 The process of the relaxation of the cosmological model to the "stationary" statistical regime (with t → 0 starting from a given "initial instant") is less interesting, however, than the properties of this regime itself with due account taken for the concrete laws of the variation of the physical characteristics of the model during the successive eras.An idea of the rate at which the stationary distribution sets in is obtained from the following example.Let the initial values "x"(0) be distributed in a narrow interval of width δ"x"(0) about some definite number.