Gravitational waves from p-form inflation

被引:22
作者
Kobayashi, Tsutomu [1 ]
Yokoyama, Shuichiro [2 ]
机构
[1] Waseda Univ, Dept Phys, Shinjuku Ku, Tokyo 1698555, Japan
[2] Nagoya Univ, Dept Phys & Astrophys, Chikusa Ku, Nagoya, Aichi 4648602, Japan
来源
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2009年 / 05期
关键词
cosmological perturbation theory; inflation; PERTURBATIONS; SPECTRUM;
D O I
10.1088/1475-7516/2009/05/004
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Recently it was shown that an inflationary background can be realized by any p-form field non-minimally coupled to gravity. In this paper,we study gravitational waves generated during p-form inflation. Even though the background evolution is identical to that in conventional scalar field inflation, the behavior of gravitational waves is different in p-form inflation. In particular, we find that the propagation speed of gravitational waves differs from unity in 2- and 3-form inflationary models. We point out that the squared speed becomes negative in the large field models. The small field models are free from pathologies and the correction to the spectrum of gravitational waves turns out to be very small.
引用
收藏
页数:13
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