arXiv · 1412.7111
Does the first chaotic inflation model in supergravity provide the best fit to the Planck data?
Abstract
I describe the first model of chaotic inflation in supergravity, which was proposed by Goncharov and the present author in 1983. The inflaton potential of this model has a plateau-type behavior $V_{0} (1- {8\over 3}\, e^{-\sqrt 6 |ϕ|})$ at large values of the inflaton field. This model predicts $n_{s} = 1-{2\over N} \approx 0.967$ and $r = {4\over 3 N^{2}} \approx 4 \times 10^{-4}$, in good agreement with the Planck data. I propose a slight generalization of this model, which allows to describe not only inflation but also dark energy and supersymmetry breaking.
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Andrei Linde. 2015-01-17. Does the first chaotic inflation model in supergravity provide the best fit to the Planck data?. https://doi.org/10.1088/1475-7516%2F2015%2F02%2F030
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