Stark Broadening of the Spectral Lines of Ne V

International audienceUsing a semiclassical approach, we have calculated ab initio electron-, proton-, and ionized helium-impact line widths and shift for 26 Ne V multiplets. Energy levels and oscillator strengths have been calculated using SUPERSTRUCTURE code. Results have been presented for an electron density of 1017 cm-3 as a function of temperature, and are compared with experimental and other theoretical results