quantum corrections and the inflationary observables
arXiv:1404.7349 · doi:10.1088/1475-7516/2014/09/005
Abstract
We study a model of inflation with terms quadratic and logarithmic in the Ricci scalar, where the gravitational action is . These terms are expected to arise from one loop corrections involving matter fields in curved space-time. The spectral index and the tensor to scalar ratio yield and . i.e. is an order of magnitude bigger or smaller than the original Starobinsky model which predicted . Further enhancement of gives a scale invariant or higher. Other inflationary observables are . Despite the enhancement in , if the recent BICEP2 measurement stands, this model is disfavoured.
arXiv commentLaTeX, 9+1 pages, 5 figures
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