Spectral line shifts of H-like neon in hot and dense plasmas

zhang li; li xiang-dong

Volume 18 Issue 05

May 2006

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Article Navigation > High Power Laser and Particle Beams > 2006 > 18(05): 0-

cheng xinbing, zhang yu, zhang hongbo, et al. Theoretical analysis of discharge process of spiral Blumlein pulse forming line[J]. High Power Laser and Particle Beams, 2010, 22.

Citation:

zhang li, li xiang-dong. Spectral line shifts of H-like neon in hot and dense plasmas[J]. High Power Laser and Particle Beams, 2006, 18.

cheng xinbing, zhang yu, zhang hongbo, et al. Theoretical analysis of discharge process of spiral Blumlein pulse forming line[J]. High Power Laser and Particle Beams, 2010, 22.

Citation:

zhang li, li xiang-dong. Spectral line shifts of H-like neon in hot and dense plasmas[J]. High Power Laser and Particle Beams, 2006, 18.

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Spectral line shifts of H-like neon in hot and dense plasmas

zhang li^1,2,
li xiang-dong¹

1.
State Key Laboratory of High Field Laser Physics,Shanghai Institute of Optics and Fine Mechanics,P.O.Box 800-211,Chinese Academy of Sciences,Shanghai 201800,China;
2.
Graduate School of Chinese Academy of Sciences,Beijing 100049,China

Publish Date: 2006-05-15

Abstract

Abstract

By supposing the ion sphere model, the self-consistent field method between the Poisson-Boltzmann equation and the Dirac equation is used to calculate the energy levels of H-like neon immersed in hot and dense plasmas. Consequently, the effects of the plasma on the bound energy levels, and on the transitions between 1s and 2p electron configurations are studied. The results show that the spectral line shift increases with the increase of electron density, and decreases with the increase of electron temperature. The discrepancy of the fine spectral splitting decreases with the increase of electron density, and increases with the increase of electron temperature. All the variations will not only seriously affect the final spectrum simulations, but also make it possible to experimentally obse
- h-like ion plasma,
- spectral line shift,
- fine structure splitting,
- ion sphere model,

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