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We propose the introduction of a Heisenberg symmetry of the Kahler potential to solve the problems with chaotic inflation in supergravity, as a viable alternative to the use of shift symmetry.
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For textbook reviews on inflation see: A. R. Liddle and D. H. Lyth, “Cosmological inflation and large-scale structure,” Cambridge, UK: Univ. Pr. (2000) 400 p
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