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 , all model parameters and relevant observables are computed. It is found the curvaton field value is constrained into a narrow range, - and the running of the spectral index is . We show that if the curvaton is added, the models are heavily degenerated on the - plane. However, introducing a new plane, the degeneracy can be resolved. To distinguish the curvaton models, precise measurements of not only but also and the tensor tilt are required.
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