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We describe a way to construct supergravity models with an arbitrary inflaton potential V ({\phi}) and show that all other scalar fields in this class of models can be stabilized at the inflationary trajectory by a proper choice of the K\"ahler potential.
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R. Kallosh and A. Linde, “New models of chaotic inflation in supergravity,” JCAP 1011
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V. Demozzi, A. Linde and V. Mukhanov, in preparation
Cited in the paper.
Cited in the paper.
2010
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2010
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H. M. Lee, “Chaotic inflation in Jordan frame supergravity,” JCAP 1008
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