Reheating constraints on modified single-field natural inflation models

In this paper, we discuss three modified single-field natural inflation models in detail, including Special generalized natural inflation model (SNI), extended natural inflation model (ENI) and natural inflation inspired model (NII). We derive the analytical expression of the tensor-to-scalar ratio...

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Bibliographic Details
Main Authors: Cheng, W. (Author), Pan, Y. (Author), Yu, Q. (Author), Zhou, H. (Author), Zhou, R. (Author)
Format: Article
Language:English
Published: Springer Science and Business Media Deutschland GmbH 2022
Online Access:View Fulltext in Publisher
LEADER 01905nam a2200181Ia 4500
001 10.1140-epjc-s10052-022-10559-8
008 220718s2022 CNT 000 0 und d
020 |a 14346044 (ISSN) 
245 1 0 |a Reheating constraints on modified single-field natural inflation models 
260 0 |b Springer Science and Business Media Deutschland GmbH  |c 2022 
856 |z View Fulltext in Publisher  |u https://doi.org/10.1140/epjc/s10052-022-10559-8 
520 3 |a In this paper, we discuss three modified single-field natural inflation models in detail, including Special generalized natural inflation model (SNI), extended natural inflation model (ENI) and natural inflation inspired model (NII). We derive the analytical expression of the tensor-to-scalar ratio r and the spectral index ns for those models. Then the reheating temperature Tre and reheating duration Nre are analytically derived. Moreover, considering the CMB constraints, the feasible space of the SNI model in (ns, r) plane is almost covered by that of the NII, which means the NII is more general than the SNI. In addition, there is no overlapping space between the ENI and the other two models in (ns, r) plane, which indicates that the ENI and the other two models exclude each other, and more accurate experiments can verify them. Furthermore, the reheating brings tighter constraints to the inflation models, but they still work for a different reheating universe. Considering the constraints of ns, r, Nk and choosing Tre near the electroweak energy scale, one can find that the decay constants of the three models have no overlapping area and the effective equations of state ωre should be within 14≲ωre≲45 for the three models. © 2022, The Author(s). 
700 1 |a Cheng, W.  |e author 
700 1 |a Pan, Y.  |e author 
700 1 |a Yu, Q.  |e author 
700 1 |a Zhou, H.  |e author 
700 1 |a Zhou, R.  |e author 
773 |t European Physical Journal C