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The Li-8(d, p)Li-9 reaction and astrophysical B-8(p, gamma)C-9 reaction rate

机译:Li-8(d,p)Li-9反应和天体B-8(p,γ)C-9反应速率

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摘要

Angular distribution of the Li-8(d, p)Li-9(g.s). reaction at E-cm = 7.8 MeV was measured in inverse kinematics. The square of asymptotic normalization coefficient (ANC) for the virtual decay Li-9 -> Li-8 + n was derived to be 1.33 +/- 0.33 fm(-1) through distorted wave Born approximation (DWBA) analysis, for the first time. According to charge symmetry, (ANC)(2) for C-9 -> B-8 + p was then extracted to be 1. 14 +/- 0.29 fm(-1). We have deduced the astrophysical S-factors and reaction rates for direct capture in B-8(p, y)C-9 at energies of astrophysical relevance using the ANC for C-9 -> B-8 + p extracted from the mirror system. (c) 2005 Elsevier B.V. All rights reserved.
机译:Li-8(d,p)Li-9(g.s)的角分布。以反向运动学测量E-cm = 7.8 MeV时的反应。对于虚拟衰减Li-9-> Li-8 + n的渐近归一化系数(ANC)的平方是通过失真波博恩近似(DWBA)分析得出的,其第一个值为1.33 +/- 0.33 fm(-1)时间。根据电荷对称性,然后将C-9-> B-8 + p的(ANC)(2)提取为1. 14 +/- 0.29 fm(-1)。我们已经推论了天体物理S因子和反应速率,可使用ANC的C-9-> B-8 + p从镜面系统中提取,以天体相关性的能量直接捕获B-8(p,y)C-9 。 (c)2005 Elsevier B.V.保留所有权利。

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