Weak gravity strongly constrains large-field axion inflation

被引:114
|
作者
Heidenreich, Ben [1 ]
Reece, Matthew [1 ]
Rudelius, Tom [1 ]
机构
[1] Harvard Univ, Dept Phys, Cambridge, MA 02138 USA
来源
基金
美国国家科学基金会;
关键词
Compactification and String Models; Cosmology of Theories beyond the SM; Models of Quantum Gravity; CONJECTURE; LANDSCAPE; ENTROPY;
D O I
10.1007/JHEP12(2015)108
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
Models of large-field inflation based on axion-like fields with shift symmetries can be simple and natural, and make a promising prediction of detectable primordial gravitational waves. The Weak Gravity Conjecture is known to constrain the simplest case in which a single compact axion descends from a gauge field in an extra dimension. We argue that the Weak Gravity Conjecture also constrains a variety of theories of multiple compact axions including N-flation and some alignment models. We show that other alignment models entail surprising consequences for how the mass spectrum of the theory varies across the axion moduli space, and hence can be excluded if further conjectures hold. In every case that we consider, plausible assumptions lead to field ranges that cannot be parametrically larger than M-Pl. Our results are strongly suggestive of a general inconsistency in models of large-field inflation based on compact axions, and possibly of a more general principle forbidding super-Planckian field ranges.
引用
收藏
页码:1 / 41
页数:41
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