Curvaton scenarios with inflaton decays into curvatons

Abstract

We consider the possible decay of the inflaton into curvaton particles during reheating and analyse its effect on curvaton scenarios. Typical decay curvatons are initially relativistic then become non-relativistic, changing the background history of the Universe. We show that this change to the background is the only way in which observational predictions of the scenario are modified. Moreover, once the required amplitude of perturbations is fixed by observation there are no signatures of such decays in other cosmological observables. The decay curvatons can prevent the Universe from becoming dominated by the curvaton condensate, making it impossible to match observations in parts of parameter space. This constrains the branching ratio of the inflaton to curvaton to be less than of order $0.1$ typically. If the branching ratio is below about $10^{-4}$ it has negligible impact on the model parameter space and can be ignored.

arXiv comment9 pages PDFLatex with 6 incorporated figures. Minor updates to match PRD published version

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Cited by in corpus (5)

• The First Three Seconds: a Review of Possible Expansion Histories of the Early Universe
• Measuring the duration of inflation with the curvaton
• Revised $f_{\mathrm{NL}}$ parameter in Curvaton Scenario
• The running curvaton
• Testing Inflationary Cosmology