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

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