Article

Random potentials and cosmological attractors

Andrei LindeDepartment of Physics and SITP, Stanford University, Stanford, California 94305 U.S.A

2017en

ABI

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.

Identifiers

DOI: 10.1088/1475-7516/2017/02/028

Citations and references

Cited by 30 references

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