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A new benchmark of soft X-ray transition energies of Ne , CO 2 , and SF 6 : paving a pathway towards ppm accuracy.
Stierhof, J; Kühn, S; Winter, M; Micke, P; Steinbrügge, R; Shah, C; Hell, N; Bissinger, M; Hirsch, M; Ballhausen, R; Lang, M; Gräfe, C; Wipf, S; Cumbee, R; Betancourt-Martinez, G L; Park, S; Niskanen, J; Chung, M; Porter, F S; Stöhlker, T; Pfeifer, T; Brown, G V; Bernitt, S; Hansmann, P; Wilms, J; Crepso López-Urrutia, J R; Leutenegger, M A.
Afiliación
  • Stierhof J; Dr. Karl Remeis-Observatory and Erlangen Centre for Astroparticle Physics, Friedrich-Alexander-Universität Erlangen-Nürnberg, Sternwartstr. 7, 96049 Bamberg, Germany.
  • Kühn S; Max-Planck-Institut für Kernphysik, Saupfercheckweg 1, 69117 Heidelberg, Germany.
  • Winter M; Institute of Theoretical Physics, Friedrich-Alexander-Universität Erlangen-Nürnberg, Staudtstr. 7/B2, 91058 Erlangen, Germany.
  • Micke P; CNRS, Institut NEEL, Université Grenoble Alpes, CNRS, Institut NEEL, 25 rue des Martyrs BP 166, 38042 Grenoble Cedex 9, France.
  • Steinbrügge R; Max-Planck-Institut für Kernphysik, Saupfercheckweg 1, 69117 Heidelberg, Germany.
  • Shah C; CERN, 1211 Geneva 23, Switzerland.
  • Hell N; Deutsches Elektronen-Synchrotron DESY, Notkestr. 85, 22607 Hamburg, Germany.
  • Bissinger M; Max-Planck-Institut für Kernphysik, Saupfercheckweg 1, 69117 Heidelberg, Germany.
  • Hirsch M; NASA Goddard Space Flight Center, 8800 Greenbelt Rd., Greenbelt, MD 20771 USA.
  • Ballhausen R; Lawrence Livermore National Laboratory, 7000 East Ave., Livermore, CA 94550 USA.
  • Lang M; Lawrence Livermore National Laboratory, 7000 East Ave., Livermore, CA 94550 USA.
  • Gräfe C; Dr. Karl Remeis-Observatory and Erlangen Centre for Astroparticle Physics, Friedrich-Alexander-Universität Erlangen-Nürnberg, Sternwartstr. 7, 96049 Bamberg, Germany.
  • Wipf S; Dr. Karl Remeis-Observatory and Erlangen Centre for Astroparticle Physics, Friedrich-Alexander-Universität Erlangen-Nürnberg, Sternwartstr. 7, 96049 Bamberg, Germany.
  • Cumbee R; Dr. Karl Remeis-Observatory and Erlangen Centre for Astroparticle Physics, Friedrich-Alexander-Universität Erlangen-Nürnberg, Sternwartstr. 7, 96049 Bamberg, Germany.
  • Betancourt-Martinez GL; Dr. Karl Remeis-Observatory and Erlangen Centre for Astroparticle Physics, Friedrich-Alexander-Universität Erlangen-Nürnberg, Sternwartstr. 7, 96049 Bamberg, Germany.
  • Park S; Dr. Karl Remeis-Observatory and Erlangen Centre for Astroparticle Physics, Friedrich-Alexander-Universität Erlangen-Nürnberg, Sternwartstr. 7, 96049 Bamberg, Germany.
  • Niskanen J; Institut für Optik und Quantenelektronik, Friedrich-Schiller-Universität Jena, Max-Wien-Platz 1, 07743 Jena, Germany.
  • Chung M; NASA Goddard Space Flight Center, 8800 Greenbelt Rd., Greenbelt, MD 20771 USA.
  • Porter FS; Department of Astronomy, University of Maryland, College Park, MD 20742 USA.
  • Stöhlker T; Institut de Recherche en Astrophysique et Planétologie, 9, avenue du Colonel Roche BP 44346, 31028 Toulouse Cedex 4, France.
  • Pfeifer T; Ulsan National Institute of Science and Technology, 50 UNIST-gil, Ulsan, South Korea.
  • Brown GV; Institute for Methods and Instrumentation in Synchrotron Radiation Research G-ISRR, Helmholtz-Zentrum Berlin für Materialien und Energie, Albert-Einstein-Strasse 15, 12489 Berlin, Germany.
  • Bernitt S; Ulsan National Institute of Science and Technology, 50 UNIST-gil, Ulsan, South Korea.
  • Hansmann P; NASA Goddard Space Flight Center, 8800 Greenbelt Rd., Greenbelt, MD 20771 USA.
  • Wilms J; Institut für Optik und Quantenelektronik, Friedrich-Schiller-Universität Jena, Max-Wien-Platz 1, 07743 Jena, Germany.
  • Crepso López-Urrutia JR; GSI Helmholtzzentrum für Schwerionenforschung, Planckstraße 1, 64291 Darmstadt, Germany.
  • Leutenegger MA; Helmholtz-Institut Jena, Fröbelstieg 3, 07743 Jena, Germany.
Article en En | MEDLINE | ID: mdl-35273463
ABSTRACT
Abstract A key requirement for the correct interpretation of high-resolution X-ray spectra is that transition energies are known with high accuracy and precision. We investigate the K-shell features of Ne , CO 2 , and SF 6 gases, by measuring their photo ion-yield spectra at the BESSY II synchrotron facility simultaneously with the 1s-np fluorescence emission of He-like ions produced in the Polar-X EBIT. Accurate ab initio calculations of transitions in these ions provide the basis of the calibration. While the CO 2 result agrees well with previous measurements, the SF 6 spectrum appears shifted by ∼ 0.5 eV, about twice the uncertainty of the earlier results. Our result for Ne shows a large departure from earlier results, but may suffer from larger systematic effects than our other measurements. The molecular spectra agree well with our results of time-dependent density functional theory. We find that the statistical uncertainty allows calibrations in the desired range of 1-10 meV, however, systematic contributions still limit the uncertainty to ∼ 40-100 meV, mainly due to the temporal stability of the monochromator energy scale. Combining our absolute calibration technique with a relative energy calibration technique such as photoelectron energy spectroscopy will be necessary to realize its full potential of achieving uncertainties as low as 1-10 meV.

Texto completo: 1 Base de datos: MEDLINE Idioma: En Revista: Eur Phys J D At Mol Opt Phys Año: 2022 Tipo del documento: Article

Texto completo: 1 Base de datos: MEDLINE Idioma: En Revista: Eur Phys J D At Mol Opt Phys Año: 2022 Tipo del documento: Article