Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 488, Issue 3, Pages 3844-3856Publisher
OXFORD UNIV PRESS
DOI: 10.1093/mnras/stz1966
Keywords
cosmological parameters; dark energy; cosmology: observations
Categories
Funding
- National Science Foundation [CNS-1006860, EPS-1006860, EPS-0919443]
- Department of Energy [DE-SC0019038]
- National Natural Science Foundation of China [11703034, 11773032, 11573031]
- National Astronomical Observatories of China Nebula Talents Program
- U.S. Department of Energy (DOE) [DE-SC0019038] Funding Source: U.S. Department of Energy (DOE)
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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 1.7 sigma) and dark energy dynamics (up to a little over 2 sigma) over a cosmological constant Lambda. The data also favour, at 1,8 sigma to 3,4 sigma, depending on the model and data combination, a lower Hubble constant than what is measured from the local expansion rate.
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