The6Li(22Ne,26Mg)d α-transfer experiment for the study of low-energy resonances in22Ne(α,γ)26Mg-Reference-Cited by-同舟云学术

The6Li(22Ne,26Mg)d α-transfer experiment for the study of low-energy resonances in22Ne(α,γ)26Mg

Published:2014 Issue: Volume:66 Page:07017
ISSN:2100-014X
Container-title:EPJ Web of Conferences
language:
Short-container-title:EPJ Web of Conferences

Author:

Ota Shuya,Makii Hiroyuki,Ishii Tetsuro,Angell Christopher,Bardayan Daniel W.,Chiba Satoshi,Nishinaka Ichiro,Nishio Katsuhisa,Matos Milan,Mitsuoka Shinichi,Pain Steven

Publisher

EDP Sciences

Link

http://www.epj-conferences.org/10.1051/epjconf/20146607017/pdf

Reference13 articles.

1. The origin of the heavy elements: The s process

2. Radiative C-13 burning in asymptotic giant branch stars and s-processing

3. Properties ofNe22(α,n)25Mg resonances

4. Reaction rates of the s-process neutron sources Ne-22(alpha, n)Mg-25 and C-13(alpha, n)O-16

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1. <sup>22</sup>Ne(α, n)<sup>25</sup>Mg: The key neutron source in massive stars;Chinese Science Bulletin;2022-05-24

2. Decay properties of 22Ne + α resonances and their impact on s-process nucleosynthesis;Physics Letters B;2020-03

3. Alpha-Capture Reaction Rate for $$^{22}$$ Ne( $$\alpha $$ , n) via Sub-Coulomb $$\alpha $$ -Transfer and Its Effect on Final Abundances of s-Process Isotopes;Springer Proceedings in Physics;2019

4. High-resolution study of levels in the astrophysically important nucleus Mg26 and resulting updated level assignments;Physical Review C;2018-04-30

5. Re-examining the Mg26(α,α′)Mg26 reaction: Probing astrophysically important states in Mg26;Physical Review C;2017-11-08