Smooth reheating and dark matter via non-Abelian gauge theory-Reference-Cited by-同舟云学术

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Smooth reheating and dark matter via non-Abelian gauge theory

Published:2024-10 Issue: Volume:857 Page:138995
ISSN:0370-2693
Container-title:Physics Letters B
language:en
Short-container-title:Physics Letters B

Author:

Biondini S.,Kolešová H.^ORCID,Procacci S.

Funder

University of Bern

Forskningsrådet

Swiss National Science Foundation

Publisher

Elsevier BV

Reference73 articles.

1. MeV scale reheating temperature and thermalization of neutrino background;Kawasaki;Phys. Rev. D,2000

2. What is the lowest possible reheating temperature?;Hannestad;Phys. Rev. D,2004

3. New constraints on the reheating temperature of the universe after WMAP-5;De Bernardis;Astropart. Phys.,2008

4. Planck 2018 results. I. Overview and the cosmological legacy of Planck;Aghanim;Astron. Astrophys.,2020

5. Planck 2018 results. X. Constraints on inflation;Akrami;Astron. Astrophys.,2020

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