Random potentials and cosmological attractors

Published 16 February 2017 © 2017 IOP Publishing Ltd and Sissa Medialab srl
, , Citation Andrei Linde JCAP02(2017)028 DOI 10.1088/1475-7516/2017/02/028

1475-7516/2017/02/028

Abstract

I show that the problem of realizing inflation in theories with random potentials of a limited number of fields can be solved, and agreement with the observational data can be naturally achieved if at least one of these fields has a non-minimal kinetic term of the type used in the theory of cosmological α-attractors.

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10.1088/1475-7516/2017/02/028