Sweeping Horndeski canvas: new growth-rate parameterization for modified-gravity theories

Abstract

Abstract We propose and numerically validate a new fitting formula that is sufficiently accurate to model the growth of structure in Horndeski theories of modified gravity for upcoming Stage IV and V large-scale structure surveys. Based on an analysis of more than 18,000 Horndeski models and adopting the popular parameterization of the growth rate f(z) = Ω M (z) γ , we generalize the constant growth index γ to a two-parameter redshift-dependent quantity,  γ(z), that more accurately fits these models. We demonstrate that the functional form  γ(z) = γ 0 + γ 0 z 2/(1 + z) improves the median χ 2 of the fit to viable Horndeski models by a factor of ∼ 40 relative to that of a constant γ, and is sufficient to obtain unbiased results even for precise measurements expected in Stage IV and V surveys. Finally, we constrain the parameters of the new fitting formula using current cosmological data.