Abstract
In this work, we consider four gravity models—the Hu-Sawicki, Starobinsky, Exponential and Tsujikawa models—and use a range of cosmological data, together with Markov Chain Monte Carlo sampling techniques, to constrain the associated model parameters. Our main aim is to compare the results we get when is treated as a free parameter with their counterparts in a spatially flat scenario. The bounds we obtain for in the former case are compatible with a flat geometry. It appears, however, that a higher value of the Hubble constant allows for more curvature. Indeed, upon including in our analysis a Gaussian likelihood constructed from the local measurement of , we find that the results favor an open universe at a little over . This is perhaps not statistically significant, but it underlines the important implications of the Hubble tension for the assumptions commonly made about spatial curvature. We note that the late-time deviation of the Hubble parameter from its equivalent is comparable across all four models, especially in the nonflat case. When , the Hu-Sawicki model admits a smaller mean value for , which increases the said deviation at redshifts higher than unity. We also study the effect of a change in scale by evaluating the growth rate at two different wave numbers . Any changes are, on the whole, negligible, although a smaller does result in a slightly larger average value for the deviation parameter .
4 More- Received 8 June 2021
- Accepted 22 October 2021
DOI:https://doi.org/10.1103/PhysRevD.104.123503
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