咨询与建议

看过本文的还看了

相关文献

该作者的其他文献

文献详情 >Large-Scale Shell Model for Nu... 收藏

Large-Scale Shell Model for Nuclear Structure and Nuclear Astrophysics Studies

Large-Scale Shell Model for Nuclear Structure and Nuclear Astrophysics Studies

作     者:王韩奎 金华 孙扬 何翊绮 秦伟 王高亮 WANG Hankui;JIN Hua;SUN Yang;HE Yiqi;QIN Wei;WANG Gaoliang

作者机构:College of Physics and Telecommunication EngineeringZhoukou Normal University Department of Mathematics and PhysicsShanghai Dianji University Department of Physics and AstronomyShanghai Jiao Tong University College of Mathematics and StatisticsZhoukou Normal University 

出 版 物:《原子核物理评论》 (Nuclear Physics Review)

年 卷 期:2016年第33卷第2期

页      面:242-245页

核心收录:

学科分类:08[工学] 0827[工学-核科学与技术] 082701[工学-核能科学与工程] 

基  金:National Natural Science Foundation of China(11505302 11575112 11135005) 

主  题:large-scale shell model monopole correction single-particle state core-excitation exotic nuclei 

摘      要:The study of neutron-rich nuclei near132 Sn is interesting and important for both nuclear structure and nuclear astrophysics. For a considerably large model space allowing cross-shell excitations,a new effective Hamiltonian is determined by employing the extended pairing-plus-quadrupole model with monopole corrections. Calculations for two mass regions, for the north-east quadrant of132 Sn with Z 50 and N 82 and for the south-west quadrant with Z 50 and N 82, have been performed recently. The structure of these nuclei is analyzed in detail, and the role of the monopole corrections can be clearly seen.

读者评论 与其他读者分享你的观点

用户名:未登录
我的评分