类镍钨离子共振激发速率系数

本文利用基于相对论组态混合的扭曲波近似方法,细致研究了类镍钨离子从基态到3l-14l'(l=s,p,d;l'=0-3)各组态共106条单激发态能级,通过类铜双激发态3l174l'n"l"和3l175l'n"l"的电子碰撞共振激发速率系数.本工作的结果与R矩阵计算值相比较存在较大差别.     

钨离子双电子复合过程的理论研究

利用全相对论组态相互作用理论方法, 研究了W28+离子由基态俘获一个电子形成双激发态(3d104s24p64d10 )-1 nln'l'(n = 4~6, n' = 4~15)的双电子复合(DR)过程. 比较分析了3s、3p、3d、4s、4p和4d电子激发对DR速率系数的贡献, 分析了3d、4s、4p和4d电子激发的DR速率系数随轨道量子数l' 的变化. 考虑和已有的计算完全相同的初态, 中间双激发态以及辐射和俄歇末态的情况下, 得到了和已有的计算符合很好的结果. 在综合了分析得到的对W28+离子DR过程有明显贡献的各种因素后,进一步得到了总DR速率系数. 其中, 考虑DAC效应对总DR速率系数有不可忽略的影响. 对DR速率系数进行了参数拟合, 拟合值与计算值的偏差小于1％.     

Co-like Au52+离子双电子复合的理论研究

基于准相对论Hatree-Fock理论,采用Cowan程序详细计算了Co-like A u52+离子的双电子复合速率系数、自电离几率以及自电离能级.计算结果表明:由于径向波函数的穿透效应使得该离子自电离能级3d84l5s(l=s、 p、d、f)升高,造成能级间隔不随外层激发电子轨道角动量的增加单调减小的异常现象,即Δ(E3d8 4l5d-E3d84l5p)＞Δ(E3d84l5p-E3d84l5s)＞Δ(E 3d84l5f-E3d84l5d);双激发自电离态平均自电离几率具有特定的变化关系;双电子复合速率系数随着电子温度逐渐增加具有共振、高温收敛等特点,且双激发态轨道角动量大且宇称为奇的通道复合速率系数较大,其中辐射衰变通道为3d84fnd-3d9nd 的复合过程占优势,在Te=0.49*"KeV时共振峰αDR=1.01×10-11(cm 3sec-1).     

类镍钨离子共振激发速率系数

本文利用基于相对论组态混合的扭曲波近似方法，细致研究了类镍钨离子从基态到3l^-14l＇（l=s，p，d；l’=0—3）各组态共106条单激发态能级，通过类铜双激发态3l^174l’n＇l＂和3l^175l’n＂l＂的电子碰撞共振激发速率系数．本工作的结果与R矩阵计算值相比较存在较大差别，     

W~(28+)离子双电子复合速率系数的理论研究

利用全相对论组态相互作用理论方法,研究了W~(28+)离子由基态俘获一个电子形成双激发态(3d~(10)4s~24p~64d~(10))~(-1)nln'l'(n=4~6,n'=4~15)的双电子复合(DR)过程.比较分析了3s、3p、3d、4s、4p和4d电子激发对DR速率系数的贡献,分析了3d、4s、4p和4d电子激发的DR速率系数随轨道量子数l'的变化.考虑和已有的计算完全相同的初态,中间双激发态以及辐射和俄歇末态的情况下,得到了和已有的计算符合很好的结果 .在综合了分析得到的对W~(28+)离子DR过程有明显贡献的各种因素后,进一步得到了总DR速率系数.其中,考虑DAC效应对总DR速率系数有不可忽略的影响.对DR速率系数进行了参数拟合,拟合值与计算值的偏差小于1%.     

钨离子双电子复合过程的理论研究

摘要: 利用全相对论组态相互作用理论方法, 研究了W28+离子由基态俘获一个电子形成双激发态(3d104s24p64d10 )-1 nln''l''(n = 4~6, n'' = 4~15)的双电子复合(DR)过程. 比较分析了3s、3p、3d、4s、4p和4d电子激发对DR速率系数的贡献, 分析了3d、4s、4p和4d电子激发的DR速率系数随轨道量子数l'' 的变化. 考虑和已有的计算完全相同的初态, 中间双激发态以及辐射和俄歇末态的情况下, 得到了和已有的计算符合很好的结果. 在综合了分析得到的对W28+离子DR过程有明显贡献的各种因素后,进一步得到了总DR速率系数. 其中, 考虑DAC效应对总DR速率系数有不可忽略的影响. 对DR速率系数进行了参数拟合, 拟合值与计算值的偏差小于1％.     

电子与类铍N3+和O4+离子碰撞激发截面的相对论扭曲波计算

采用全相对论扭曲波方法,系统地计算了类铍N3+和 O4+离子从基态到2s2p和2p2 的各激发态以及从亚稳态到2p2各激发态的电子碰撞激发截面,详细地讨论了靶态的关联效应对激发截面的影响.结果表明:对于2s-2p的单电子激发,在低能碰撞时,靶态的电子关联效应起非常重要的作用,且使得激发截面降低;而高能碰撞时,靶态波函数的描述对连续态波函数的影响比较小,对激发截面影响也比较小.对于2s2-2p2的双电子激发,其中基态2s2 1 S0到J=0的2p2 3 P0,1S0的激发截面较大,其主要原因是末离子态波函数与基组态波函数的混合,但是其他几个激发的激发截面较小.     

基态类Ne锗离子双电子复合的半相对论计算

采用半相对论多组态Ｈａｒｔｒｅｅ一Ｆｏｃｋ模型，计算了类Ｎｅ锗离子经过３ｌ３ｌ＇和４ｌ４ｌ＇双激发态到类Ｎａ离子单激发态的态对态双电子复合速率系数，同时给出了描写上述复合过程的参数Ｂ和。通过对求和而获得的部分双电子复合速率系数与其它理论计算结果进行了比较。     

类铷W37+离子双电子复合速率系数的理论研究

 利用全相对论组态相互作用理论方法,研究了类铷W³⁷⁺离子从基组态3s²3p⁶3d¹⁰4s²4p⁶4d经过双激发态(3s²3p⁶3d¹⁰4s²4p⁶4d)^-1nln′l′(n,n′=4,5)的双电子复合过程,得到了该离子在温度为1~5×10⁴ eV范围内的总双电子复合速率系数。分析比较了不同电子激发的双电子复合速率系数,结果表明:4p电子激发的双电子复合速率系数在低温时给出了主要贡献,而3d的贡献在高温时突出。由于强组态相互作用,两电子一光子跃迁对双电子复合速率系数的贡献不可忽略,其中辐射跃迁4p⁵4d5d5f-4p⁶4f5d的贡献是双激发态4p⁵4d5d5f总的双电子复合速率系数的5%。对双电子复合、辐射复合以及三体复合速率系数的比较表明,在所研究的温度范围内双电子复合速率系数最大。     

类硼氧离子基态双电子复合速率系数的研究

由于氧广泛存在于星际物质中,对氧等离子体的诊断十分重要。双电子复合速率系数是对等离子体平衡状态诊断的重要参数。本文采用全相对论Flexible atomic code(FAC)研究了类硼氧离子从基态2s22p1(J=1/2)俘获电子,经过2s12p2 n′l′双激发态通道的双电子复合速率系数。忽略贡献很小的辐射级联效应,考虑组态相关,细致计算了n′≤9,l′≤n′-1的所有组态。使用了n′-3标度规律采用组态-组态外推法计算,计算了n′≤1000的所有组态总双电子复合速率系数。分析了双电子复合速率系数与不同被俘获轨道主量子数n′和轨道量子数l′的关系,认为对双电子复合其主要贡献的是n′=3和n′=5,且DR系数在l′=2时出现峰值。即基态通过2s2p2 n′l′的双电子复合伴线光谱中最强的光谱线对应跃迁为2s2p23d的双电子复合过程。该通道总的DR系数随温度升高而先增后减,在0.5eV左右出现最大值,认为此温度下双电子复合效率最高。低温时对于n′较大的组态可以忽略,高温时则需要考虑。     

Transfer of a weakly bound electron in collisions of Rydberg atoms with neutral particles. II. Ion-pair formation and resonant quenching of the Rb(nl) and Ne(nl) States by Ca, Sr, and Ba atoms

Electron-transfer processes are studied in thermal collisions of Rydberg atoms with alkaline-earth Ca(4s ²), Sr(5s ²), and Ba(6s ²) atoms capable of forming negative ions with a weakly bound outermost p-electron. We consider the ion-pair formation and resonant quenching of highly excited atomic states caused by transitions between Rydberg covalent and ionic terms of a quasi-molecule produced in collisions of particles. The contributions of these reaction channels to the total depopulation cross section of Rydberg states of Rb(nl) and Ne(nl) atoms as functions of the principal quantum number n are compared for selectively excited nl-levels with l ? n and for states with large orbital quantum numbers l = n ? 1, n ? 2. It is shown that the contribution from resonant quenching dominates at small values of n, and the ion-pair formation process begins to dominate with increasing n. The values and positions of the maxima of cross sections for both processes strongly depend on the electron affinity of an alkaline-earth atom and on the orbital angular momentum l of a highly excited atom. It is shown that in the case of Rydberg atoms in states with large l ～ n ? 1, the rate constants of ion-pair formation and collisional quenching are considerably lower than those for nl-levels with l ? n.     

锂原子光电离过程中的弛豫效应

利用基于多组态Dirac-Fock方法的程序包GRASP92和RATIP以及在此基础上最新发展的RERR06程序,计算了锂原子1s²nl(n=2,3; l=s, p) 的内壳层和外壳层的光电离截面. 计算中详细考虑了光电离过程中的弛豫效应. 结果表明：在锂原子内壳层电子的光电离过程中弛豫效应较强,而在外壳层电子的光电离过程中弛豫效应较弱. 另外,相应于不同态的内壳层光电离过程,其弛豫效应的影响也不同,对激发态的影响比对基态的影响大,对高激发态 关键词： 多组态Dirac-Fock方法 光电离截面 弛豫效应     

高离化态类镍离子电子碰撞激发过程的相对论扭曲波理论研究

利用相对论扭曲波方法和新发展的研究电子碰撞激发过程的计算程序REIE06,系统计算了电子碰撞激发高离化态类镍Gd³⁶⁺和Rn⁵⁸⁺—U⁶⁴⁺(Z=86—92)离子从基态到4l(l=s,p,d,f)次壳层精细结构能级的碰撞强度和截面.研究了随等电子系列变化时,从基态到与X射线激光有关的3d⁹4p和3d⁹4d激发态能级的电子碰撞激发截面随Z的变化,讨论了强的组态相互作用对高离化态类镍离子截面的影响.通过对Gd³⁶⁺离子涉及X射线激光跃迁的相关能级电子碰撞激发速率系数的计算,分析了等离子体中电子温度对碰撞过程的影响.同时,目前部分计算结果与以往的理论结果进行了比较,得到了很好的一致性. 关键词： 电子碰撞激发 相对论扭曲波方法 高离化态类镍离子     

Calculation of dielectronic recombination cross sections and rate coefficients for heliumlike carbon

A simplified relativistic configuration interaction method is used to calculate the dielectronic recombination cross sections and rate coefficients for heliumlike carbon. In this method, the infinite resonant doubly excited states can be treated conveniently in the frame of Quantum Defect Theory. Our calculated cross sections are in agreements with the experimental measurements except for the 1s2lnl'(n=6,7) resonances. The total energy-integrated cross sections and rate coefficients over all dielectronic resonances are in agreements with the experimental measurements within percent. Received: 7 July 1997 / Revised: 7 October 1997 / Accepted: 8 December 1997     

Resonance excitation process for Ni-like gold

A detailed and large-scale calculation on the resonant excitation rate coefficients from the ground state to the 106 fine-structure levels belonging to 3l¹⁷4l^′(l=0,1,2;l^′=0,1,2,3) configurations of Ni-like gold have been performed using the relativistic distorted-wave approximation. The contributions through all possible Cu-like doubly excited states 3l¹⁷4l^′n^″l^″and 3l¹⁷5l^′n^″l^″(n^″≤15,l^″≤8) are calculated explicitly. The radiative damping effects on resonant excitation rates are studied. Significant effects arising from decays to autoionizing levels are also investigated. The n⁻³scaling law is investigated and is used to obtain the contributions from high-n configurations. Contributions from resonant excitation are found to be as important as direct excitation processes for most transitions. In some cases, resonant excitation can enhance the excitation rate coefficients by an order of magnitude. In addition, the total dielectronic recombination rate coefficients of Ni-like gold are also presented and compared with other works.     

Multielectron ionization of atoms by fast ions: An approximation by normalized exponentials

Multielectron ionization of neutral atoms by fast positive ions is considered in terms of the independent particle model. A relatively simple technique for calculating the multielectron ionization probabilities and cross sections through the impact parameter is suggested in which one-electron ionization probabilities are represented as normalized exponentials p _nl(b) = p _nl(b) = p _nl(0)exp(?α_nl b), where b is the impact parameter and n and l are quantum numbers of the target atomic shell. Exponent α_nl is determined from the Born one-electron ionization cross section for target atoms, and preexponential p _nl(0) (the ionization probability at a zero impact parameter) is found from a geometrical model. This technique provides the normalization condition p _nl(b) ≤ 1 irrespective of the velocity and charge of striking ions and makes it possible to calculate the one-, two-, and three-electron ionization cross sections, which, when added up, make a major contribution to the total cross section, up to a factor of 2. The results of our computations are compared with experimental data and analytical results of other authors.     

Breit相互作用对类氦离子亚稳态1s2s 3S1电子碰撞激发截面的影响

利用新近发展的基于全相对论扭曲波方法研究电子-离子碰撞激发过程的计算程序,通过对Breit相互作用的考虑,计算了类氦等电子序列离子从亚稳态1s2s³S₁激发2s电子到n=2,3壳层的电子碰撞激发截面;研究了不同入射电子能量时Breit相互作用对碰撞激发截面的影响,进一步总结了沿等电子序列变化时,Breit相互作用对截面影响的一般规律.部分计算结果与实验结果进行了比较,得到了很好的一致性. 关键词： 全相对论扭曲波方法 Breit相互作用 电子碰撞激发截面     

Energy Levels of Doubly Excited States in Argon

Term energies of doubly excited states in argon and argon ions have been determined using single-configuration Hartree-Fock calculation. The energies calculated for KL3s3p⁶nl and KL3s⁶3p⁴nln1 states of Ar show a fairly good agreement with the experimental results obtained by various techniques. However, for Ar+, Ar²+, Ar²+ and Ar³+ states there are no experimental data available in the literature for comparison.     

Angular distributions of scattered excited muonic hydrogen atoms

Coulomb deexcitation differential cross sections of excited muonic hydrogen in collisions with the hydrogen atom are studied for the first time. In the fully quantum-mechanical close-coupling approach, both the differential cross sections for the nl → n′l′ transitions and l-averaged differential cross sections have been calculated for the initial exotic atom states with n = 2–6 at kinetic energies of E _cm = 0.01–15 eV and for scattering angles of ϑ_cm = 0°–180°. The vacuum polarization shifts of the ns states are taken into account. The differential cross sections of the elastic and Stark scattering obtained in the same approach are also presented. The main features of the calculated differential cross sections are discussed, and a strong anisotropy of Coulomb deexcitation cross sections is predicted. The text was submitted by the authors in English.     

Resonant electron impact excitation of highly charged Fe ions studied with a compact electron beam ion trap

We present extreme ultraviolet spectra of 3s3p–3s3d transitions in Fe¹⁴⁺ observed with a compact electron beam ion trap. The contributions of indirect excitation via a metastable state and resonant excitation are studied by observing the electron energy dependence of the spectra for the energy range of 60–210 eV. The results indicate that the 3s3d ¹D₂ level is directly excited from the 3s² ground state whereas the 3s3d ³D₃ level has a large contribution of the indirect excitation via the 3s3p ³P₂ metastable state. Comparisons with the theoretical excitation cross sections including MNn resonant excitations show good qualitative agreement with the experimental results for the electron energy dependent features.