When does the inflaton decay?

DOI10.1088/1475-7516/2018/05/018OpenAlexW2750861387WikidataQ129872598 ScholiaQ129872598MaRDI QIDQ5023747

Cristian Armendariz-Picon

Publication date: 24 January 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1708.09755

zbMATH Keywords

inflationphysics of the early universe

Mathematics Subject Classification ID

Relativity and gravitational theory (83-XX)

Related Items (2)

On the expected backreaction during preheating ⋮ Scalar two-point functions at the late-time boundary of de Sitter

Cites Work

• Unnamed Item
• Unnamed Item
• Proof of the Bogoliubov-Parasiuk theorem on renormalization
• Über die Multiplikation der Kausalfunktionen in der Quantentheorie der Felder
• A new type of isotropic cosmological models without singularity
• Convergence of Bogoliubov's method of renormalization in momentum space
• Bessel Functions of Purely Imaginary Order, with an Application to Second-Order Linear Differential Equations Having a Large Parameter
• Nonperturbative dynamics of reheating after inflation: A review
• Bound States in Quantum Field Theory
• Quantum Fields in Curved Space

This page was built for publication: When does the inflaton decay?