High-Precision Transition Energy Measurements of Neonlike Fe XVII Ions

dc.contributor.authorShah, Chintan
dc.contributor.authorTogawa, Moto
dc.contributor.authorBotz, Marc
dc.contributor.authorDanisch, Jonas
dc.contributor.authorGoes, Joschka J.
dc.contributor.authorBernitt, Sonja
dc.contributor.authorMaxton, Marleen
dc.contributor.authorKöbnick, Kai
dc.contributor.authorBuck, Jen
dc.contributor.authorSeltmann, Jörn
dc.contributor.authorHoesch, Moritz
dc.contributor.authorGu, Ming Feng
dc.contributor.authorPorter, F. Scott
dc.contributor.authorPfeifer, Thomas
dc.contributor.authorLeutenegger, Maurice A.
dc.contributor.authorCheung, Charles
dc.contributor.authorSafronova, Marianna S.
dc.contributor.authorLópez-Urrutia, José R. Crespo
dc.date.accessioned2024-02-06T18:11:59Z
dc.date.available2024-02-06T18:11:59Z
dc.date.issued2024-01-16
dc.description.abstractWe improve eight-fold 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 velocity-equivalent +/- ~5 km/s in their rest energies, substantially improving our knowledge of this key astrophysical ion. Our large-scale configuration-interaction computations include more than four million configurations and agree with the experiment at a level without precedent for a ten-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.
dc.description.sponsorshipThis research was funded by the Max Planck Society (MPG) and the German Federal Ministry of Education and Research (BMBF) under project 05K13SJ2. C.S. acknowledges support from NASA under grant number 80GSFC21M0002 and MPG. F.S.P. and M.A.L. acknowledge support from the NASA Astrophysics Program. The theoretical work has been supported by the US NSF Grants No. PHY-2012068, PHY-2309254, and US Office of Naval Research Grant No. N00014-20-1-2513. Calculations were performed in part using the computing resources at the University of Delaware, in particular, the Caviness and DARWIN high-performance computing clusters. M.S.S. thanks MPIK for hospitality. We thank 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 the P04 team at PETRA III for their skillful and reliable work.
dc.description.urihttps://arxiv.org/abs/2401.08395
dc.format.extent13 pages
dc.genrejournal articles
dc.genrepreprints
dc.identifier.urihttps://doi.org/10.48550/arXiv.2401.08395
dc.identifier.urihttp://hdl.handle.net/11603/31566
dc.language.isoen_US
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Center for Space Sciences and Technology
dc.relation.ispartofUMBC Faculty Collection
dc.rightsThis work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law.
dc.rightsPDM 1.0 DEED Public Domain Mark 1.0 Universalen
dc.rights.urihttps://creativecommons.org/publicdomain/mark/1.0/
dc.titleHigh-Precision Transition Energy Measurements of Neonlike Fe XVII Ions
dc.typeText
dcterms.creatorhttps://orcid.org/0000-0002-6484-3803

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