Riemannian Structure imposed on Friedmann and more general spacetimes
In the paper we consider two Finsler-like Riemannian metrics, which can be in a natural way introduced into general relativity. One of those metrics $γ_{ab}$ is degenerate and the second $h_{ab}$ is nondegenerate. We are mainly interested with the metric $h_{ab}$ and comparing the geometric structure determined by this metric $h_{ab}$ with the geometric structure determined by the Lorentzian metric $g_{ab}$ of the underlying spacetime. Full comparison we have given for Friedmann Universis. The preliminary version of the paper was presented by one of us (J.G.) on conference POTOR 6 in Szczecin 2019. We think that the our introduction of the Riemannian metric $h_{ab}$ into spacetime is simpler and more general than to so-called Wick rotation.