Abstract
The gravitational interaction is discussed within the framework of gauge gravitational theoryin the Riemann-Cartan space-time. In the case of spatially homogeneous isotopic gravitatingsystems the gravitational repulsion at extreme conditions near limiting energy density and thetransition from gravitational repulsion to attraction in dependence on energy density isstudied. The conversion to Friedman regime and the transition to gravitational repulsion atvery small energy densities is analyzed.
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