Answers are grounded in this paper and cite their sources.
Theoretical models are constructed of the hard x-ray spectra resulting from electron capture by fully stripped Ne¹⁰⁺ ions traversing the gases Ne, He, H₂, CO₂, and H₂O. The measured spectra are superpositions of individual lines of Ne⁹⁺. An exact description of the radiative cascade is used. Initial excited populations that reproduce the measured spectra are derived and quantitative predictions of the energies and intensities of lines in the soft x-ray and extreme ultraviolet regions are made. These lines when observed will be powerful diagnostic probes of the capture mechanism and of the diverse range of laboratory and astrophysical plasmas in which it occurs.
No takes yet. Share an insight, caveat, or question.
Rigazio et al. (2002) studied this question.
Synapse has enriched 10 related papers. Consider them for comparative context: