Quantum torsion with non-zero standard deviation: non-perturbative approach for cosmology
arXiv:1210.5878 · doi:10.1016/j.physletb.2013.01.008
Abstract
Cosmology with non-perturbative quantum corrections resulting from torsion is considered. It is shown that the evolution of closed, open and flat Universes is changed because of the presence of a non-zero dispersion of quantum torsion. The evolution of a Universe with quantum torsion and with one type of average curvature can be similar to the evolution of a Universe without quantum torsion and with another type of average curvature. For the description of the non-perturbative quantum torsion, a vector field approximation is applied.
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