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Phys Rev E Stat Nonlin Soft Matter Phys. 2002 Nov;66(5):056402. doi: 10.1103/PhysRevE.66.056402. Epub 2002 Nov 11.

Charge-exchange-induced two-electron satellite transitions from autoionizing levels in dense plasmas.

Physical review. E, Statistical, nonlinear, and soft matter physics

F B Rosmej, H R Griem, R C Elton, V L Jacobs, J A Cobble, A Ya Faenov, T A Pikuz, M Geissel, D H H Hoffmann, W Süss, D B Uskov, V P Shevelko, R C Mancini

Affiliations

  1. GSI-Darmstadt, Plasmaphysik, Planckstrasse 1, D-64291 Darmstadt, Germany.

PMID: 12513602 DOI: 10.1103/PhysRevE.66.056402

Abstract

Order-of-magnitude anomalously high intensities for two-electron (dielectronic) satellite transitions, originating from the He-like 2s(2) 1S0 and Li-like 1s2s(2) (2)S(1/2) autoionizing states of silicon, have been observed in dense laser-produced plasmas at different laboratories. Spatially resolved, high-resolution spectra and plasma images show that these effects are correlated with an intense emission of the He-like 1s3p 1P-1s(2) 1S lines, as well as the K(alpha) lines. A time-dependent, collisional-radiative model, allowing for non-Maxwellian electron-energy distributions, has been developed for the determination of the relevant nonequilibrium level populations of the silicon ions, and a detailed analysis of the experimental data has been carried out. Taking into account electron density and temperature variations, plasma optical-depth effects, and hot-electron distributions, the spectral simulations are found to be not in agreement with the observations. We propose that highly stripped target ions (e.g., bare nuclei or H-like 1s ground-state ions) are transported into the dense, cold plasma (predominantly consisting of L- and M-shell ions) near the target surface and undergo single- and double-electron charge-transfer processes. The spectral simulations indicate that, in dense and optically thick plasmas, these charge-transfer processes may lead to an enhancement of the intensities of the two-electron transitions by up to a factor of 10 relative to those of the other emission lines, in agreement with the spectral observations.

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