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Quantum and Semiclassical Stark Widths for Ar VII Spectral Lines

DOI: https://doi.org/10.3390/atoms6020020

Keywords: Stark broadening, Ar VII line profiles, stars, white dwarfs, atomic data, scattering

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Abstract:

Abstract We present in this paper the results of a theoretical study of electron impact broadening for several lines of the Ar VII ion. The results have been obtained using our quantum mechanical method and the semiclassical perturbation one. Results are presented for electron density 10 18 cm ?3 and for electron temperatures ranging from 2 × 10 4 to 5 × 10 5 K required for plasma modeling. Our results have been compared to other semiclassical ones obtained using different sources of atomic data. A study of the strong collisions contributions to line broadening has been performed. The atomic structure and collision data used for the calculations of line broadening are also calculated by our codes and compared to available theoretical results. The agreement found between the two calculations ensures that our line broadening procedure uses adequate structure and collision data. View Full-Tex

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