Intensities and shifts of Lyman and Balmer lines of hydrogen-like ions in high density plasmas
The spectral line intensities and line shifts of Lyman and Balmer series for transitions up to n = 5 of hydrogen-like ion are studied in plasmas with densities and temperatures in the ranges ne ∼ 1018–1021 cm−3, Te = 0.3–1.2 eV respectively. The screened potential used to describe the interaction be...
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Series: | Matter and Radiation at Extremes |
Online Access: | http://dx.doi.org/10.1016/j.mre.2018.07.001 |
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doaj-54b8f3e6189c4e2fabc6c5bda2c7f8d52020-11-25T00:27:56ZengAIP Publishing LLCMatter and Radiation at Extremes2468-080X2018-11-013630031110.1016/j.mre.2018.07.001004806MREIntensities and shifts of Lyman and Balmer lines of hydrogen-like ions in high density plasmasG.P. Zhao0L. Liu1J.G. Wang2R.K. Janev3J. Yan4Institute of Applied Physics and Computational Mathematics, P. O. Box 8009-26, Beijing 100088, ChinaInstitute of Applied Physics and Computational Mathematics, P. O. Box 8009-26, Beijing 100088, ChinaInstitute of Applied Physics and Computational Mathematics, P. O. Box 8009-26, Beijing 100088, ChinaMacedonian Academy of Sciences and Arts, P. O. Box 428, 1000 Skopje, MacedoniaInstitute of Applied Physics and Computational Mathematics, P. O. Box 8009-26, Beijing 100088, ChinaThe spectral line intensities and line shifts of Lyman and Balmer series for transitions up to n = 5 of hydrogen-like ion are studied in plasmas with densities and temperatures in the ranges ne ∼ 1018–1021 cm−3, Te = 0.3–1.2 eV respectively. The screened potential used to describe the interaction between charged particles includes the electron exchange-correlation and finite-temperature gradient effects and is valid for both weakly and strongly coupled plasmas. The dependencies of alpha, beta and gamma line shifts of Lyman and Balmer series on plasma density (for fixed temperature) and temperature (for fixed density) are investigated. The results for the Hα line shifts are compared with the available high-density experimental data.http://dx.doi.org/10.1016/j.mre.2018.07.001 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
G.P. Zhao L. Liu J.G. Wang R.K. Janev J. Yan |
spellingShingle |
G.P. Zhao L. Liu J.G. Wang R.K. Janev J. Yan Intensities and shifts of Lyman and Balmer lines of hydrogen-like ions in high density plasmas Matter and Radiation at Extremes |
author_facet |
G.P. Zhao L. Liu J.G. Wang R.K. Janev J. Yan |
author_sort |
G.P. Zhao |
title |
Intensities and shifts of Lyman and Balmer lines of hydrogen-like ions in high density plasmas |
title_short |
Intensities and shifts of Lyman and Balmer lines of hydrogen-like ions in high density plasmas |
title_full |
Intensities and shifts of Lyman and Balmer lines of hydrogen-like ions in high density plasmas |
title_fullStr |
Intensities and shifts of Lyman and Balmer lines of hydrogen-like ions in high density plasmas |
title_full_unstemmed |
Intensities and shifts of Lyman and Balmer lines of hydrogen-like ions in high density plasmas |
title_sort |
intensities and shifts of lyman and balmer lines of hydrogen-like ions in high density plasmas |
publisher |
AIP Publishing LLC |
series |
Matter and Radiation at Extremes |
issn |
2468-080X |
publishDate |
2018-11-01 |
description |
The spectral line intensities and line shifts of Lyman and Balmer series for transitions up to n = 5 of hydrogen-like ion are studied in plasmas with densities and temperatures in the ranges ne ∼ 1018–1021 cm−3, Te = 0.3–1.2 eV respectively. The screened potential used to describe the interaction between charged particles includes the electron exchange-correlation and finite-temperature gradient effects and is valid for both weakly and strongly coupled plasmas. The dependencies of alpha, beta and gamma line shifts of Lyman and Balmer series on plasma density (for fixed temperature) and temperature (for fixed density) are investigated. The results for the Hα line shifts are compared with the available high-density experimental data. |
url |
http://dx.doi.org/10.1016/j.mre.2018.07.001 |
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1725337636924555264 |