The hep reaction and the solar neutrino problem

被引：0
|
作者：
Marcucci, LE [1 ]
机构：
[1] Old Dominion Univ, Dept Phys, Norfolk, VA 23529 USA
来源：
NUCLEAR PHYSICS A | 2001年 / 689卷 / 1-2期
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D O I：
暂无
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：
The results of a new calculation of the astrophysical S-factor for the proton weak capture on He-3 are reviewed. The method used to obtain very accurate initial and final state wave functions and to construct the nuclear weak current operator is described. Finally, the implications of these results for the Super-Kamiokande solar neutrino data are discussed.
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页码：280C / 289C
页数：10
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