Completing natural inflation

被引:471
作者
Kim, JE [1 ]
Nilles, HP
Peloso, M
机构
[1] Seoul Natl Univ, Sch Phys, Seoul 151747, South Korea
[2] Univ Bonn, Inst Phys, D-53115 Bonn, Germany
[3] Univ Minnesota, Sch Phys & Astron, Minneapolis, MN 55455 USA
来源
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2005年 / 01期
关键词
inflation; axions;
D O I
10.1088/1475-7516/2005/01/005
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
If the inflaton is a pseudo-scalar axion, the axion shift symmetry can protect the flatness of its potential from too large radiative corrections. This possibility, known as natural inflation, requires an axion scale which is greater than the (reduced) Planck scale. It is unclear whether such a high value is compatible with an effective field theoretical description, and whether the global axionic symmetry survives quantum gravity effects. We propose a mechanism which provides an effective large axion scale, although the original one is sub-Planckian. The mechanism is based on the presence of two axions, with a potential provided by two anomalous gauge groups. The effective large axion scale is due to an almost exact symmetry between the couplings of the axions to the anomalous groups. We also comment on a possible implementation in heterotic string theory.
引用
收藏
页码:61 / 70
页数:10
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