Constraining the 22Ne(α,γ)26Mg and 22Ne(α,n)25Mg reaction rates using sub-Coulomb α-transfer reactions
Author:
Funder
National Nuclear Security Administration
U.S. Department of Energy
Publisher
Elsevier BV
Subject
Nuclear and High Energy Physics
Reference36 articles.
1. Thesprocess: Nuclear physics, stellar models, and observations
2. Neutron-Capture Elements in the Early Galaxy
3. The astrophysical implications of low-energy resonances in 22Ne + α
4. N22e(α,n)M25g: The Key Neutron Source in Massive Stars
5. Study of the 22Ne(α, n)25Mg reaction: a possible source of stellar neutronS
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1. The s Process and Beyond;Annual Review of Nuclear and Particle Science;2023-09-25
2. Study of the Mg22 Waiting Point Relevant for X-Ray Burst Nucleosynthesis via the Mg22(α,p)Al25 Reaction;Physical Review Letters;2023-09-15
3. Progress in Nuclear Astrophysics: a multi-disciplinary field with still many open questions;Journal of Physics: Conference Series;2023-09-01
4. The resonances in the $$^{22}$$Ne+$$\alpha $$ fusion reactions;The European Physical Journal A;2023-01-30
5. Horizons: nuclear astrophysics in the 2020s and beyond;Journal of Physics G: Nuclear and Particle Physics;2022-11-01
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