The growth of matter perturbations in the f(T) gravity
Abstract
In this paper, we study the growth index of matter density perturbations for the power law model in f(T) gravity. Using the parametrization γ(z)=γ0+γ1 z 1+z for the growth index, which approximates the real evolution of γ(z) very well, and the observational data of the growth factor, we find that, at 1σ confidence level, the power law model in f(T) gravity is consistent with the observations, since the obtained theoretical values of γ0 and γ1 are in the allowed region.
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