首页> 外文会议>International Symposium on Origin of Matter and Evolution of Galaxies >The extraction of fractions of the resonant component from analyzing powers in ~6Li(d, a)4He and ~6Li(d, po)7Li reactions at very low incident energies
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The extraction of fractions of the resonant component from analyzing powers in ~6Li(d, a)4He and ~6Li(d, po)7Li reactions at very low incident energies

机译:在非常低的入射能中,在〜6LI(d,a)4he和〜6li(d,po)7li反应中分析谐振成分的级分。在非常低的事件能量下

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Recently, several groups deduced the astrophysical S(E) factor for 6Li+d reactions at zero energy using cross section data for astrophysical interests [1, 2]. Generally astrophysical S(E) factor at zero energy was extrapolated from data which is not affected by electron screening. The extrapolated S(E) factor depends on the reaction model. The model dependence especially appears when the cross section has two components, resonant component and nonresonant one. In this work, we extracted the fraction of the resonant component in the ~6Li(d,a)4He and ~6Li(d,p)7Li reactions using polarization observables.
机译:最近,几组使用横截面数据用于天体物理兴趣的横截面数据,将6Li + D的Astrophysical S(E)因子推导出6LI + D反应[1,2]。通常,零能量的天体物理S(e)因子被从未受电子筛选影响的数据推断。外推的S(E)因子取决于反应模型。当横截面有两个组分,谐振分量和非念珠菌时,尤其出现模型依赖性。在这项工作中,我们利用偏振可观察结果提取了〜6LI(D,A)4He和〜6LI(D,P)7LI反应的谐振组分的级分。

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