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Open AccessFeature PaperArticle

Reheating via Gravitational Particle Production in Simple Models of Quintessence or ΛCDM Inflation

by 1,*,† and 2,3,†
1
Departament de Matemàtiques, Universitat Politècnica de Catalunya, Colom 11, 08222 Terrassa, Spain
2
Departament de Matemàtiques, Universitat Politècnica de Catalunya, Diagonal 647, 08028 Barcelona, Spain
3
Fakultät für Physik, Ludwig-Maximilians-Universität, Theresienstr. 37, 80333 München, Germany
*
Author to whom correspondence should be addressed.
These authors contributed equally to this work.
Galaxies 2017, 5(4), 78; https://doi.org/10.3390/galaxies5040078
Received: 11 October 2017 / Revised: 9 November 2017 / Accepted: 10 November 2017 / Published: 14 November 2017
(This article belongs to the Special Issue Cosmology and the Quantum Vacuum)
We have tested some simple Λ 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. View Full-Text
Keywords: gravitational particle production; inflation; kination gravitational particle production; inflation; kination
MDPI and ACS Style

De Haro, J.; Aresté Saló, L. Reheating via Gravitational Particle Production in Simple Models of Quintessence or ΛCDM Inflation. Galaxies 2017, 5, 78.

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