  Homogeneous isotropic models with two torsion functions built in the
framework of the Poincare gauge theory of gravity based on general expression
of gravitational Lagrangian by certain restrictions on indefinite parameters
are analyzed numerically. Special points of cosmological solutions at
asymptotics and conditions of their stability in dependence of indefinite
parameters are found. Procedure of numerical integration of the system of
gravitational equations at asymptotics is considered. Numerical solution for
accelerating Universe without dark energy and dark matter is obtained. It is
shown that by certain restrictions on indefinite parameters obtained
cosmological solutions are in agreement with SNe Ia observational data and Big
Bang Nucleosynthesis predictions. Statefinder diagnostics is discussed in order
to compare considered cosmological model with other models.
