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.
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Univ Tokyo, Inst Cosm Ray Res, Kashiwa, Chiba 2778582, Japan
Univ Tokyo, Todai Inst Adv Study, Kavli Inst Phys & Math Universe WPI, Kashiwa, Chiba 2778582, JapanUniv Tokyo, Inst Cosm Ray Res, Kashiwa, Chiba 2778582, Japan
Kawasaki, Masahiro
Saikawa, Ken'ichi
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Tokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528511, JapanUniv Tokyo, Inst Cosm Ray Res, Kashiwa, Chiba 2778582, Japan
Saikawa, Ken'ichi
Takeda, Naoyuki
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Univ Tokyo, Inst Cosm Ray Res, Kashiwa, Chiba 2778582, JapanUniv Tokyo, Inst Cosm Ray Res, Kashiwa, Chiba 2778582, Japan