K-shell photoionization of Na-like to Cl-like ions of Mg, Si, S, Ar, and Ca
arXiv:1010.3734 · doi:10.1088/0067-0049/192/1/7
Abstract
We present -matrix calculations of photoabsorption and photoionization cross sections across the K-edge of Mg, Si, S, Ar, and Ca ions with more than 10 electrons. The calculations include the effects of radiative and Auger damping by means of an optical potential. The wave functions are constructed from single-electron orbital bases obtained using a Thomas--Fermi--Dirac statistical model potential. Configuration interaction is considered among all states up to . The damping processes affect the resonances converging to the K-thresholds causing them to display symmetric profiles of constant width that smear the otherwise sharp edge at the photoionization threshold. These data are important for modeling of features found in photoionized plasmas.
arXiv commentAccepted for publication in ApJS. 20 pages, 5 figures
References in corpus (11)
- Photoionization Modeling and the K Lines of Iron
- The Ionized Gas and Nuclear Environment in NGC 3783. I. Time-Averaged 900 ks Chandra Grating Spectroscopy
- Modeling of iron K lines: radiative and Auger decay data for Fe II-Fe IX
- K-shell Photoabsorption of Oxygen Ions
- Decay Properties of K-Vacancy States in Fe X-Fe XVII
- X-Ray Spectroscopy of the Low-Mass X-ray Binaries 2S 0918-549 and 4U1543-624: Evidence for Neon-Rich Degenerate Donors
- Chandra Grating Spectroscopy of the X-ray Binary 4U 1700-37 in a Flaring State
- Nitrogen K-shell photoabsorption
- K-shell photoionization of ground-state Li-like carbon ions [C]: experiment, theory and comparison with time-reversed photorecombination
- K-shell photoionization of ground-state Li-like boron ions [B]: Experiment and Theory
- K-Shell Photoabsorption Studies of the Carbon Isonuclear Sequence
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