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Curvature tension: Evidence for a closed universe

Will HandleyAstrophysics Group, Cavendish Laboratory, J. J. Thomson Avenue, Cambridge CB3 0HE, United Kingdom
2021en
ABI

Аннотация

The curvature parameter tension between Planck 2018, cosmic microwave background (CMB) lensing, and baryon acoustic oscillation (BAO) data is measured using the suspiciousness statistic to be $2.5--3\ensuremath{\sigma}$. Conclusions regarding the spatial curvature of the Universe which stem from the combination of these data should therefore be viewed with suspicion. Without CMB lensing or BAO, Planck 2018 has a moderate preference for closed universes, with Bayesian betting odds of over $50\ensuremath{\mathbin:}1$ against a flat universe and over $2000\ensuremath{\mathbin:}1$ against an open universe.

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