- Open Access
Precise energy determination of Ni and Fe in high ionization states using a microcalorimeter
Phys. Rev. A 114, 052808 – Published 9 November, 2026
DOI: https://doi.org/10.1103/ynpq-nhq6
Abstract
Accurate laboratory transition energies for the Ni blend are urgently needed both for atomic-structure benchmarking and interpretation of astrophysical x-ray spectra observed with space telescopes. Crucially, inferred abundances of these elements, which are essential for the diagnostics of hot plasmas, depend on the treatment of those overlapping transitions. By combining a transition-edge-sensor x-ray microcalorimeter array and a superconducting electron beam ion trap, we distinguish with line widths between and the key transitions from Ni xx to Ni xxvii, including previously unmeasured ones, from the lines of Fe xx to Fe xxv. Collisional-radiative calculations using the Flexible Atomic Code agree well with our results. By calibrating all sensors individually and correcting for their temporal drifts we achieve an average uncertainty below for their transition energies, easing the interpretation of astrophysical spectra. Furthermore, our charge-state-resolved results benchmark theory for complex open-shell ions in the intermediate coupling regime, for which we compare the results from pure configuration interaction and calculations including many-body perturbation theory (MBPT) and find a significant improvement when including MBPT.
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