Publication Date:
2013-01-18
Description:
Author(s): B. Guo (郭冰), J. Su (苏俊), Z. H. Li (李志宏), Y. B. Wang (王友宝), S. Q. Yan (颜胜权), Y. J. Li (李云居), N. C. Shu (舒能川), Y. L. Han (韩银录), X. X. Bai (白希祥), Y. S. Chen (陈永寿), W. P. Liu (柳卫平), H. Yamaguchi (山口英斉), D. N. Binh, T. Hashimoto (橋本尚志), S. Hayakawa (早川勢也), D. Kahl, S. Kubono (久保野茂), J. J. He (何建军), J. Hu (胡钧), S. W. Xu (许世伟), N. Iwasa, N. Kume, and Z. H. Li (李智焕) The evolution of massive stars with very low-metallicities depends critically on the amount of CNO nuclides which they produce. The 12 N( p , γ ) 13 O reaction is an important branching point in the rap processes, which are believed to be alternative paths to the slow 3 α process for producing CNO seed nucl... [Phys. Rev. C 87, 015803] Published Thu Jan 17, 2013
Keywords:
Nuclear Astrophysics
Print ISSN:
0556-2813
Electronic ISSN:
1089-490X
Topics:
Physics
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