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It is shown that cosmological equations for homogeneous isotropic modelsdeduced in the framework of the Poincar\'e gauge theory of gravity by certainrestrictions on indefinite parameters of gravitational Lagrangian take atasymptotics the same form as cosmological equations of general relativitytheory for $\Lambda CDM$-model. Terms related to dark matter and dark energy incosmological equations of standard theory for $\Lambda CDM$-model are connectedin considered theory with the change of gravitational interaction provoked byspacetime torsion.

Accelerating Universe with spacetime torsion but without dark matter and dark energy