A new published paper from a STSM of CA21128-PROBONO, by Milan S. Dimitrijević, Magdalena D. Christova and Sylvie Sahal-Bréchot in Data  2024, 9(6):77

Keywords: atomic data; Stark broadening; N VI; proton–boron fusion, line profiles; atomic processes; stellar atmospheres

Data on Stark Broadening of N VI Spectral Lines

Milan S. Dimitrijević, Magdalena D. Christova and Sylvie Sahal-Bréchot

Data 2024, 9(6), 77

https://doi.org/10.3390/data9060077

 

Abstract: Data on Stark broadening parameters, spectral line widths, and shifts for 15 multiplets of N VI, whose spectral lines are broadened by collisions with electrons, protons, alpha particles (He III) and B III, B IV, B V and B VI ions, are presented. They have been calculated using the semiclassical perturbation theory, for temperatures from 50,000 K to 2,000,000 K, and perturber densities from 1016 cm−3 up to 1024 cm−3. The data for e, p and He III are of particular interest for the analysis and modelling of atmospheres of hot and dense stars, as, e.g., white dwarfs, and for investigation of their spectra, and data for boron ions are used for analysis and modelling of laser-driven plasma in proton–boron fusion research.

Cite:
Dimitrijević MS, Christova MD, Sahal-Bréchot S. Data on Stark Broadening of N VI Spectral Lines. Data. 2024; 9(6):77. https://doi.org/10.3390/data9060077 


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