Status and future directions for direct cross-section measurements of the 13C (α, n) 16O reaction for astrophysics
L Csedreki, G Gyurky, D Rapagnani… - Journal of Physics G …, 2024 - iopscience.iop.org
Abstract The 13 C (α, n) 16 O reaction is the main neutron source of the s-process taking
place in thermally pulsing AGB stars and it is one of the main candidate sources of neutrons …
place in thermally pulsing AGB stars and it is one of the main candidate sources of neutrons …
[HTML][HTML] The New Deep-Underground Direct Measurement of 22Ne(α, γ)26Mg with EASγ: A Feasibility Study
D Mercogliano, A Best, D Rapagnani - Galaxies, 2024 - mdpi.com
22Ne (α, γ) 26Mg is pivotal in the understanding of several open astrophysical questions, as
the nucleosynthesis beyond Fe through the s-process, but its stellar reaction rate is still …
the nucleosynthesis beyond Fe through the s-process, but its stellar reaction rate is still …