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Three Form Inflation

Astrophysics 2007-05-23 v1 High Energy Physics - Theory

Abstract

It is noted that inflation driven by a three form with arbitrary self coupling satisfies a consistency relation nS1=2nTn_S-1=2n_T, between spectral indices of scalar and tensor cosmological perturbations. The standard consistency relation for the ratio of the amplitudes of perturbations is only valid for quadratic self coupling of the three form.

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Cite

@article{arxiv.astro-ph/0401520,
  title  = {Three Form Inflation},
  author = {Andrei Gruzinov},
  journal= {arXiv preprint arXiv:astro-ph/0401520},
  year   = {2007}
}

Comments

4 pages