Random potentials and cosmological attractors
2017; Institute of Physics; Volume: 2017; Issue: 02 Linguagem: Inglês
10.1088/1475-7516/2017/02/028
ISSN1475-7516
Autores Tópico(s)Galaxies: Formation, Evolution, Phenomena
ResumoI 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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