Observation of strong two-electron-one-photon transitions in few-electron ions

M. Togawa, S. Kühn, C. Shah, P. Amaro, R. Steinbrügge, J. Stierhof, N. Hell, M. Rosner, K. Fujii, M. Bissinger, R. Ballhausen, M. Hoesch, J. Seltmann, S. Park, F. Grilo, F. S. Porter, J. P. Santos, M. Chung, T. Stöhlker, J. WilmsT. Pfeifer, G. V. Brown, M. A. Leutenegger, S. Bernitt, J. R. Crespo López-Urrutia

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7 Scopus citations

Abstract

We resonantly excite the K series of O5+ and O6+ up to principal quantum number n=11 with monochromatic x rays, producing K-shell holes, and observe their relaxation by soft-x-ray emission. Some photoabsorption resonances of O5+ reveal strong two-electron-one-photon (TEOP) transitions. We find that for the [(1s2s)15p3/2]3/2;1/2 states, TEOP relaxation is by far stronger than the radiative decay and competes with the usually much faster Auger decay path. This enhanced TEOP decay arises from a strong correlation with the near-degenerate upper states [(1s2p3/2)14s]3/2;1/2 of a Li-like satellite blend of the He-like Kα transition. Even in three-electron systems, TEOP transitions can play a dominant role, and the present results should guide further research on the ubiquitous and abundant many-electron ions where electronic energy degeneracies are far more common and configuration mixing is stronger.

Original languageEnglish
Article number053109
JournalPhysical Review A
Volume102
Issue number5
DOIs
StatePublished - Nov 25 2020
Externally publishedYes

Funding

Financial support was provided by the Max-Planck-Gesellschaft and Bundesministerium für Bildung und Forschung through Project No. 05K13SJ2. We acknowledge DESY (Hamburg, Germany), a member of the Helmholtz Association HGF, for the provision of experimental facilities. Parts of this research were carried out at PETRAIII. Work by C.S. was supported by the Deutsche Forschungsgemeinschaft Project No. 266229290 and by an appointment to the NASA Postdoctoral Program at the NASA Goddard Space Flight Center, administered by Universities Space Research Association under contract with NASA. P.A. acknowledges support from Fundação para a Ciência e a Tecnologia, Portugal, under Grant No. UID/FIS/04559/2020(LIBPhys) and under Contract No. SFRH/BPD/92329/2013. Work at UNIST was supported by the National Research Foundation of Korea (Grant No. NRF-2016R1A5A1013277). Work at LLNL was performed under the auspices of the U.S. Department of Energy under Contract No. DE-AC52-07NA27344 and supported by NASA grants to LLNL. M.A.L. and F.S.P. acknowledge support from NASA's Astrophysics Program.

FundersFunder number
NRF-2016R1A5A1013277
Universities Space Research Association
U.S. Department of EnergyDE-AC52-07NA27344
National Aeronautics and Space Administration
Deutsche Forschungsgemeinschaft266229290
Fundação para a Ciência e a TecnologiaUID/FIS/04559/2020, SFRH/BPD/92329/2013
Bundesministerium für Bildung und Forschung05K13SJ2
National Research Foundation of Korea
Max-Planck-Gesellschaft

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