WLW 原子核质量模型在r过程研究中的应用

本工作利用最近提出的WLW宏观-微观原子核质量模型, 在经典 r过程框架下 很好地描述了太阳系r过程核素丰度分布. 与常用的FRDM质量模型相比, 新计算更好地再现了A≈ 135和A≈ 180质量区的太阳系r过程核素丰度, 尤其 避免了其他相似计算中A=135 附近出现的 与观测不符的丰度峰问题. 分析表明, 这种差异可能暗示WLW更为合理地处理了壳结构和对称能.     

Exotic Magnetic Rotation in 22F

The rotation structure in exotic neutron-rich nucleus 22F is investigated based on the configuration πd5/2（×）vd5/2s^-1 with the newly developed tilted axis cranking relativistic mean field theory in a fully microscopic and seff- consistent way. The possible existence of magnetic rotation is suggested for ^22F via investigating the spectra, the relation between the rotational frequency and the angular momentum, the electromagnetic transition probabilities B（ M1） and /3（E2） together with the shears mechanism characteristic of magnetic rotation. The effect of the nuclear current is also discussed by comparing the calculation results with and without currents.     

First attempt to overcome the disaster of Dirac sea in imaginary time step method

Efforts have been made to solve the Dirac equation with axially deformed scalar and vector WoodsSaxon potentials in the coordinate space with the imaginary time step method. The results of the singleparticle energies thus obtained are consistent with those calculated with the basis expansion method, which demonstrates the feasibility of the imaginary time step method for the relativistic static problems.     

152Gd核高自旋态的研究

利用¹⁴⁸Nd(⁹Be, 5n)¹⁵²Gd重离子熔合蒸发反应, 对¹⁵²Gd(Z=64, N=88)核的高自旋态进行了研究. 在¹⁵²Gd核中发现了10多个新的高自旋能级和一个新的S带结构. 实验中首次观察到¹⁵²Gd核完整的第一个带交叉, 与推转壳模型计算结果和邻近核实验结果的比较显示带交叉是由一对i_13/2中子的顺排造成的. 通过对¹⁵²Gd核运动学转动惯量的分析, 得到¹⁵²Gd核的形状随着自旋变化的实验证据.     

πg9/2νh11/2 doublet bands in A～100 mass region

Using the model with one particle and one hole coupled with a triaxial rotor, the πg9/2/1/2νh11/2 doublet bands in the A～100 mass region are studied, and compared with the πg9/2/1/2νh11/2 doublet bands. It is found that the calculated results for the configuration of πg9/2/1/2νh11/2 are very similar the results for a pure h11/2 proton particle and a neutron quasiparticle with λn = ε5. After including the pair correlation, the model describes the candidate chiral doublet bands in 106Rh successfully, which supports the interpretation of chirality geometry.     

А∧Ca和А∧∧Ca超核中的巨中子晕现象

利用密度相关零程对力的相对论连续谱Hartree—Bogolubov方法，对偶中子数的Ca同位素从质子滴线到中子滴线范围内的单∧超核和双∧超核基态性质进行了系统研究。与通常的原子核相比，单∧超核和双∧超核中起子提供的吸引力会相应地降低中子费米面。所预言的中子滴线超核分别为А∧Ca和А∧∧Ca，比原来预测的通常滴线核^74Ca多两个中子。基于对双中子分离能、中子密度分布、半径、单粒子能谱、轨道占据数和连续谱贡献的分析，预言了超核中的巨中子晕现象。     

208ΛPb的超子分布半径和中子星结构

从相对论平均场理论出发,考虑核子、超子和介子自由度,研究了208ΛPb的超子分布半径与中子星的性质以及它们之间的关系. 计算发现当超子的耦合常数比值由0.3增大到1时,对NLSH和NL3参数组,超核的超子分布半径分别由3.905和3.849fm增大到4.346和4.230fm,而中子星的最大质量分别由1.516和1.429M⊙增大到2.776和2.744M⊙,质量为1.4M⊙的中子星半径分别由13.13和12.79km增大到13.24和13.29km.即中子星的最大质量和半径随超子分布半径增大而增加. 这样只要从实验上确定208ΛPb的超子分布半径,就可以得到中子星结构的信息.     

Shell Correction at the Saddle Point for Superheavy Nucleus

The potential energy surface for superheavy nucleus has been studied within the framework of the constrained relativistic mean field theory, and the shell correction energy as a function of de[ormation has been extracted by the Strutinsky shell correction procedure. Contrary to the usual expectation, the shell correction energy at the saddle point is too important to be neglected, and it has essential contribution to the fission barrier in superheavy nucleus.     

Λ ACa和ΛΛ ACa超核中的巨中子晕现象

利用密度相关零程对力的相对论连续谱Hartree-Bogoliubov方法,对偶中子数的Ca同位素从质子滴线到中子滴线范围内的单Λ超核和双Λ超核基态性质进行了系统研究.与通常的原子核相比,单Λ超核和双Λ超核中超子提供的吸引力会相应地降低中子费米面.所预言的中子滴线超核分别为77ΛCa和78ΛΛCa,比原来预测的通常滴线核⁷⁴Ca多两个中子.基于对双中子分离能、中子密度分布、半径、单粒子能谱、轨道占据数和连续谱贡献的分析,预言了超核中的巨中子晕现象.     

_Λ~(208)Pb的超子分布半径和中子星结构

从相对论平均场理论出发 ,考虑核子、超子和介子自由度 ,研究了2 0 8ΛPb的超子分布半径与中子星的性质以及它们之间的关系 .计算发现当超子的耦合常数比值由 0 .3增大到 1时 ,对NLSH和NL3参数组 ,超核的超子分布半径分别由3 .90 5和 3 .849fm增大到 4.3 4 6和 4.2 3 0fm ,而中子星的最大质量分别由 1 .51 6和1 .42 9M⊙ 增大到 2 .776和 2 .744M⊙ ,质量为 1 .4M⊙ 的中子星半径分别由 1 3 .1 3和 1 2 .79km增大到 1 3 .2 4和 1 3 .2 9km。即中子星的最大质量和半径随超子分布半径增大而增加 .这样只要从实验上确定2 0 8ΛPb的超子分布半径 ,就可以得到中子星结构的信息