The 22 Ne( α,n) 25 Mg reaction - state of the art, astrophysics, and perspectives
(2025)
Journal Article
Best, A., Adsley, P., Amberger, R., Battino, U., Chillery, T., La Cognata, M., deBoer, R. J., Mercogliano, D., Ota, S., Rapagnani, D., Sidhu, R. S., Spartà, R., Tumino, A., & Wiescher, M. (2025). The 22 Ne( α,n) 25 Mg reaction - state of the art, astrophysics, and perspectives. European Physical Journal A: Hadrons and Nuclei, 61(5), Article 99. https://doi.org/10.1140/epja/s10050-025-01572-y
One of the most important stellar neutron sources is the 22Ne(α, n)25Mg reaction, which gets activated both during the helium intershell burning in asymptotic giant branch stars and in core helium and shell carbon burning in massive stars. The 22Ne(α... Read More about The 22 Ne( α,n) 25 Mg reaction - state of the art, astrophysics, and perspectives.