Random Potentials and Cosmological Attractors
classification
✦ hep-th
astro-ph.COgr-qchep-ph
keywords
attractorscosmologicalfieldspotentialsrandomachievedagreementalpha
read the original 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 $\alpha$-attractors.
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