arXiv · hep-ph/9405337
Flat Potential for Inflaton with a Discrete $R$-invariance in Supergravity
Abstract
We show that a very flat potential of inflaton required for a sufficient inflation is naturally obtained in $N=1$ supergravity by imposing a discrete $R$-invariance $Z_{n}$. Several cosmological constraints on parameters in the inflaton superpotential are derived. The reheating temperature turns out to be $(1-10^8)$GeV for the cases of $n$=3--10. Baryogenesis in this model is also discussed briefly.
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K. Kumekawa, T. Moroi, T. Yanagida. 1994-05-20. Flat Potential for Inflaton with a Discrete $R$-invariance in Supergravity. https://doi.org/10.1143/ptp%2F92.2.437
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