在协变密度泛函理论框架内研究镜像核的中子皮厚和质子半径的变化趋势

IF 1.5 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
Pankaj Kumar, Sarabjeet Kaur, Virender Thakur, Raj Kumar, Shashi K. Dhiman
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引用次数: 0

摘要

原子核的中子外皮会影响富中子原子核的结构,但其精确测量却相当具有挑战性。我们采用基于密度依赖介子交换相互作用的共变密度函数理论(CDFT),对轻到中等质量原子核的中子表面和质子半径进行了预测。利用我们的微观预测,我们发现中子皮层和等时空不对称之间存在线性相关。计算还扩展到发现镜像核的质子和中子半径之间的线性关系。利用核力的电荷对称性,还研究了富中子核的中子表面与相应镜像核对的质子半径之差之间的相关性。研究发现,加入 ISB 项会影响 48Ca-48Ni 镜像核对的镜像差电荷半径。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
A study of trends of neutron skin thickness and proton radii of mirror nuclei within the framework of covariant density functional theory

The neutron skin of atomic nuclei impacts the structure of neutron-rich nuclei, but its accurate measurement is quite challenging. We present predictions for neutron skins and proton radii for light to medium mass nuclei by employing Covariant Density Functional Theory (CDFT) based on density-dependent meson-exchange interaction. Using our microscopic predictions, we find a linear correlation between the neutron skin and the isospin asymmetry. The calculations are also extended to find a linear relationship between proton and neutron radii of mirror nuclei. Using the charge symmetry property of nuclear forces, a correlation between the neutron skin of neutron-rich nuclei and difference between the proton radii of the corresponding mirror pair has also been investigated. The inclusion of ISB term is found to affect the mirror difference charge radii of 48Ca-48Ni mirror pair.

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来源期刊
Modern Physics Letters A
Modern Physics Letters A 物理-物理:核物理
CiteScore
3.10
自引率
7.10%
发文量
186
审稿时长
3 months
期刊介绍: This letters journal, launched in 1986, consists of research papers covering current research developments in Gravitation, Cosmology, Astrophysics, Nuclear Physics, Particles and Fields, Accelerator physics, and Quantum Information. A Brief Review section has also been initiated with the purpose of publishing short reports on the latest experimental findings and urgent new theoretical developments.
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