Apparent charge symmetry violation in the D(d, p)T and D(d, n)3He fusion reactions at stellar energies

被引:2
|
作者
Nebia, F
Beaumevieille, H
Ouichaoui, S
机构
[1] Univ Sci & Technol Houari Boumediene, Fac Sci, Bab Ezzouar 16111, Alger, Algeria
[2] Univ Grenoble 1, F-38026 Grenoble, France
[3] CNRS, IN2P3, Inst Sci Nucl, F-38026 Grenoble, France
关键词
astrophysical factor; anisotropy; WKB approximation; D(d; p)T; n)He-3;
D O I
10.1016/S1631-0705(02)01362-2
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The existing experimental data concerning the D(d,p)T and D(d,n)He-3 reactions at stellar energies are analysed using the WKB approximation. The s and p partial waves decomposition of the astrophysical S(E) factor is presented; the anisotropies are also investigated. An interpretation coherent with the charge symmetry of the p wave astrophysical factor, S-l(i)(E), and the anisotropy, A(i)(E) (i = n, p), for these fusion reactions is given in terms of two known l(-) levels in He-4 at Ex = 23.64 MeV (T = 1) and 24.25 MeV (T = 0).
引用
收藏
页码:733 / 739
页数:7
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