Spin-driven inflation
arXiv:gr-qc/0008015 · doi:10.1016/0375-9601(93)91059-E
Abstract
Following recent studies of Ford, we suggest -- in the framework of general relativity -- an inflationary cosmological model with the self-interacting spinning matter. A generalization of the standard fluid model is discussed and estimates of the physical parameters of the evolution are given.
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