1. High-Precision Determination of Oxygen Kα Transition Energy Excludes Incongruent Motion of Interstellar Oxygen
- Author
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Renata Cumbee, Thomas Pfeifer, Jörn Wilms, P. Micke, C. Gräfe, Gregory V. Brown, Jakob Stierhof, Maurice A. Leutenegger, SungNam Park, Ralf Ballhausen, Natalie Hell, Moses Chung, F. S. Porter, S. Wipf, Chintan Shah, Sven Bernitt, G. L. Betancourt-Martinez, M. Bissinger, Vladimir A. Yerokhin, René Steinbrügge, Andrey Surzhykov, M. Lang, Steffen Kühn, J. Niskanen, M. Hirsch, Thomas Stöhlker, J. R. Crespo López-Urrutia, and W. C. Stolte
- Subjects
Physics ,Absorption spectroscopy ,General Physics and Astronomy ,chemistry.chemical_element ,Scale (descriptive set theory) ,01 natural sciences ,Oxygen ,Measure (mathematics) ,Spectral line ,Ion ,symbols.namesake ,chemistry ,0103 physical sciences ,Rydberg formula ,symbols ,Atomic physics ,010306 general physics ,Energy (signal processing) - Abstract
We demonstrate a widely applicable technique to absolutely calibrate the energy scale of x-ray spectra with experimentally well-known and accurately calculable transitions of highly charged ions, allowing us to measure the K-shell Rydberg spectrum of molecular O_{2} with 8 meV uncertainty. We reveal a systematic ∼450 meV shift from previous literature values, and settle an extraordinary discrepancy between astrophysical and laboratory measurements of neutral atomic oxygen, the latter being calibrated against the aforementioned O_{2} literature values. Because of the widespread use of such, now deprecated, references, our method impacts on many branches of x-ray absorption spectroscopy. Moreover, it potentially reduces absolute uncertainties there to below the meV level.
- Published
- 2020
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