以改进的定域密度近似研究核子-有限核的相对论微观光学势

本文以Walecka模型为基础,研究改进的定域密度近似下的核子-有限核的相对论微观光学势。采用高斯形状因子折叠定域密度近似下的光学势,得到包含相互作用力程效应的改进的定域密度近似下的光学势。高斯形状因子中的参数由符合P-⁴⁰Ca光学势的体积分与均方根半径的唯象值来决定。与定域密度近似计算相比,改进的定域密度近似下的微观光学势与唯象势更加接近,以此光学势分析质子与核的弹性散射,亦得到与实验值符合得更好的结果。 关键词：     

核结构效应对重离子阻尼碰撞中核子交换过程的影响

本文基于核子交换模型,其中包括不同原子核之间的核子交换和同一个原子核内的粒子空穴激发,同时考虑了能量自由度与质量自由度之间的耦合.目的是研究原子核碰撞中形状的动力学变化过程特别是颈自由度和原子核的壳层结构对于核子交换过程以致对于碎片质量和电荷的一次矩,二次矩,中子质子关联函数以及能量耗散影响.并将计算结果与实验数据进行了比较和讨论.     

Isospin Effect of Coulomb Interaction on Nuclear Stopping in Intermediate Energy Heavy Ion Collisions

Nuclei offer an interesting isospin situation where symmetry potential, Coulomb term and isopin dependent nucleon-nucleon collisions are simultaneously present. However, in general, Coulomb potential is not studied in the heavy ion collisions. As we know that the Coulomb potential is an important asymmetry term which can bring important isospin effect into the observable in the intermediate energy heavy ion collisions. Recently extensions by Colonna et al.[1] to finite nuclei show that Coulomb and surface effects reduce instability regions. So in this paper the isospin effects of Coulomb term and symmetry potential on the nuclear stopping at intermediate energy heavy ion collisions are studied by using isospin-dependent quantum molecular dynamics model (IQMD).     

J/ψ→ppω过程的协变张量分析方法

在相对论协变张量分析的理论框架下,给出了衰变道J/ψ→ppω对应各种可能的中间共振态N*的衰变振幅,通过Monte-Carlo模拟,得到该衰变道中p(p)角分布、pω(pω)不变质量分布及Dalitz图等.     

邮票上的物理学史(61)--粒子物理学:观念和理论

粒子物理学是1897年随着汤姆孙发现电子而建立的.其发展迄今可以分为三个阶段,每个阶段历经三四十年.     

色屏蔽效应与核子-核子相互作用

利用包含屏蔽效应的色禁闭位,我们研究了核子-核子相互作用.结果表明,在用含有色屏蔽效应的禁闭位代替线性或谐振子禁闭位后,不仅解决了色Van der Waals力的长尾巴问题,而且色Van Waals力提供了一部分核子-核子相互作用的中程吸引.     

Effect of 0h11/2 Level on Shell Model Calculations of ^105Sb and ^107Sb

The full and reduced shell model calculations have been carried out for the light odd-even ^105Sb and ^107Sb isotopes. The model space has been chosen as 1d5/2, 0g7/2, 1d3/2, 2s1/2, and 0h11/2 for the full calculations and excluded 0h11/2 for the reduced calculations. The reduced shell model calculations of ^105Sb and ^107Sb isotopes are presented for the first time. We obtain the energy spectra for the ^105Sb and ^107Sb isotopes in the full and reduced model space by using CD-Bonn two-body effective nucleon-nucleon interaction. The resulting energy spectra are compared to the experimental results to understand the effect of the 0h11/2 level on the shell model calculations. We draw conclusions about the right model space in the shell model calculations for the isotopes around the N =Z= 50 region of the periodic table.     

Isotope Dependence of Superheavy Nucleus Formation Cross Section

The dynamical process in the superheavy nucleus synthesis is studied on the basis of the two-dimensional Smoluchowski equation. Special attention is paid to the isotope dependence of the cross section for the superheavy nucleus formation by means of making a comparison among the reaction systems of ^54Re＋204pb, ^56Re ＋206Pb, and ^58Fe＋^208Pb. It is found by this comparison that the formation cross section is very sensitive to the conditional saddle-point height and the neutron separation energy of the compound nucleus. Reaction systems with lower height of conditional saddle-point and smaller neutron separation energy are more favourable for the synthesis of the superheavy nucleus.     

在非拓扑孤立子模型中核子的电磁形状因子

从Friedberg-李政道的非拓扑孤立子模型出发得到一个新的夸克禁闭势.利用这个新的禁闭势,预言了核子的静态性质,并与实验数据进行了比较.理论很好地解释了实验结果.