摘要
In thin paper. we shall apply the Ω-field theory as first proposed by Yu￣[1] to cosmology.Under the assumption that the spacetime geometry of the Universe isdescribed by the Robertson-Walker metric and the matter temsor consists only of theΩ-field,the Universe is found to follow a de Sitter Expansion. The horizon and flatnessproblems may thus be explained in a simple and natural way.
In thin paper. we shall apply the Ω-field theory as first proposed by Yu￣[1] to cosmology.Under the assumption that the spacetime geometry of the Universe isdescribed by the Robertson-Walker metric and the matter temsor consists only of theΩ-field,the Universe is found to follow a de Sitter Expansion. The horizon and flatnessproblems may thus be explained in a simple and natural way.
