| Production of ^13N Secondary Beam |
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| 引用本文： | ZENG Sheng LI Zhi-hong LIAN Gang WANG You-bao SU Jun YAN Sheng-quan WANG Bao-xiang GUO Bing BAI Xi-xiang LIU Wei-ping. Production of ^13N Secondary Beam[J]. 中国原子能科学研究院年报, 2006, 0(1): 110-111 |
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| 作者姓名： | ZENG Sheng LI Zhi-hong LIAN Gang WANG You-bao SU Jun YAN Sheng-quan WANG Bao-xiang GUO Bing BAI Xi-xiang LIU Wei-ping |
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| 基金项目： | Supported by National Natural Science Foundation （ 10575136） |
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| 摘 要： | Explosive hydrogen burning occurs in very massive （M≥ 10^5-10^8M） star with high temperature and density. Hot pp chain, hot CNO, hot NeNa-MgAl chain and the flowing rp ap process will play a prominent role in hydrogen burning as the temperature goes higher. When the temperature of the star is higher than 10^8 K, high temperature CNO chain is dominant in hydrogen burning,
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| 关 键 词： | 氮 同位素 生产量 原子核 |
Production of ^13N Secondary Beam |
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