English

Multi-chaotic inflation with and without spectator field

Cosmology and Nongalactic Astrophysics 2022-08-03 v2 General Relativity and Quantum Cosmology High Energy Physics - Phenomenology

Abstract

Motivated by the result of Planck+BICEP/Keck recently released, we investigate the consistency of the multi-field inflation models in terms of the spectral index nsn_s and the tensor-to-scalar ratio rr. In this study, we focus on double-inflaton models with and without a spectator field. We find that inflaton with a quadratic potential can become viable when three fields with a specific hierarchical mass spectrum are realized such that two fields act as inflatons and the other one is the spectator. We also discuss the conditions to avoid the fine-tuning, by careful study of how the prediction depends on the background trajectory in the inflaton-field space.

Keywords

Cite

@article{arxiv.2203.09698,
  title  = {Multi-chaotic inflation with and without spectator field},
  author = {Yukiyoshi Morishita and Tomo Takahashi and Shuichiro Yokoyama},
  journal= {arXiv preprint arXiv:2203.09698},
  year   = {2022}
}

Comments

22 pages, 7 figures, accepted for publication in JCAP

R2 v1 2026-06-24T10:17:52.196Z