Curvaton reheating in logamediate inflationary model
arXiv:0912.4721 · doi:10.1103/PhysRevD.80.123531
Abstract
In a logamediate inflationary universe model we introduce the curvaton field in order to bring this inflationary model to an end. In this approach we determine the reheating temperature. We also outline some interesting constraints on the parameters that describe our models. Thus, we give the parameter space in this scenario.
Accepted by PRD
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- The curvaton scenario in Brane cosmology: model parameters and their constraints
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