| Production of ^10c Secondary Beam |
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| 引用本文： | SU Jun LI Zhi-hong LIAN Gang WANG You-bao GUO Bing ZENG Sheng YAN Sheng-quan WANG Bao-xiang BAI Xi-xiang LIU Wei-ping. Production of ^10c Secondary Beam[J]. 中国原子能科学研究院年报, 2005, 0(1): 96-98 |
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| 作者姓名： | SU Jun LI Zhi-hong LIAN Gang WANG You-bao GUO Bing ZENG Sheng YAN Sheng-quan WANG Bao-xiang BAI Xi-xiang LIU Wei-ping |
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| 基金项目： | 国家自然科学基金资助项目（10235030） |
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| 摘 要： | 理论上存在着两种矛盾的预言，即通过碰撞核相对运动与破裂道的耦合使全熔合截面压低或增强。最近，Hagino作了一改进的耦合道模型计算，试图调和两种相冲突的处理。他的理论处理预言结果，在库仑位垒以下能区破裂使全熔合截面增强，而在垒上能区，破裂使全熔合截面压低。不同的理论预言，需要精确可靠的实验作判断。
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| 关 键 词： | ^10C 核反应 核合成 次级束 |
Production of ^10c Secondary Beam |
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| Abstract: | The inhomogeneous big bang models assume a universe with regions of high-density proton-rich materials surrounded by those of low-density neutron-rich materials, thus many reactions caused by unstable nuclei are very important. Fig. 1 shows a part of the nuclear reaction network of primordial nucleosynthesis . The reactions related to ^10C are considerable in the investigation of primordial nucleosynthesis. |
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