On the possibility of large axion decay constants

被引:290
作者
Banks, T [1 ]
Dine, M [1 ]
Fox, PJ [1 ]
Gorbatov, E [1 ]
机构
[1] Univ Calif Santa Cruz, Santa Cruz Inst Particle Phys, Santa Cruz, CA 95064 USA
来源
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2003年 / 06期
关键词
axions; inflation; string theory and cosmology;
D O I
10.1088/1475-7516/2003/06/001
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The decay constant of the QCD axion is required by observation to be small compared with the Planck scale. In theories of 'natural inflation' and certain proposed anthropic solutions of the cosmological constant problem it would be interesting to obtain a large decay constant for axion-like fields from microscopic physics. String theory is the only context in which one can sensibly address this question. Here we survey a number of periodic fields in string theory in a variety of string vacua. In some examples, the decay constant can be parametrically larger than the Planck scale but the effective action then contains appreciable harmonics of order f(A)/M-p. As a result, these fields are no better inflaton candidates than Planck scale axions.
引用
收藏
页码:1 / 14
页数:14
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