Radii of Thorium Nuclides Lying in Between the Drip Lines

U. E, Prof Antony Joseph
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Abstract

Background: Nuclear rms radii give information about the nuclear structure, nuclear shape, deformation etc. Microscopic methods are widely used for the study of nuclear structure properties. Hartree-Fock method with an effective interaction of Skyrme force is used for studying the nuclear structure properties.Purpose: To calculate the rms radii of proton and neutron for thorium nuclei, lying between the drip lines, by using the microscopic mean field theory. The nuclear rms radii data is useful for identifying the shape variation of thorium nuclei, from proton drip line to neutron drip line. It also helps to identify the trends in nuclear radii variation as we move towards the drip line. This nuclear data will be useful in designing experiments in future and also in understanding the behaviour of complex nuclei. Microscopic study of thorium nuclei is also important in the astrophysical environments.Methods: This study is based on the Skyrme interacting potential in the Hartree-Fock mean field theory. Iterative diagonalization method with the help of a computational code is used for solving the Hartree-Fock equation.Results: We have calculated the rms radii of neutron, proton and their total with SV, SLY4 and UDF2 parametrization of the Skyrme force. Neutron rms radii, proton rms radii and total rms radii of thorium nuclei are found to increase with neutron number. UDF2 parametrization shows an oscillatory nature in the rms radii. This may be due to the shape change of thorium nuclei when adding neutrons.Conclusions: The rms radii of thorium nuclei are found to increase with neutron number. The Skyrme force with UDF2 parametrization is the most suitable one for the structure studies of thorium nuclei.
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滴油管之间钍核素的半径
背景:核均方根半径提供了核结构、核形状、核变形等信息。显微方法被广泛用于核结构性质的研究。采用具有Skyrme力有效相互作用的Hartree-Fock方法研究了核的结构性质。目的:用微观平均场理论计算滴线之间钍核的质子和中子的均方根半径。核均方根半径数据对于确定钍原子核从质子滴线到中子滴线的形状变化是有用的。它还有助于确定核半径变化的趋势,因为我们移动到滴油管。这些核数据对将来设计实验和理解复杂核的行为是有用的。钍核的微观研究在天体物理环境中也很重要。方法:基于Hartree-Fock平均场理论中的Skyrme相互作用势进行研究。在计算代码的帮助下,采用迭代对角化方法求解Hartree-Fock方程。结果:我们用SV、sl4和UDF2参数化计算出了中子、质子的均方根半径和总均方根半径。钍原子核的中子均方根半径、质子均方根半径和总均方根半径随中子数的增加而增大。UDF2参数化在均方根半径上显示出振荡性质。这可能是由于加入中子后钍原子核的形状发生了变化。结论:钍原子核的均方根半径随中子数的增加而增大。采用UDF2参数化的Skyrme力最适合于钍原子核的结构研究。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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