Sonja Bernitt

X-ray and extreme-ultraviolet spectra from collisions of Ar$^{18+}$ and O$^{8+}$ ions with neutrals

Stepan Dobrodey [1], Chintan Shah [1,2,3], Sonja Bernitt [1,4], Ming Feng Gu [6], Liyi Gu [7], Thomas Pfeifer [1], José R. Crespo López-Urrutia

Abstract

We present measurements of K-shell x-ray emission following charge exchange of fully ionized argon with various neutral gaseous targets at small collision energies inside an electron beam ion trap. We also resolve the principal quantum number of electron capture in extreme-ultraviolet spectra from initially bare and hydrogen-like oxygen ions held in the same trap. We analyze discrepancies between these as well as previous measurements with theoretical models based on the multichannel Landau-Zener approach.

High-Precision Transition Energy Measurements of Neon-like Fe XVII Ions

Chintan Shah [1,2,3], Moto Togawa [2,4,5], Marc Botz [2,5], Jonas Danisch [2], Joschka J. Goes [2], Sonja Bernitt [6,7,8,2], Marleen Maxton [2,9,10], Kai Köbnick, Jen Buck, Jörn Seltmann, Moritz Hoesch [10], Ming Feng Gu [11], F. Scott Porter [1], Thomas Pfeifer [2], Maurice A. Leutenegger [1], Charles Cheung [12], Marianna S. Safronova [12,2], José R. Crespo López-Urrutia

Abstract

We improve by a factor of 4-20 the energy accuracy of the strongest soft X-ray transitions of Fe XVII ions by resonantly exciting them in an electron beam ion trap with a monochromatic beam at the P04 beamline of the PETRA III synchrotron facility. By simultaneously tracking instantaneous photon-energy fluctuations with a high-resolution photoelectron spectrometer, we minimize systematic uncertainties down to 10-15 meV, or velocity equivalent $\pm\sim$5 km s$^{-1}$ in their rest energies, substantially improving our knowledge of this key astrophysical ion. Our large-scale configuration-interaction computations include more than four million relativistic configurations and agree with the experiment at a level without precedent for a 10-electron system. Thereby, theoretical uncertainties for interelectronic correlations become far smaller than those of quantum electrodynamics (QED) corrections. The present QED benchmark strengthens our trust in future calculations of many other complex atomic ions of interest to astrophysics, plasma physics, and for the development of optical clocks with highly charged ions.