]
  1. Department of Physics, Kansas State University, 116 Cardwell Hall, Manhattan, KS 66502, USA
  2. Key Laboratory for Computational Astrophysics, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100012, China
+ Show Author Affiliations

ABSTRACT In this paper, we use all available baryon acoustic oscillation, Hubble parameter, and quasar angular size data to constrain six dark energy cosmological models, both spatially flat and non-flat. Depending on the model and data combination considered, these data mildly favour closed spatial hypersurfaces (by as much as 1.7σ) and dark energy dynamics (up to a little over 2σ) over a cosmological constant Λ. The data also favour, at 1.8σ to 3.4σ, depending on the model and data combination, a lower Hubble constant than what is measured from the local expansion rate.

Research Organization:
Kansas State Univ., Manhattan, KS (United States)
Sponsoring Organization:
USDOE Office of Science (SC), High Energy Physics (HEP); National Natural Science Foundation of China (NSFC); National Science Foundation (NSF)
Grant/Contract Number:
SC0019038; 11703034; 11773032; 11573031; CNS-1006860; EPS-1006860; EPS-0919443
OSTI ID:
1546872
Alternate ID(s):
OSTI ID: 1642542
Journal Information:
Monthly Notices of the Royal Astronomical Society, Journal Name: Monthly Notices of the Royal Astronomical Society Vol. 488 Journal Issue: 3; ISSN 0035-8711
Publisher:
Royal Astronomical SocietyCopyright Statement
Country of Publication:
United Kingdom
Language:
English
Citation Metrics:
Cited by: 61 works
Citation information provided by
Web of Science

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Cited By (5)

Planck 2015 constraints on spatially-flat dynamical dark energy models journal October 2019
Does spatial flatness forbid the turnaround epoch of collapsing structures? journal December 2019
Quasar X-ray and UV flux, baryon acoustic oscillation, and Hubble parameter measurement constraints on cosmological model parameters journal January 2020
General cosmography model with spatial curvature journal December 2019
Using the Tilted flat-ΛCDM and the Untilted Non-flat ΛCDM Inflation Models to Measure Cosmological Parameters from a Compilation of Observational Data journal September 2019

Figures / Tables (10)

Table 1(p. 4)table Table 1
Table 2(p. 4)table Table 2
Figure 1(p. 6)figure Figure 1
Table 3(p. 6)table Table 3
Table 4(p. 7)table Table 4
Figure 2(p. 8)figure Figure 2
Figure 3(p. 9)figure Figure 3
Figure 4(p. 10)figure Figure 4
Figure 5(p. 11)figure Figure 5
Figure 6(p. 12)figure Figure 6

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Related Subjects

79 ASTRONOMY AND ASTROPHYSICS
Cosmological parameters
dark energy
cosmology: observations