Measurement of ²H(¹²N, ¹³O)n Angular Distribution and Determination of Astrophysical ¹²N（p, γ）¹³O Reaction Rate  

作　　者：GUO Bing SU Jun LI Zhi-hong WANG You-bao YAN Sheng-quan LI Yun-ju SHU Neng-chuan HAN Yin-lu BAI Xi-xiang CHEN Yong-shou LIU Wei-ping H.Yamaguchi D.N.Binh T.Hashimoto S.Hayakawa D.Kahl S.Kubono HE Jian-jun HU Jun XU Shi-wei N.Iwasa N.Kume LI Zhi-huan 

机构地区：[1]Department of Nuclear Physics Center for Nuclear Study,University of Tokyo Institute of Modern Physics,Chinese Academy of Sciences Department of Physics,Tohoku University School of Physics and State Key Laboratory of Nuclear Physics and Technology,Peking University

出　　处：《Annual Report of China Institute of Atomic Energy》2012年第1期60-61,共2页中国原子能科学研究院年报（英文版）

基　　金：Supported by National Natural Science Foundation of China (11021504, 10875175, 10720101076, 10975193, 11075219);973 Program(2013CB834406);KAKEHI of Japan (21340053)

摘　　要：The evolution of massive stars with very low-metallicities depends critically on the amount of CNO nuclides which they produce. The 12N(p, γ)13O reaction is an important branching point in the rap processes, which are believed to be alternative paths to the slow αp process for producing CNO seed nuclei and thus could change the fate of massive stars. In the present work, the angular distribution of

分 类 号：O571.4[理学—粒子物理与原子核物理]