Revised decay properties of the key 93-keV resonance in the Mg 25 ( p , ? ) reaction and its influence on the MgAl cycle in astrophysical environments

Revised decay properties of the key 93-keV resonance in the Mg 25 ( p , ? ) reaction and its influence on the MgAl cycle in astrophysical environments
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修正了 Mg 25 ( p , ? ) 反应中关键 93-keV 共振的衰变特性及其对天体物理环境中 MgAl 循环的影响

DOI:
10.1103/physrevc.105.l042801
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发表时间:
2022
期刊:
影响因子:
3.1
通讯作者:
Lotay G
Lotay G
中科院分区:
物理与天体物理2区
文献类型:
--
作者:
Lotay G

文献摘要

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用聚变-蒸发反应重新研究了6398.3(8)keV激发态的衰变性质。该能级表示系统中一个关键的93.1(8)-keV共振,其相对分支到基态,已被确定为(stat.)(system .)。这比最近的评估值高得多,意味着放射性产生的宇宙射线有相当大的增加。
The-decay properties of an excited state inat 6398.3(8) keV have been reexamined using thefusion-evaporation reaction. This level represents a key 93.1(8)-keV resonance in thesystem and its relative branching to theground state,, has been determined to be(stat.)(syst.). This is a significantly higher value than the most recent evaluation and implies a considerable increase in the production of cosmicrays fromradioactivity.