| Determination of Astrophysical ^26Si（p, γ）^27p Reaction Rate From Asymptotic Normalization Coefficients of ^27Mg →^26Mg ＋ n |
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| 作者姓名： | GUO Bing LI Zhi-hong BAI Xi-xiang LIU Wei-ping SHU Neng-chuan CHEN Yong-shou |
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| 摘 要： | The 1.809 MeV T-ray from the decay of ^26Al is an excellent observable for some astrophysical events, such as novae and X-ray burst. The nucleosynthesis of ^26A1 is dominated by the reaction chain ^24Mg（p,γ）^25Al（β＋）^25Mg（p,γ）^26Al, however,
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| 关 键 词： | 天体物理 ^26Si（p γ）^27P反应 反应截面 反应率 衰变 渐近标准化系数 |
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