论文标题
用于天体物理应用的Cu-Isoelectronic AS，SE和BR离子的辐射特性
Radiative properties of Cu-isoelectronic As, Se and Br ions for astrophysical applications
论文作者
论文摘要
我们为$ ns_ {1/2} $，$ np_ {1/2,3/2} $，$ n'd_ {3/2,5/2} $和$ n'f_ $ n'f_ $ n'f_ $ n'f_ $ n'd $ np_ $ n'd_ $ n = 6 $ np np_ $ n = 4，$ n = 4，$ n = 4，$ n = 4，$ n = $ n = 4，$ n = 4，$ n = 4，$ n = 4，$ n = $ n = 4，$ n = 4，$ n = 4，$ n = 4，$ n = $ n = $ n = $ n = $ n = $ np_ $ np_， Cu-Isoelectronic as，se和br ions。由于无法对这些光谱数据进行精确的观察结果，它们的准确估计非常有趣，并且有助于分析包含AS，SE和BR元素的天体内部的各种天体物理现象。已经采用了相对论理论框架中的全阶扰动多体方法来确定原子波函数，该函数进一步用于用不确定性估算上述数量。我们发现我们的某些结果与较早可用的结果之间存在显着差异。
We present precise radiative data of line strengths, transition probabilities and oscillator strengths for the allowed transitions among the $nS_{1/2}$, $nP_{1/2,3/2}$, $n'D_{3/2,5/2}$ and $n'F_{5/2,7/2}$ states with $n=4$ to $6$ and $n'=4,5$ of the Cu-isoelectronic As, Se and Br ions. Due to unavailability of precise observations of these spectroscopic data, their accurate estimations are of great interest and useful in analyzing various astrophysical phenomena undergoing inside the heavenly bodies that contain As, Se and Br elements. An all-order perturbative many-body method in the relativistic theory framework has been employed to determine the atomic wave functions, which are further used to estimate the above quantities with the uncertainties. We found significant differences between some of our results and results that are available earlier.
