Ω－场的暴涨宇宙

Inflation in Ω-Field Cosmology

本文主旨在应用余提出的Ω－场理论￣［１］，去研究宇宙学问题。假设时空遵从罗伯逊－沃尔克（Ｒ－Ｗ）度规的结构，而能量张量动量张量只包含Ω－场的项，我们证明宇宙早期存在一急速暴涨阶段。视界问题和平直性问题从而获得简单而自然的解释。

In this 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 is described by the Robertson-Walker metric and the matter tensor consists only of the Ω-field, the Universe is found to follow a de Sitter expansion.The hor-izon and flatness problems may thus be explained in a simple and natural way.