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In this paper we exploit the theory of the dynamical systems to study thedynamics of the standard cosmological model of the universe, which is known asthe $\Lambda$CDM model. We assume that the matter content in our universeconsists of barotropic perfect fluids without mutual interaction. Furthermore,we present the appropriate physical interpretation, as well as new dependenciesbetween the scale expansion factor of the universe and cosmological densityparameters.

Dynamics of the $\Lambda$CDM model of the universe from the aspect of the dynamical systems theory