Natural-linewidth measurements of the 3⁢𝐶 and 3⁢𝐷 soft-x-ray transitions in Ni xix

Author(s)Shah, Chintan
Author(s)Kühn, Steffen
Author(s)Bernitt, Sonja
Author(s)Steinbrügge, René
Author(s)Togawa, Moto
Author(s)Berger, Lukas
Author(s)Buck, Jens
Author(s)Hoesch, Moritz
Author(s)Seltmann, Jörn
Author(s)Kozlov, Mikhail G.
Author(s)Porsev, Sergey G.
Author(s)Gu, Ming Feng
Author(s)Porter, F. Scott
Author(s)Pfeifer, Thomas
Author(s)Leutenegger, Maurice A.
Author(s)Cheung, Charles
Author(s)Safronova, Marianna S.
Author(s)Crespo López-Urrutia, José R.
Date Accessioned2024-06-21T19:34:32Z
Date Available2024-06-21T19:34:32Z
Publication Date2024-06-10
DescriptionThis article was originally published in Physical Review A . The version of record is available at: https://doi.org/10.1103/PhysRevA.109.063108. ©2024 American Physical Society. Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Open access publication funded by Max Planck Society.
AbstractWe used the monochromatic soft-x-ray beamline P04 at the synchrotron-radiation facility PETRA III to resonantly excite the strongest 2⁢𝑝−3⁢𝑑 transitions in neonlike Nixix ions, [2⁢𝑝6]𝐽=0→[(2⁢𝑝5)1/23⁢𝑑3/2]𝐽=1 and [2⁢𝑝6]𝐽=0→[(2⁢𝑝5)3/23⁢𝑑5/2]𝐽=1, respectively dubbed 3⁢𝐶 and 3⁢𝐷, achieving a resolving power of 15 000 and signal-to-background ratio of 30. We obtain their natural linewidths, with an accuracy of better than 10%, as well as the oscillator-strength ratio 𝑓⁡(3⁢𝐶)/𝑓⁡(3⁢𝐷)=2.51⁢(11) from analysis of the resonant fluorescence spectra. These results agree with those of previous experiments, earlier predictions, and our own advanced calculations.
SponsorThis research was funded by the Max Planck Society (MPG) and the German Federal Ministry of Education and Research (BMBF) under Project No. 05K13SJ2. C.S. acknowledges support from MPG and the NASA Astrophysics Program. F.S.P. and M.A.L. acknowledge support from the NASA Astrophysics Program. The theoretical work was supported by U.S. NSF Grants No. PHY-2012068 and No. PHY-2309254, U.S. Office of Naval Research Grant No. N00014-20-1-2513, and the European Research Council (ERC) under the Horizon 2020 Research and Innovation Programme of the European Union (Grant Agreement No. 856415). Calculations were performed in part using the computing resources at the University of Delaware, in particular the Caviness and DARWIN high-performance computing clusters. This theoretical work, including M.G.K.'s contributions, was carried out as part of a scientific collaboration during the calendar year 2020. 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 PETRA III. We thank J. Viefhaus and R. Follath for valuable discussions on x-ray monochromator resolution and performance and the synchrotron-operation team and P04 team at PETRA III for their skillful and reliable work. M.S.S. thanks MPIK, Heidelberg, for hospitality.
CitationShah, Chintan, Steffen Kühn, Sonja Bernitt, René Steinbrügge, Moto Togawa, Lukas Berger, Jens Buck, et al. “Natural-Linewidth Measurements of the 3 C and 3 D Soft-x-Ray Transitions in Ni Xix.” Physical Review A 109, no. 6 (June 10, 2024): 063108. https://doi.org/10.1103/PhysRevA.109.063108.
ISSN2469-9934
URLhttps://udspace.udel.edu/handle/19716/34512
Languageen_US
PublisherPhysical Review A
dc.rightsAttribution 4.0 Internationalen
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/
TitleNatural-linewidth measurements of the 3⁢𝐶 and 3⁢𝐷 soft-x-ray transitions in Ni xix
TypeArticle
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