Phenomenological model for the early universe
作者： N. C. Tsamis , R. P. Woodard
DOI: 10.1103/PHYSREVD.80.083512
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摘要: We consider the description of cosmological dynamics from onset inflation by a perfect fluid whose parameters must be consistent with strength enhanced quantum loop effects that can arise during inflation. The source these nonlocal and simple incarnation it is studied both analytically numerically. resulting evolution stops in calculable amount time leads to an oscillatory universe vanishing mean value for curvature scalar oscillation frequency which we compute.
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