Level Widths of Low-lying 16F States From 15N（7Li, 6Li）16N Reaction  

作　　者：DU Xian-chao GUO Bing LI Zhi-hong LI Yun-ju SU Jun YAN Sheng-quan BAI Xi-xiang FAN Qi-wen GAN Lin JIN Sun-jun JING Long LI Er-tao LI Zhi-chang LIAN Gang LIU Jian-cheng SHEN Yang-ping TANG Xiao-dong WANG You-bao WU Zhi-dan ZENG Sheng ZHANG Wei-jie LIU Wei-ping 

机构地区：[1]Depar tment of Nuclea r Physics [2]College of Physics Science and Technology,Shenzhen University [3]Institute of Modern Physics,Chinese Academy of Sciences

出　　处：《Annual Report of China Institute of Atomic Energy》2013年第1期48-48,共1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(11321064,11075219,11375269,11275272,1275018);973 Program of China(2013CB834406)

摘　　要：12C(α,γ)16O reaction plays a crucial role in stellar nucleosynthesis.To date the lowest energy of the measurement of this reaction is about 0.9 MeV in center-of-mass frame.The extrapolation of the measured cross sections to lower energies is complicated by two states located at 45 keV(Jπ=1-)and245 keV(Jπ=2+)levels below the 12C+αthreshold.The cross section at low energies of

关 键 词：STELLAR SECTIONS lowest TAILS Breit distorted constrained WEAKLY ANGULAR largely 

分 类 号：P144[天文地球—天体物理]