English

Curvaton in large field inflation

Cosmology and Nongalactic Astrophysics 2015-06-19 v2 General Relativity and Quantum Cosmology High Energy Physics - Phenomenology

Abstract

We comprehensively explore the quadratic curvaton models in the chaotic inflation. In the light of the BICEP2 result r0.2r \approx 0.2, all model parameters and relevant observables are computed. It is found the curvaton field value is constrained into a narrow range, σ=O(102\sigma_* = \mathcal{O}(10^{-2}-101)10^{-1}) and the running of the spectral index is ns103n_s' \gtrsim -10^{-3}. We show that if the curvaton is added, the models are heavily degenerated on the nsn_s - rr plane. However, introducing a new plane, the degeneracy can be resolved. To distinguish the curvaton models, precise measurements of not only rr but also nsn_s' and the tensor tilt nTn_T are required.

Keywords

Cite

@article{arxiv.1404.0951,
  title  = {Curvaton in large field inflation},
  author = {Tomohiro Fujita and Masahiro Kawasaki and Shuichiro Yokoyama},
  journal= {arXiv preprint arXiv:1404.0951},
  year   = {2015}
}

Comments

16pages, 12figures, ver2: typo corrected, figs. 5-9 and 11 are revised

R2 v1 2026-06-22T03:42:21.608Z