Reheating via gravitational particle production in simple models of quintessence or $\Lambda$CDM inflation
Jaume Haro, Llibert Arest\'e Sal\'o

TL;DR
This paper tests simple $ ext{Lambda}$CDM and quintessence inflation models against recent BICEP and Planck data, focusing on gravitational particle production during reheating to ensure compatibility with nucleosynthesis.
Contribution
It evaluates the viability of simple inflation models by matching observational data and analyzing reheating temperatures from gravitational particle production.
Findings
Models consistent with BICEP and Planck data
Reheating temperatures support nucleosynthesis
Gravitational particle production effectively reheats the universe
Abstract
We have tested some simple CDM (the same test is also valid for quintessence) inflation models, imposing that they match with the recent observational data provided by the BICEP and Planck's team and leading to a reheating temperature, which is obtained via gravitational particle production after inflation, supporting the nucleosynthesis success.
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