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With the help of an applied software package written by the authors, we haveaveraged the effective total barotropic coefficient $\kappa=(-\lambda +p)/(\lambda+\epsilon$) of the classical scalar field and the cosmological termand have shown that during cosmological evolution for sufficiently large valuesof the cosmological constant the Universe transitions from the inflationarystage to a nonrelativistic stage, and then, after a plateau, it transitions toa later inflationary stage.

russian physics journal

Averaging of the Equations of the Standard Cosmological Model over Rapid  Oscillations: Influence of the cosmological term on the mean value of the  effective barotropic coefficient