Selecting energy-momentum trace dependent gravity theories with LSS

We study scalar cosmological perturbations in $f(R, T)$ modified gravity theories being T the trace of the energy-momentum tensor. We provide detailed equations for the matter energy density contrast. We solve then numerically to promote a comparison with available large scale structure (LSS) formation observational data on f σ₈ and also addressing the S₈ tension. We identify $f(R,T)$ models that lead either to growth enhancement or suppression. Since recent results in the literature indicate a preference for the latter feature, this type of analysis is quite useful to select viable modifications of gravity. We studied class of such $f(R,T)$ models are either ruled out or severely restricted.