Data Descriptor
Version 1
Preserved in Portico This version is not peer-reviewed
Data on Stark Broadening of N VI Spectral Lines
Version 1
: Received: 21 March 2024 / Approved: 22 March 2024 / Online: 22 March 2024 (11:45:43 CET)
A peer-reviewed article of this Preprint also exists.
Dimitrijević, M.S.; Christova, M.D.; Sahal-Bréchot, S. Data on Stark Broadening of N VI Spectral Lines. Data 2024, 9, 77. Dimitrijević, M.S.; Christova, M.D.; Sahal-Bréchot, S. Data on Stark Broadening of N VI Spectral Lines. Data 2024, 9, 77.
Abstract
Data on Stark broadening parameters, spectral line widths and shifts, for 15 multiplets of N VI, which 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. These data are particularly of interest for the analysis and modelling of atmospheres of hot and dense stars, as e.g. white dwarfs, and for investigation of their spectra, but also for analyis ad modelling of laser driven plasma in proton-boron fusion research.
Keywords
atomic data; Stark broadening; N VI; proton-boron fusion; line profiles; atomic processes; stellar atmospheres
Subject
Physical Sciences, Atomic and Molecular Physics
Copyright: This is an open access article distributed under the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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