γ Decay of New Neutron-rich Nuclei ^(175)Er
γ Decay of New Neutron-rich Nuclei  ̄(175)Er
摘要
γ Decay of New Neutron-rich Nuclei ^(175)ErγDecayofNewNeutron-richNuclei^(175)Er¥ZhangXueqian;YuanShuanggui;YangWeifan;YuXian;...
-
1Gu Jinnan and Zhang Changhua.Structure Properties of Light Neutron-rich Nuclei[J].IMP & HIRFL Annual Report,1994(0):116-116.
-
2Relativistic Mean-field Study of Light Neutron-rich Nuclei[J].Annual Report of China Institute of Atomic Energy,1995(0):13-14.
-
3郭艳青,任中洲.Structures of Light Neutron-Rich Nuclei with Orbit-Orbit Coupling[J].Chinese Physics Letters,2007,24(3):652-655. 被引量:1
-
4颜廷志,李龙龙,王瑞丰,颜廷锋.Yield ratios and directed flows of light fragments from reactions induced by neutron-rich nuclei at intermediate energy[J].Chinese Physics C,2017,41(4):75-79.
-
5Neutron Halo and Spin-orbit Splitting in some Neutron-rich Nuclei[J].Annual Report of China Institute of Atomic Energy,1995(0):12-12. 被引量:1
-
6LIQing-Feng,LIZhu-Xia,ZHAOEn-Guang,H.Stoecker.Re-visit N/Z Ratio of Free Nucleons from Collisions of Neutron-Rich Nuclei as a Probe of EoS of Asymmetric Nuclear Matter[J].Communications in Theoretical Physics,2004,41(3):435-440.
-
7Rajiv Kumar,Rajesh Kharab,H. C. Sharma.Intermediate Energy Coulomb Excitation of Neutron-Rich Nuclei[J].Chinese Physics Letters,2010,27(3):104-107.
-
8LI Qing-feng,LI Zhu-xia.Re-visit N/Z Ratio of Free Nucleons From Collisions of Neutron-Rich Nuclei as a Probe of EoS of Asymmetric Nuclear Matter[J].Annual Report of China Institute of Atomic Energy,2005(1):70-70.
-
9LI Qing-feng , LI Zhu-xia.Re-visit the N/Z Ratio of Free Nucleons From Collisions of Neutron-rich Nuclei as a Probe of EoS of Asymmetric Nuclear Matter[J].Annual Report of China Institute of Atomic Energy,2004(1):29-30.
-
10Wang Meng, Xiao Guoqing, Zhan Wenlong, Guo Zhongyan, Wang JiansongSun Zhiyu, Li Jiaxing, Tian Wendong, Chen Zhiqiang, Xiao ZhigangMao Ruishi, RIKEN group and INP group.Reaction Cross-section Measurements of Neutron-rich Nuclei ^(11,12,14)Be and ^(13-15)B[J].近代物理研究所和兰州重离子加速器实验室年报:英文版,2002(1):26-26.