CAOSP abstracts, Volume: 53, No.: 3, year: 2023

Author(s): Christova, M.D.; Dimitrijević, M.S.; Sahal-Bréchot, S.
Journal: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 53, no. 3, p. 84-93.
Date: 12/2023
Title: On the Stark broadening of N VI spectral lines
Keyword(s): Stark broadening, spectral line shapes, atomic data, N VI, proton-boron fusion
Pages: 84 -- 93
DOI: https://doi.org/10.31577/caosp.2023.53.3.84
NASA ADS Abstract Service: 2023CoSka..53c..84C
Citation:
License: This work is licensed under a Creative Commons Attribution 4.0 International License

Abstract: Results for the Stark broadening parameters for spectral lines within one spectral series of N VI 2s-np (n = 2 -- 4) triplet transitions are included. Plasma conditions of interest cover temperatures from 50 000 K to 2 000 000 K, perturber density is 10¹⁷ cm^-3, and electrons, and boron ions (B III, B IV, B V and B VI) are perturbers. These conditions correspond to those in laser driven plasma for proton boron fusion reaction. The contribution in Stark width and shift of different types of perturbers is analyzed. The width versus principal quantum number is presented.