English

Multi-Natural Inflation

High Energy Physics - Phenomenology 2014-05-30 v3 Cosmology and Nongalactic Astrophysics High Energy Physics - Theory

Abstract

We propose a multi-natural inflation model in which the single-field inflaton potential consists of two or more sinusoidal potentials that are comparable in size, but have different periodicity with a possible non-zero relative phase. The model is versatile enough to realize both large-field and small-field inflation. We show that, in a model with two sinusoidal potentials, the predicted values of the spectral index and tensor-to-scalar ratio lie within the 1σ1\sigma region of the Planck data. In particular, there is no lower bound on the decay constants in contrast to the original natural inflation. We also show that, in a certain limit, multi-natural inflation can be approximated by a hilltop quartic inflation model.

Keywords

Cite

@article{arxiv.1401.5212,
  title  = {Multi-Natural Inflation},
  author = {Michael Czerny and Fuminobu Takahashi},
  journal= {arXiv preprint arXiv:1401.5212},
  year   = {2014}
}

Comments

11 pages, 4 figures; updated version: comment on BICEP2 added, matches with published version

R2 v1 2026-06-22T02:50:49.653Z