scholarly journals Collision strengths and effective collision strengths for Ne-like Ge

2017 ◽  
Vol 95 (11) ◽  
pp. 1161-1179
Author(s):  
Wessameldin S. Abdelaziz

We have carried out a calculation of 241 levels for Ne-like Ge (Z = 36) to calculate electron impact collision strengths and effective collision strengths belonging to 1s22s22p5nl, 1s22s12p6nl (n = 3, 4, 5, 6; l = s, p, d, f, g, and h) configurations, which have been calculated by the fully relativistic flexible atomic code (FAC). Our calculations, based on the distorted-wave method with large configuration interactions, are included. Collision strengths have been generated over an electron energy range of (10–20 000 eV) and they have been listed at seven representative energies of 65.33, 1714.98, 2944.1, 4868.3, 7564.6, 11 040, and 15 221 eV in this work, and effective collision strengths data have been calculated from these at electron plasma temperatures 650, 850, 1050, 1250, 1450, 1650, and 1850 eV. Our results are compared with those available in the literature. It is found that the resonance effects are important in calculating the effective collision strengths.

Cross-sections for excitation of the 2 3 P state of helium from the ground state have been calculated by the distorted-wave method. The polarization of radiation emitted as a result of the excitation is also calculated. Comparison is made with the corresponding results given by the Born—Oppenheimer approximation. Although there are considerable differences at electron energies below 100 eV these are much less marked than for the excitation of the 2 3 S state. The distorted wave method gives cross-sections in closer agreement with observation but substantial discrepancies still remain. It is difficult, however, to estimate their magnitude with any certainty because there are inconsistencies in the observed data.


2014 ◽  
Vol 89 (5) ◽  
Author(s):  
Song bin Zhang ◽  
Xing Yu Li ◽  
Jian Guo Wang ◽  
Yi Zhi Qu ◽  
Xiangjun Chen

2005 ◽  
Vol 72 (1) ◽  
Author(s):  
M. S. Pindzola ◽  
F. Robicheaux ◽  
J. A. Ludlow ◽  
J. Colgan ◽  
D. C. Griffin

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