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Paper   IPM / Astronomy / 12603
School of Astronomy
  Title:   Curvaton and the inhomogeneous end of inflation
1.  Hooshyar Assadullahi
2.  Hassan Firouzjahi
3.  Mohammad Hossein Namjoo
4.  David Wands
  Status:   Published
  Journal: JCAP
  Year:  2012
  Pages:   024
  Supported by:  IPM
We study the curvature perturbations and non-Gaussianities generated from the combined effects of inhomogeneous end of inflation and curvaton mechanism. This double role is played by an isocurvature field which is massless during inflation but acquire a mass instantaneously at the end of inflation via the waterfall phase transition. We calculate the resulting primordial non-Gaussianity characterized by the non-linearity parameter, fNL, recovering the usual end-of-inflation result when the field decays promptly and the usual curvaton result if the field decays sufficiently late.

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