# Single photoionization of the Kr-like Rb II ion in the photon energy   range 22 - 46.0 eV

**Authors:** Brendan M. McLaughlin, James F. Babb

arXiv: 1903.06032 · 2019-04-12

## TL;DR

This study measures and analyzes the photoionization cross sections of Kr-like Rb$^+$ ions across 22-46 eV, comparing experimental data with advanced theoretical calculations to identify resonance features and metastable state contributions.

## Contribution

It provides high-resolution experimental data and benchmarks large-scale Dirac Coulomb R-matrix theoretical calculations for Rb$^+$ photoionization, including resonance identification.

## Key findings

- Resonance features dominate 22-32 eV range.
- Fano window resonances observed above 32 eV.
- Theoretical calculations agree well with experimental data.

## Abstract

Single photoionization cross sections for Kr-like Rb$^+$ ions are reported in the energy (wavelength) range 22 eV (564 \AA) to 46 eV (270 \AA). Theoretical cross section calculations for this {\it trans}-Fe element are compared with measurements from the ASTRID radiation facility in Aarhus, Denmark and the dual laser plasma (DLP) technique, at respectively 40 meV and 35 meV FWHM energy resolution. In the photon energy region 22 - 32 eV the spectrum is dominated by excitation autoionizing resonance states. Above 32 eV the cross section exhibit classic Fano window resonances features, which are analysed and discussed. Large-scale theoretical photoionization cross-section calculations, performed using a Dirac Coulomb $R$-matrix approximation are bench marked against these high resolution experimental results. Comparison of the theoretical work with the experimental studies allowed the identification of resonance features and their parameters in the spectra in addition to contributions from excited metastable states of the Rb$^+$ ions.

## Full text

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## Figures

15 figures with captions in the complete paper: https://tomesphere.com/paper/1903.06032/full.md

## References

27 references — full list in the complete paper: https://tomesphere.com/paper/1903.06032/full.md

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Source: https://tomesphere.com/paper/1903.06032