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.
|Journal||Physical Review D - Particles, Fields, Gravitation and Cosmology|
|State||Published - 29 Dec 2009|