arXiv · astro-ph/0606392
Extended Curvaton reheating in inflationary models
Abstract
The curvaton reheating in a non-oscillatory inflationary universe model is studied in a Jordan-Brans-Dicke theory. For different scenarios, the temperature of reheating is computed. The result tells us that the reheating temperature becomes practically independent of the Jordan-Brans-Dicke parameter $w$. This reheating temperature results to be quite different when compared with that obtained from Einstein`s theory of gravity.
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Cuauhtemoc Campuzano, Sergio del Campo, Ramon Herrera. 2006-06-15. Extended Curvaton reheating in inflationary models. https://doi.org/10.1088/1475-7516%2F2006%2F06%2F017
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