arXiv · 1612.04505
Random Potentials and Cosmological Attractors
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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Andrei Linde. 2017-01-03. Random Potentials and Cosmological Attractors. https://doi.org/10.1088/1475-7516%2F2017%2F02%2F028
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