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Oscillons from Pure Natural Inflation

2017/11/28 by Jeong-Pyong Hong, Masahiro Kawasaki, Masahito Yamazaki · 1 voice
Physics and Astronomy · #astro-ph.CO #hep-ph #hep-th

paper · pdf · doi:10.1103/physrevd.98.043531

published as Phys. Rev. D 98, 043531 (2018) · 7 pages, 4 figures

arxiv published 2017/11/28 · arxiv created 2018/09/12 · arxiv updated 2018/09/14

Abstract

We examine the oscillon formation in a recently proposed inflation model of the pure natural inflation, where the inflaton is an axion that couples to a strongly-coupled pure Yang-Mills theory. The plateau of the inflaton potential, which is favored by recent observations, drives the fragmentation of the inflaton and can produce spatially localized oscillons. We find that the oscillons are formed for F<~ O(0.1) MPl, with F the effective decay constant of the model. We also comment on observational implications of the oscillons.

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