Random Potentials and Cosmological Attractors
  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 $\alpha$-attractors. 
Andrei Linde
hep-th astro-ph.CO gr-qc hep-ph