Spectral Index in Curvaton Scenario
Abstract
A red tilted primordial power spectrum is preferred by WMAP five-year data and a large positive local-type non-Gaussianity fNL might be observed as well. In this short note we find that a red tilted and large non-Gaussian primordial power spectrum cannot be naturally obtained in curvaton model, because fNL is related to the initial condition of inflation.
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