Quantum mechanical line widths of ionized oxygen, silicon, and aluminium; comparisons with recent experimental results

Author:

Elabidi H1ORCID,Sahal-Bréchot S2ORCID,Dimitrijević M S23ORCID,Hamdi R4ORCID,Belhadj W1ORCID

Affiliation:

1. Physics Department, College of Applied Science, Umm Al-Qura University , Makkah Almukarramah, Saudi Arabia

2. LERMA, Observatoire de Paris, PSL University, CNRS, Sorbonne Université , France

3. Astronomical Observatory , Volgina 7, 11060 Belgrade, Serbia

4. College of Al-Qunfudah Health Sciences, Umm Al-Qura University , Makkah Almukarramah, Saudi Arabia

Abstract

ABSTRACT We present in this paper new quantum Half Widths at Half intensity Maximum (HWHM) for 101 spectral lines of the following ions: O II (35 lines), O III (20 lines), Si II (9 lines), Si III (12 lines), and Al III (25 lines). The present quantum results are compared to new experimental ones. No previous quantum calculations have been performed for these ions. The relatively high differences found between the new and previous measurements and the available theoretical calculations encourage us to conduct these quantum calculations. Our quantum method has been used many years ago and has given good results compared to other approaches, so it can be a useful tool to check the new experimental results or to understand the disagreement found for some lines. Furthermore, the obtained results can be used for the abundance determination of elements, the calculation of stellar opacity, the interpretation and modelling of stellar spectra, and the estimation of the relative transfer through stellar plasmas, etc. Part of the present results will be also implemented to the data base of Stark broadening parameters STARK-B.

Funder

Ministry of Education

CNRS

CEA

CNES

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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