Calculations of energy levels, radiative transition parameters, hyperfine structure constants <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si5.svg" display="inline" id="d1e5155"><mml:msub><mml:mrow><mml:mi>A</mml:mi></mml:mrow><mml:mrow><mml:mi>J</mml:mi></mml:mrow></mml:msub></mml:math> - <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si6.svg" display="inline" id="d1e5165"><mml:msub><mml:mrow><mml:mi>B</mml:mi></mml:mrow><mml:mrow><mml:mi>J</mml:mi></mml:mrow></mml:msub></mml:math>, Landé <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si7.svg" display="inline" id="d1e5175"><mml:msub><mml:mrow><mml:mi>g</mml:mi></mml:mrow><mml:mrow><mml:mi>J</mml:mi></mml:mrow></mml:msub></mml:math> factors and isotope shifts for Sc XX using the MCDF-RCI method-Reference-Cited by-同舟云学术

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Calculations of energy levels, radiative transition parameters, hyperfine structure constants AJ - BJ, Landé gJ factors and isotope shifts for Sc XX using the MCDF-RCI method

Published:2023-07 Issue: Volume:16 Page:100160
ISSN:2666-0326
Container-title:Physics Open
language:en
Short-container-title:Physics Open

Author:

Rathi Shikha^ORCID,Sharma Lalita^ORCID

Funder

Ministry of Education, India

Publisher

Elsevier BV

Subject

General Physics and Astronomy

Reference56 articles.

1. Inputting hyperfine structure into synthetic spectrum codes;Wahlgren;Mem. Della Soc. Astron. Ital. Suppl.,2005

2. Transition probabilities of Sc i and Sc ii and scandium abundances in the sun, arcturus, and HD 84937;Lawler;Astrophys. J. Suppl. Ser.,2019

3. Chemical composition of the solar surface;Prieto;J. Astrophys. Astron.,2020

4. Solar system abundances and condensation temperatures of the elements;Lodders;Astrophys. J.,2003

5. High-precision abundances of Sc, Mn, Cu, and Ba in solar twins-trends of element ratios with stellar age;Nissen;Astron. Astrophys.,2016

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