Effects of shell correction on α decay properties

The shell correction effects on the α decay properties of heavy and superheavy nuclei have been studied in a macroscopic-microscopic manner. The macroscopic part is constructed from the generalized liquid drop model(GLDM), whereas the microscopic part, namely, the shell correction energy, brings about certain effects on the potential barriers and half-lives under a WKB approximation, which is emphasized in this work. The results show that the shell effects play a significant role in the estimation of the α decay half-lives within the actinide region.Predictions of the α decay half-lives are then generated for superheavy nuclei, which will provide useful information for future experiments.     

多粒子多空穴能态密度的谐振子模型计算

在严格考虑了泡利不相容原理的前提下,导出了任意单粒子哈密顿量下多粒子多空穴态的能态密度的一般性精确公式;并应用半经典的Thomas-Fermi近似,计算了三维线性谐振子下的能态密度;计算了g_1p至g_10p,g_1h至g_7h以及g_1p－1h至g_6p－6h能态密度;讨论了泡利不相容的影响,与微子模型中通用的等间隔模型的能态密度进行了比较.由计算结果看出,激子模型中通用的等间隔单粒子能级密度模式在由核子诱发的核反应中,是一很好的近似.     

n+11B反应的理论计算和分析

在统一的豪泽–费许巴赫理论和激子模型的基础上,利用光学模型来处理中子诱发轻核核反应的一种新理论已经产生.利用这一新理论,对当入射中子En≤20MeV时n+¹¹B反应的所有反应截面,出射中子和α粒子的双微分截面进行了计算.通过比较理论计算的各种截面,出射中子总的双微分截面与实验数据,可以认为这一理论模型处理轻核核反应是很成功的.