176Yb的β衰变

采用投影壳模型对¹⁷⁶Yb的β衰变进行了计算, 并与实验结果进行了比较.     

IBFM模型U(6/4)超对称SO(6)极限的能谱统计

用相互作用玻色子费米子模型(IBFM)计算了奇A核U(6/4)超对称SO(6)极限的理论能谱，对不确定核的最近邻能级间距分布和能谱刚性度进行了研究，并对影响能谱统计特征的因素进行了讨论. 结果表明，有限的玻色子数N的大小显著地影响能谱统计. 当N接近于真实核的玻色子数时，子群SOBF(5)的作用强度和自旋对能谱统计起重要作用. 然而，当N趋于无穷大时，能谱统计总是趋于Poisson分布.     

对初中数学深度学习的探索

初中生受身心发展局限性的影响,他们的学习行为有时停留在浅层学习(Surface Learning)的层面,存在碎片化、浅表化、浮躁化的显现和忧虑.学生很难深度加工知识信息、深度理解复杂概念、深度掌握内在含义,进而建构个人化和情境化的知识体系以解决复杂问题.为此,笔者探索数学深度学习(Deep Learning)发生的可能途径,力图破解停留于浅层的问题.     

Efect of Tensor Force on the Halo Structure of ~(29)Ne and ~(31)Ne

The structure of Ne isotopes has been investigated by using deformed Skyrme–Hartree–Fock(SHF)method and BCS approximation.Especially the efect of tensor force on the halo structure of 29Ne and 31Ne is discussed.To this end,the tensor contributions are considered to the energy density function and the single particle potential in SHF theory.For comparison,four Skyrme interactions are used:SLy5 and SGII without tensor force,and SLy5+T and SGII+T with tensor force.The results indicate that the inclusion of tensor force shows a more pronounced halo structure for31Ne.