Indirect measurement of the 57.7 keV resonance strength for the astrophysical γ -ray source of the Mg25(p,γ)Al26 reaction
Author:
Funder
National Natural Science Foundation of China
National Basic Research Program of China
Continuous Basic Scientific Research
Publisher
American Physical Society (APS)
Link
http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevC.102.025804/fulltext
Reference47 articles.
1. HEAO 3 discovery of Al-26 in the interstellar medium
2. Radioactive 26Al from massive stars in the Galaxy
3. Excess 26Mg in the Allende Meteorite
4. Carbon, nitrogen, magnesium, silicon, and titanium isotopic compositions of single interstellar silicon carbide grains from the Murchison carbonaceous chondrite
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1. Updated reaction rate of Mg25(p,γ)Al26 and its astrophysical implication;Physical Review C;2023-06-05
2. Progress on nuclear reaction rates affecting the stellar production of 26Al;Journal of Physics G: Nuclear and Particle Physics;2023-01-01
3. First result from the Jinping Underground Nuclear Astrophysics experiment JUNA: precise measurement of the 92 keV 25Mg(p, γ)26Al resonance;Science Bulletin;2022-01
4. Measurement of the low energy 25Mg(p,γ)26Al resonances;EPJ Web of Conferences;2022
5. Direct measurement of the resonance strengths and branching ratios of low-energy (p, γ) reactions on Mg isotopes *;Chinese Physics C;2021-08-01
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