English

The Curvature Perturbation in the Axion-type Curvaton Model

Cosmology and Nongalactic Astrophysics 2014-11-18 v3 General Relativity and Quantum Cosmology High Energy Physics - Phenomenology High Energy Physics - Theory

Abstract

We study the axion-type curvaton model, with emphasis on the large field regime where analytic results are very difficult to obtain. We evaluate the tensor-scalar ratio rr using WMAP normalization and the non-linearity parameters fNLf_{NL} and gNLg_{NL} by solving the equations numerically using the δN\delta N formalism. We compare them with results for the curvaton with quadratic potential. We find that rr is much smaller for the axion-type case compared to the result from the quadratic potential, with the difference increasingly more pronounced at larger field values. gNLg_{NL} is found to be positive, unlike the quadratic case where it is negative, and the amplitude of gNLg_{NL} is much larger. Moreover, there is a nearly linear scaling between gNLg_{NL} and fNLf_{NL}, with small deviation from linearity at large field values. The slope between gNLg_{NL} and fNLf_{NL} depends on the parameters characterizing the axion-type curvaton model. We further consider a mixed scenario where both the inflaton and the curvaton contribute to the primordial power spectrum and the non-Gaussianity parameters are found to be much larger than those in the case with quadratic potential.

Keywords

Cite

@article{arxiv.0902.2619,
  title  = {The Curvature Perturbation in the Axion-type Curvaton Model},
  author = {Pravabati Chingangbam and Qing-Guo Huang},
  journal= {arXiv preprint arXiv:0902.2619},
  year   = {2014}
}

Comments

22 pages, 9 figures; one figure on \tau_{NL} and refs added; refs added, minor revision for publication in JCAP