Subleading effects and the field range in axion inflation

被引:27
|
作者
Parameswaran, Susha [1 ]
Tasinato, Gianmassimo [2 ]
Zavala, Ivonne [2 ]
机构
[1] Univ Liverpool, Dept Math Sci, Liverpool L69 7ZL, Merseyside, England
[2] Swansea Univ, Dept Phys, Swansea SA2 8PP, W Glam, Wales
关键词
inflation; axions; string theory and cosmology; NATURAL INFLATION; ANISOTROPY;
D O I
10.1088/1475-7516/2016/04/008
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
An attractive candidate for the inflaton is an axion slowly rolling down a flat potential protected by a perturbative shift symmetry. Realisations of this idea within large field, natural and monomial inflation have been disfavoured by observations and are difficult to embed in string theory. We show that subleading, but significant non-perturbative corrections can superimpose sharp cliffs and gentle plateaus into the potential, whose overall effect is to enhance the number of e-folds of inflation. Sufficient e-folds are therefore achieved for smaller field ranges compared to the potential without such corrections. Thus, both single-field natural and monomial inflation in UV complete theories like string theory, can be restored into the favour of current observations, with distinctive signatures. Tensor modes result un-observably small, but there is a large negative running of the spectral index. Remarkably, natural inflation can be achieved with a single field whose axion decay constant is sub-Planckian.
引用
收藏
页数:19
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