Inflation in ω-field cosmoloty
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In this paper, we shall apply the ω-field theory as first proposed by Yu13 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 theω-field, the Universe is found to follow a de Sitter Expansion. The horizon and flatness problems may thus be explained in a simple and natural way.
Key wordsω-field inflation Robertson-Walker metric
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