Low-lying resonances in Si26 relevant for the determination of the astrophysical Al25(p,γ)Si26 reaction rate
Author:
Funder
National Science Foundation
U.S. Department of Energy
Florida State University
Argonne National Laboratory
Publisher
American Physical Society (APS)
Link
http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevC.105.035805/fulltext
Reference38 articles.
1. Radioactive 26Al in the galaxy: observations versus theory
2. Aluminum-26 in the early solar system - Fossil or fuel
3. The Imprint of Nova Nucleosynthesis in Presolar Grains
4. Observation of the $^{26}Al$ emission distribution throughout the Galaxy with INTEGRAL/SPI
Cited by 4 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献
1. Measurement of the Al25(d,n)Si26 reaction and impact on the Al25(p,γ)Si26 reaction rate;Physical Review C;2023-12-14
2. Confirmation of a new resonance in Si26 and contribution of classical novae to the galactic abundance of Al26;Physical Review C;2023-09-14
3. Si28(p,t)Si26 data reconsidered for the astrophysical Al25(p,γ)Si26 rate;Physical Review C;2023-09-12
4. Progress on nuclear reaction rates affecting the stellar production of 26Al;Journal of Physics G: Nuclear and Particle Physics;2023-01-01
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