Note on the reheating temperature in Starobinsky-type potentials
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The relation between the reheating temperature, the number of e-folds and the spectral index is shown for the Starobinsky model and some of its descendants through a very detailed calculation of these three quantities. The conclusion is that for viable temperatures between 1 MeV and 109 GeV the corresponding values of the spectral index enter perfectly in its 2s C.L., which shows the viability of this kind of models
CitationHaro, J.; Aresté, L. Note on the reheating temperature in Starobinsky-type potentials. "General Relativity and Gravitation", Desembre 2020, vol. 52, núm. 12, p. 116-1-116-13.