Note on the reheating temperature in Starobinsky-type potentials

Author:

Haro Jaume,Aresté Saló LlibertORCID

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. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Formation of trapped vacuum bubbles during inflation, and consequences for PBH scenarios;Journal of Cosmology and Astroparticle Physics;2023-10-01

2. Reheating in models with non-minimal coupling in metric and Palatini formalisms;Journal of Cosmology and Astroparticle Physics;2022-02-01

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