Reheating via gravitational particle production in simple models of quintessence or CDM inflation
arXiv:1711.03788 · doi:10.3390/galaxies5040078
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.
Proceedings of the workshop "Cosmology and the Quantum Vacuum IV" Segovia, Spain. Accepted for publication in the special Issue "Cosmology and the Quantum Vacuum" of Galaxies
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