English

Constraints on the generalized natural inflation after Planck 2018

Cosmology and Nongalactic Astrophysics 2020-07-02 v4 General Relativity and Quantum Cosmology

Abstract

Based on the dynamics of single scalar field slow-roll inflation and the theory of reheating, we investigate the generalized natural inflationary (GNI) model. Concretely, we give constraints on the scalar spectral index nsn_{s} and tensor-to scalar ratio rr for Λ\LambdaCDM +r+r model according to the latest data from Plack 2018 TT,TE,EE+lowE+lensing (P18) and BICEP2/Keck 2015 season (BK15), i.e., ns=0.9659±0.0044n_{s}=0.9659\pm0.0044 at 68%68\% confidence level (CL) and r<0.0623r<0.0623 at 95%95\%CL. We find that the GNI model is favored by P18 plus BK15 in the ranges of log10(f/Mp)=0.620.18+0.17\log_{10}(f/M_{p})=0.62^{+0.17}_{-0.18} and m=0.350.23+0.13m=0.35^{+0.13}_{-0.23} at 68%68\%CL. In addition, the corresponding predictions of the general and two-phase reheating are respectively discussed. It follows that the parameter mm has the significant effect on the model behaviors.

Keywords

Cite

@article{arxiv.1807.03596,
  title  = {Constraints on the generalized natural inflation after Planck 2018},
  author = {Nan Zhang and Ya-Bo Wu and Jun-Wang Lu and Chu-Wen Sun and Li-Jie Shou and Hai-Zhou Xu},
  journal= {arXiv preprint arXiv:1807.03596},
  year   = {2020}
}

Comments

15 pages, 15 figures, accepted for publication in CPC