Microscopic interpretation of the results of new measurements for the 3He(α, γ)7Be reaction

被引：4
|
作者：
Solovyev, A. S. [1 ]
Igashov, S. Yu. [1 ]
Tchuvil'sky, Yu. M. [2 ]
机构：
[1] Dukhov All Russia Res Inst Automat VNIIA, Moscow 127055, Russia
[2] Moscow MV Lomonosov State Univ, Skobeltsyn Inst Nucl Phys, Moscow 119991, Russia
来源：
PHYSICS OF ATOMIC NUCLEI | 2014年 / 77卷 / 12期
关键词：
Atomic Nucleus; Solar Neutrino; Microscopic Approach; Recent Experimental Data; Partial Cross Section;
D O I：
10.1134/S1063778814120175
中图分类号：
O57 [原子核物理学、高能物理学];
学科分类号：
070202 ;
摘要：
A microscopic approach based on the algebraic version of the resonating group method was implemented by applying it to the radiative capture reaction He-3(alpha, gamma)Be-7. The astrophysical S-factor of the reaction and the branching ratio between the capture to the ground and the first excited states of the Be-7 nucleus were calculated. A comparison of the theoretical results with the most recent experimental data was performed, and good agreement with these data was found. Advantages of the theoretical approach realized are indicated, and possible ways to refine upon it are outlined.
引用
收藏
页码：1453 / 1455
页数：3
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