逆二次赫尔曼势的相对论能量和信息熵

Q2 Physics and Astronomy Physics Open Pub Date : 2023-05-01 DOI:10.1016/j.physo.2023.100152
I.J. Njoku, C.P. Onyenegecha, C.J. Okereke, P. Nwaokafor, C.C. Abara
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引用次数: 0

摘要

利用参数化Nikiforov-Uvarov (pNU)方法,利用逆二次Hellman (IQH)势,得到了自旋和伪自旋对称极限下的Dirac方程的解。在精确的非相对论自旋对称极限下,得到了IQH势的能量和波函数,并用于研究系统的香农信息熵。给出了具有IQH势的Dirac方程的自旋和伪自旋对称极限的相对论能量的数值结果,并观察到它们表现出简并性。6个状态(n = 0、1、2、3、4、5)的Shannon熵结果表明,动量空间波函数和概率密度比位置空间波函数具有更好的局域性。并验证了系统的Bialynicki-Birula和Mycielski (BBM)不等式。我们的结果与先前文献报道的结果一致。
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Relativistic energies and information entropy of the inversely quadratic Hellmann potential

The solutions to the Dirac equation are obtained in the spin and pseudospin symmetry limits are presented using the parametric Nikiforov-Uvarov (pNU) method with the inversely quadratic Hellman (IQH) potential. In the exact non-relativistic spin symmetry limit, the energy and wave function of the IQH potential are obtained and used to investigate the Shannon information entropy of the system. Numerical results of the relativistic energies of the spin and pseudospin symmetry limits of the Dirac equation with the IQH potential are presented and observed to exhibit degeneracy. Also, the results of the Shannon entropy for six states (n = 0, 1, 2, 3, 4, 5) show that the momentum space wave function and probability density are better localized than the position space wave function. Also, the Bialynicki-Birula and Mycielski (BBM) inequality is verified for the system. Our results are found to be consistent with those previously reported in the literature.

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来源期刊
Physics Open
Physics Open Physics and Astronomy-Physics and Astronomy (all)
CiteScore
3.20
自引率
0.00%
发文量
19
审稿时长
9 weeks
期刊最新文献
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