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| Verfasst von: | Kühn, Steffen [VerfasserIn]  |
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| | Cheung, Charles [VerfasserIn] |
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| | Oreshkina, Natalia S. [VerfasserIn] |
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| | Steinbrügge, René [VerfasserIn] |
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| | Togawa, Moto [VerfasserIn] |
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| | Bernitt, Sonja [VerfasserIn] |
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| | Berger, Lukas [VerfasserIn] |
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| | Buck, Jens [VerfasserIn] |
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| | Hoesch, Moritz [VerfasserIn] |
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| | Seltmann, Jörn [VerfasserIn] |
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| | Trinter, Florian [VerfasserIn] |
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| | Keitel, Christoph H. [VerfasserIn] |
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| | Kozlov, Mikhail G. [VerfasserIn] |
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| | Porsev, Sergey G. [VerfasserIn] |
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| | Gu, Ming Feng [VerfasserIn] |
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| | Porter, F. Scott [VerfasserIn] |
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| | Pfeifer, Thomas [VerfasserIn] |
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| | Leutenegger, Maurice A. [VerfasserIn] |
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| | Harman, Zoltán [VerfasserIn] |
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| | Safronova, Marianna S. [VerfasserIn] |
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| | Crespo López-Urrutia, José Ramon [VerfasserIn] |
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| | Shah, Chintan [VerfasserIn] |
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| Titel: | New measurement resolves key astrophysical Fe XVII oscillator strength problem |
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| Verf.angabe: | Steffen Kühn, Charles Cheung, Natalia S. Oreshkina, René Steinbrügge, Moto Togawa, Sonja Bernitt, Lukas Berger, Jens Buck, Moritz Hoesch, Jörn Seltmann, Florian Trinter, Christoph H. Keitel, Mikhail G. Kozlov, Sergey G. Porsev, Ming Feng Gu, F. Scott Porter, Thomas Pfeifer, Maurice A. Leutenegger, Zoltán Harman, Marianna S. Safronova, José R. Crespo López-Urrutia, Chintan Shah |
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| E-Jahr: | 2022 |
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| Jahr: | 5 December 2022 |
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| Umfang: | 8 S. |
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| Fussnoten: | Gesehen am 08.12.2022 |
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| Titel Quelle: | Enthalten in: Physical review letters |
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| Ort Quelle: | College Park, Md. : APS, 1958 |
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| Jahr Quelle: | 2022 |
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| Band/Heft Quelle: | 129(2022), 24, Artikel-ID 245001, Seite 1-8 |
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| ISSN Quelle: | 1079-7114 |
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| Abstract: | One of the most enduring and intensively studied problems of x-ray astronomy is the disagreement of state-of-the art theory and observations for the intensity ratio of two Fe XVII transitions of crucial value for plasma diagnostics, dubbed 3C and 3D. We unravel this conundrum at the PETRA III synchrotron facility by increasing the resolving power 2.5 times and the signal-to-noise ratio thousandfold compared with our previous work. The Lorentzian wings had hitherto been indistinguishable from the background and were thus not modeled, resulting in a biased line-strength estimation. The present experimental oscillator-strength ratio Rexp=f3C/f3D=3.51(2)stat(7)sys agrees with our state-of-the-art calculation of Rth=3.55(2), as well as with some previous theoretical predictions. To further rule out any uncertainties associated with the measured ratio, we also determined the individual natural linewidths and oscillator strengths of 3C and 3D transitions, which also agree well with the theory. This finally resolves the decades-old mystery of Fe XVII oscillator strengths. |
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| DOI: | doi:10.1103/PhysRevLett.129.245001 |
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| URL: | Bitte beachten Sie: Dies ist ein Bibliographieeintrag. Ein Volltextzugriff für Mitglieder der Universität besteht hier nur, falls für die entsprechende Zeitschrift/den entsprechenden Sammelband ein Abonnement besteht oder es sich um einen OpenAccess-Titel handelt.
Volltext: https://doi.org/10.1103/PhysRevLett.129.245001 |
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| | Volltext: https://link.aps.org/doi/10.1103/PhysRevLett.129.245001 |
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| | DOI: https://doi.org/10.1103/PhysRevLett.129.245001 |
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| Datenträger: | Online-Ressource |
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| Sprache: | eng |
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| K10plus-PPN: | 1826633529 |
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| Verknüpfungen: | → Zeitschrift |
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New measurement resolves key astrophysical Fe XVII oscillator strength problem / Kühn, Steffen [VerfasserIn]; 5 December 2022 (Online-Ressource)
