Abstract
Using semiclassical perturbation approach in impact approximation, Stark shifts for singly charged argon (Ar II) spectral lines have been calculated. Energy levels and oscillator strengths needed for this calculation were determined using Hartree–Fock method with relativistic correction (HFR). We compare our results with experimental values for 100 spectral lines. We also present results as a function of temperature for 161 spectral lines for collisions with electrons, protons, singly charged helium and singly charged argon. This work extends our previous one.
Author supplied keywords
Cite
CITATION STYLE
Hamdi, R., Ben Nessib, N., Sahal-Bréchot, S., & Dimitrijević, M. S. (2019). Semiclassical perturbation Stark shifts of singly charged argon spectral lines. Monthly Notices of the Royal Astronomical Society, 488(2), 2473–2479. https://doi.org/10.1093/mnras/stz1835
Register to see more suggestions
Mendeley helps you to discover research relevant for your work.