2020/02/17 by George Efstathiou, Steven Gratton · 1 citation
Physics and Astronomy · #astro-ph.CO #hep-th
paper · pdf · doi:10.1093/mnrasl/slaa093
submitted to MNRAS
arxiv created 2020/02/17 · arxiv updated 2020/06/03
We revisit the observational constraints on spatial curvature following recent claims that the Planck data favour a closed Universe. We use a new and statistically powerful Planck likelihood to show that the Planck temperature and polarization spectra are consistent with a spatially flat Universe, though because of a geometrical degeneracy cosmic microwave background spectra on their own do not lead to tight constraints on the curvature density parameter OmegaK. When combined with other astrophysical data, particularly geometrical measurements of baryon acoustic oscillations, the Universe is constrained to be spatially flat to extremely high precision, with Omega_ K = 0.0004 +/-0.0018 in agreement with the 2018 results of the Planck team. In the context of inflationary cosmology, the observations offer strong support for models of inflation with a large number of e-foldings and disfavour models of incomplete inflation.