Non-Singular Cosmology and Gauge Theories of Gravitation
arXiv:gr-qc/0406030 · doi:10.1142/9789812702296_0003
Abstract
The resolution of the problem of cosmological singularity in the framework of gauge theories of gravitation is discussed. Generalized cosmological Friedmann equations for homogeneous isotropic models filled by interacting scalar fields and usual gravitating matter are deduced. It is shown that generic feature of cosmological models of flat, open and closed type is their regular bouncing character.
LaTeX2e, 16 pages