节点文献
超重核的壳结构
Shell Structure of Superheavy Nuclei
【摘要】 在相对论连续谱Hartree Bogoliubov(RCHB)理论框架下,在质子数Z=100—140和中子数N=Z+30—2Z+32等偶偶核中进行了超重球形双幻核的探索.采用的有效相互作用为NL1,NL3,NLSH,TM1,TW 99,DD ME1,PK1和PK1R.基于对双核子分离能(S2p和S2n)、双核子能隙(δ2p和δ2n)、壳修正能量(Epshell)、对能(Eppair和Enpair)和有效对能隙(Δp和Δn)等物理量和能shell和En级结构的分析,预言了可能的质子幻数和中子幻数,并观察到在超重核区壳的弱化现象.
【Abstract】 The magic proton and neutron numbers are searched in the superheavy region with proton number Z=100 —140 and neutron number N=(Z+30) — (2Z+32) by the relativistic continuum Hartree-Bogoliubov (RCHB) theory with interactions NL1, NL3, NLSH, TM1, TW99, DD-ME1, PK1, and PK1R. Based on the two-nucleon separation energies S2p and S2n , the two-nucleon gaps δ2p and δ2n, the shell correction energies Epshell and Enshell, the pairing energies Eppair and Enpair, and the pairing gaps Δp and Δn, some proton numbers and neutron numbers are suggested to be the magic numbers within the present approach. The shell quenching phenomena are observed in the region of the superheavy nuclei.
【Key words】 superheavy nuclei; relativistic mean field theory; shell structure;
- 【文献出处】 原子核物理评论 ,Nuclear Physics Review , 编辑部邮箱 ,2004年04期
- 【分类号】O571.21
- 【被引频次】1
- 【下载频次】105