Determination ofS17from the7Be(d,n)8Breaction

Determination ofS17from the7Be(d,n)8Breaction
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由 7Be(d,n)8 反应测定 S17

DOI:
10.1103/physrevc.67.011602
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发表时间:
2003
期刊:
影响因子:
3.1
通讯作者:
M. Kamimura
M. Kamimura
中科院分区:
物理与天体物理2区
文献类型:
--
作者:
K. Ogata;M. Yahiro;Y. Iseri;M. Kamimura

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用渐近归一化系数法从E= 7.5MeV的7 Be(d,n)8 B转移反应中可靠地提取了7 Be(p,γ)8 B反应的天体物理因子S17.采用基于三体模型的CDCC对转移反应进行了精确的分析。这种分析是免费的不确定性的光学潜力已在以前的DWBA分析至关重要。
The astrophysical factor S 17 for 7 Be (p, γ) 8 B reaction is reliably extracted from the transfer reaction 7 Be (d, n) 8 B at E= 7.5 MeV with the asymptotic normalization coefficient method. The transfer reaction is accurately analyzed with CDCC based on a three-body model. This analysis is free from uncertainties of the optical potentials having been crucial in the previous DWBA analyses.