Studies in Small Field Inflation
arXiv:1109.2079 · doi:10.1088/1475-7516/2012/06/033
Abstract
We explore some issues in slow roll inflation in situations where field excursions are small compared to . We argue that for small field inflation, minimizing fine tuning requires low energy supersymmetry and a tightly constrained structure. Hybrid inflation is {\it 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.
16 pages. issues with single field inflation identified and clarified; role of discrete R symmetries clarified; error in discussion of a non-hybrid model corrected
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- Consistent cosmology with Higgs thermal inflation in a minimal extension of the MSSM
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