Abstract
Abstract
The gravitational interaction is discussed within the framework of gauge gravitational theory
in the Riemann-Cartan space-time. In the case of spatially homogeneous isotopic gravitating
systems the gravitational repulsion at extreme conditions near limiting energy density and the
transition from gravitational repulsion to attraction in dependence on energy density is
studied. The conversion to Friedman regime and the transition to gravitational repulsion at
very small energy densities is analyzed.
Subject
Astronomy and Astrophysics