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Over the last few years, low- and high-redshift observations set off a tension in the measurement of the present-day expansion rate, $H_0$.
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W. Handley, C urvature tension: evidence for a closed universe, Phys. Rev. D 103
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A. Lewis, A. Challinor and A. Lasenby, E fficient computation of CMB anisotropies in closed FRW models, Astrophys. J. 538
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G. Mangano, G. Miele, S. Pastor, T. Pinto, O. Pisanti and P. D. Serpico, R elic neutrino decoupling including flavor oscillations, Nucl. Phys. B 729
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2011
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2012
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A. Lewis, E fficient sampling of fast and slow cosmological parameters, Phys. Rev. D 87
2013
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