Journal
CLASSICAL AND QUANTUM GRAVITY
Volume 24, Issue 23, Pages 5835-5847Publisher
IOP PUBLISHING LTD
DOI: 10.1088/0264-9381/24/23/007
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Homogeneous isotropic cosmological models with two torsion functions filled with scalar fields and usual gravitating matter are built and investigated in the framework of the Poincare gauge theory of gravity. It is shown that by certain restrictions on indefinite parameters of gravitational Lagrangian the cosmological equations at asymptotics contain an effective cosmological constant that can explain observable acceleration of cosmological expansion. The behavior of inflationary cosmological solutions at extremely high energy densities is analyzed and regular bouncing solutions are obtained. The role of the spacetime torsion provoking the acceleration of cosmological expansion is discussed.
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