Can we bypass no-go theorem for Ricci-inverse gravity?

Recently, Amendola et al. proposed a geometrical theory of gravity containing higher-order derivative terms. The authors introduced anticurvature scalar $(A)$, which is the trace inverse Ricci tensor ($A^{\mu\nu} = R_{\mu\nu}^{-1}$). In this work, we consider two classes Ricci-inverse -- Class I and II models. models are form $f(R, A)$ where $f$ function scalars. ${\cal F}(R, A^{\mu\nu}A_{\mu\nu})$ F}$ square tensor. For both these models, numerically solve modified Friedmann equations in redshift range $1500 < z 0$. We show that late-time evolution Universe, i.e., from matter-dominated epoch to accelerated expansion epoch, \emph{can not} be explained by Using reduced action approach, not bypass} no-go theorem for Finally, discuss implications our analysis early-Universe cosmology.