Determination of the ^25Mg（p,γ）^26Al resonance strength at Ec.m.=58 keV via shell model calculation

来源 :中国科学：物理学、力学、天文学英文版 | 被引量 : 0次 | 上传用户：qq_13439718

【摘要】

：

The observation of 26 Al is an useful tool for γ-ray astronomy and in studies of galactic chemical evolution. The most likely mechanism for 26A1 nucleosynthesi

【作者】

：

LI ZhiHong SU Jun LI YunJu GUO

【机构】

：

ChinaInstituteofAtomicEnergy,CollegeofPhysicsScienceandTechnology

【出处】

：

中国科学：物理学、力学、天文学英文版

【发表日期】

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2015年8期

【关键词】

：

共振强度壳模型计算电子测定地下实验室化学演化温度范围 γ-ray astronomy astrophysical reaction rate

【基金项目】

：

This work was supported by the National Natural Science Foundation of China （Grant Nos. 11490563, 11375269 and 11321064） and the National Key Basic Research Development Program （Grant No. 2013CB834406

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The observation of 26 Al is an useful tool for γ-ray astronomy and in studies of galactic chemical evolution. The most likely mechanism for 26A1 nucleosynthesis is in the hydrogen burning Mg Al cycle, and the 26A1 production reaction 25Mg(p,γ)26Al at the

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Determination of the ^25Mg（p,γ）^26Al resonance strength at Ec.m.=58 keV via shell model calculation

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