天体物理反应产率测量的改进活化法

S. Artemov, S. Igamov, A. Karakhodzhaev, O. R. Tojiboyev, F. Ergashev, N. Burtebayev, I. Kholbaev, R. F. Rumi, Sh. Kh. Eshkobilov, R. I. Khalikov
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引用次数: 0

摘要

提出了原始的活化方法,并利用该方法测量了天体物理相关反应[公式:见文]在能量区190-650[公式:见文]keV处的产率。通过产率值在温度范围内计算反应速率[公式:见文本]。证明了改进测量非常小的产率或截面的方法的可能性。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Modificated activation method for measurement of the yield of the astrophysical reactions
The original version of the activation method is presented and yield of the astrophysical relevant reaction [Formula: see text] has been measured at the energy region 190–650[Formula: see text]keV using this method. The rate of this reaction was calculated within the temperature region [Formula: see text] through the yield values. The possibility of improving the method for measuring very small yields or cross sections was demonstrated.
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