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Radiative rates and electron-impact excitation for the n ≤ 6 fine-structure levels in H-like ions with 13 ≤ Z ≤ 42

机译:H≤13≤42的H型离子中n≤6精细结构能级的辐射速率和电子碰撞激发

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Context. Many observed emission lines from space missions are due to highly charged H-like ions. An analysis of the lines provides information on the temperature, density, and chemical composition of plasmas. A wide range of atomic parameters, such as energy levels, radiative rates, and excitation rate coefficients are needed to achieve this goal. Aims. In this paper we report on calculations for energy levels, radiative rates, collision strengths, and effective collision strengths for transitions among the 36 lowest levels of the n ≤ 6 configurations of highly charged H-like ions with 13 ≤ Z ≤ 42. Methods. The widely used Flexible Atomic Code (FAC) is adopted for the calculation. Energy levels and radiative rates are calculated within the relativistic configuration-interaction method. Employing relativistic distorted-wave approximation, direct excitation collision strengths are calculated at eleven scattered electron energies E′f = 0.001, 0.002, 0.005, 0.01, 0.02, 0.05, 0.1, 0.2, 0.5, 1.0, and 2.5, where E′f is in units of Z2 rydbergs. Collision strengths at higher energies are estimated by interpolation/extrapolation using relativistic Bethe form. Resonance contributions through the relevant He-like doubly excited n′l′n′′l′′ configurations with n′ ≤ 7 and n′′ ≤ 75 are explicitly taken into account using the independent-process isolated-resonance approximation. Radiation damping effects are taken into account. Results. We present the radiative rates, oscillator strengths, and line strengths for all electric dipole (E1), magnetic dipole (M1), electric quadrupole (E2), magnetic quadrupole (M2), electric octupole (E3), and magnetic octupole (M3) transitions. Assuming a Maxwellian electron velocity distribution, we report effective collision strengths over a wide temperature range between 2 × 103 × Z2 and 2 × 106 × Z2 K. We believe that the present results are the most extensive and definitive atomic dataset to date for highly charged H-like ions.
机译:上下文。从太空任务观察到的许多发射线是由于高电荷的类H离子引起的。管线分析提供了有关温度,密度和等离子体化学成分的信息。为了实现这一目标,需要广泛的原子参数,例如能级,辐射速率和激发速率系数。目的在本文中,我们报告了在n≤6构型的13≤Z≤42的n≤6构型的36个最低水平之间跃迁的能级,辐射速率,碰撞强度和有效碰撞强度的计算方法。方法。计算采用了广泛使用的弹性原子码(FAC)。相对论构型-相互作用法计算能级和辐射率。采用相对论的畸变波近似法,在11个散射电子能量E'f = 0.001、0.002、0.005、0.01、0.02、0.05、0.1、0.2、0.5、1.0和2.5的情况下计算直接激发碰撞强度,其中E'f为以Z2雷德伯格为单位。使用相对论的贝特形式通过内插/外推法估算高能下的碰撞强度。通过使用独立过程隔离共振近似,明确考虑了通过相关的He类双激发n'l'n''l''配置(n'≤7和n''≤75)产生的共振贡献。考虑了辐射衰减效应。结果。我们给出了所有电偶极(E1),磁偶极(M1),电四极(E2),磁四极(M2),电八极(E3)和磁八极(M3)的辐射速率,振荡器强度和线强度过渡。假设麦克斯韦电子速度分布,我们报告了在2×103×Z2和2×106×Z2 K的较宽温度范围内的有效碰撞强度。我们相信,对于高电荷的原子,当前结果是迄今为止最广泛和确定的类氢离子。

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