2 code implementations • 12 Nov 2020 • Paul Frederik Depta, Marco Hufnagel, Kai Schmidt-Hoberg
The remarkable agreement between observations of the primordial light element abundances and the corresponding theoretical predictions within the standard cosmological history provides a powerful method to constrain physics beyond the standard model of particle physics (BSM).
High Energy Physics - Phenomenology Cosmology and Nongalactic Astrophysics
no code implementations • 19 Feb 2020 • Paul Frederik Depta, Marco Hufnagel, Kai Schmidt-Hoberg
Axion-like particles with masses in the keV-GeV range have a profound impact on the cosmological evolution of our Universe, in particular on the abundance of light elements produced during Big Bang Nucleosynthesis.
High Energy Physics - Phenomenology Cosmology and Nongalactic Astrophysics
