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• W2171808580 abstract "We explore some issues in slow roll inflation in situations where field excursions are small compared to Mp. We argue that for small field inflation, minimizing fine tuning requires low energy supersymmetry and a tightly constrained structure. Hybrid inflation is almost an inevitable outcome. The resulting theory can be described in terms of a supersymmetric low energy effective action and inflation completely characterized in terms of a small number of parameters. Demanding slow roll inflation significantly constrains these parameters. In this context, the generic level of fine tuning can be described as a function of the number of light fields, there is an upper bound on the scale of inflation, and an (almost) universal prediction for the spectral index. Models of this type need not suffer from a cosmological moduli problem." @default.
• W2171808580 created "2016-06-24" @default.
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• W2171808580 date "2012-06-21" @default.
• W2171808580 modified "2023-10-17" @default.
• W2171808580 title "Studies in small field inflation" @default.
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• W2171808580 doi "https://doi.org/10.1088/1475-7516/2012/06/033" @default.
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