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 Paris 07, CEA, Observ Paris, UMR CNRS 7164, F-75205 Paris 13, FranceUniv Paris 07, CEA, Observ Paris, UMR CNRS 7164, F-75205 Paris 13, France
Deffayet, C.
Deser, S.
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Brandeis Univ, Dept Phys, Waltham, MA 02454 USA
CALTECH, Lauritsen Lab, Pasadena, CA 91125 USAUniv Paris 07, CEA, Observ Paris, UMR CNRS 7164, F-75205 Paris 13, France
Deser, S.
Esposito-Farese, G.
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Univ Paris 06, UMR CNRS 7095, Inst Astrophys Paris, GReCO, F-75014 Paris, FranceUniv Paris 07, CEA, Observ Paris, UMR CNRS 7164, F-75205 Paris 13, France
机构:
Inst Res Fundamental Sci IPM, Sch Phys, POB 193955531, Tehran, Iran
Inst Adv Studies Basic Sci IASBS, Dept Phys, POB 45137, Zanjan, IranInst Res Fundamental Sci IPM, Sch Phys, POB 193955531, Tehran, Iran
Taghiloo, V.
Vahidinia, M. H.
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Inst Res Fundamental Sci IPM, Sch Phys, POB 193955531, Tehran, Iran
Inst Adv Studies Basic Sci IASBS, Dept Phys, POB 45137, Zanjan, IranInst Res Fundamental Sci IPM, Sch Phys, POB 193955531, Tehran, Iran
机构:
Univ Maryland, Dept Phys, East West Space Sci Ctr, College Pk, MD 20742 USAUniv Maryland, Dept Phys, East West Space Sci Ctr, College Pk, MD 20742 USA