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- W2961793911 endingPage "3856" @default.
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- W2961793911 abstract "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." @default.
- W2961793911 created "2019-07-23" @default.
- W2961793911 creator A5034786060 @default.
- W2961793911 creator A5061402622 @default.
- W2961793911 creator A5062376442 @default.
- W2961793911 date "2019-07-17" @default.
- W2961793911 modified "2023-10-17" @default.
- W2961793911 title "Baryon acoustic oscillation, Hubble parameter, and angular size measurement constraints on the Hubble constant, dark energy dynamics, and spatial curvature" @default.
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- W2961793911 doi "https://doi.org/10.1093/mnras/stz1966" @default.
- W2961793911 hasPublicationYear "2019" @default.