Abstract
AbstractThe 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 $$10^9$$
10
9
GeV the corresponding values of the spectral index enter perfectly in its $$2\sigma $$
2
σ
C.L., which shows the viability of this kind of models.
Funder
Ministerio de Economía, Industria y Competitividad, Gobierno de España
Departament d’Innovació, Universitats i Empresa, Generalitat de Catalunya
Publisher
Springer Science and Business Media LLC
Subject
Physics and Astronomy (miscellaneous)
Cited by
2 articles.
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