Data on Stark Broadening of N VI Spectral Lines

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 per...

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Bibliographic Details
Published in:Data (Basel) 2024-06, Vol.9 (6), p.77
Main Authors: Dimitrijevic, Milan S, Christova, Magdalena D, Sahal-Bréchot, Sylvie
Format: Article
Language:English
Subjects:
Alpha particles
Alpha rays
Approximation
Astrophysics
atomic data
atomic processes
Boron
Datasets
Fine structure
Laser-plasma interactions
Lasers
line profiles
Line spectra
Modelling
N VI
Nuclear fusion
Perturbation theory
Plasma
Protons
proton–boron fusion
Spectra (Spectroscopy)
Spectral linewidth
Spectrum analysis
Stark broadening
White dwarf stars
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Summary: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 10[sup.16] cm[sup.−3] up to 10[sup.24] cm[sup.−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. Dataset: The dataset is submitted as a Supplementary File. Dataset License: CC-BY 4.0
ISSN:2306-5729
2306-5729
DOI:10.3390/data9060077