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High-Precision Determination of Oxygen K_{α} Transition Energy Excludes Incongruent Motion of Interstellar Oxygen.
Leutenegger, M A; Kühn, S; Micke, P; Steinbrügge, R; Stierhof, J; Shah, C; Hell, N; Bissinger, M; Hirsch, M; Ballhausen, R; Lang, M; Gräfe, C; Wipf, S; Cumbee, R; Betancourt-Martinez, G L; Park, S; Yerokhin, V A; Surzhykov, A; Stolte, W C; Niskanen, J; Chung, M; Porter, F S; Stöhlker, T; Pfeifer, T; Wilms, J; Brown, G V; Crespo López-Urrutia, J R; Bernitt, S.
Afiliação
  • Leutenegger MA; NASA Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, Maryland 20771, USA.
  • Kühn S; Max-Planck-Institut für Kernphysik, Saupfercheckweg 1, 69117 Heidelberg, Germany.
  • Micke P; Max-Planck-Institut für Kernphysik, Saupfercheckweg 1, 69117 Heidelberg, Germany.
  • Steinbrügge R; Physikalisch-Technische Bundesanstalt, Bundesallee 100, 38116 Braunschweig, Germany.
  • Stierhof J; Deutsches Elektronen-Synchrotron DESY, Notkestrasse 85, 22607 Hamburg, Germany.
  • Shah C; Remeis-Sternwarte and Erlangen Centre for Astroparticle Physics, Friedrich-Alexander-Universität Erlangen-Nürnberg, Sternwartstrasse 7, 96049 Bamberg, Germany.
  • Hell N; NASA Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, Maryland 20771, USA.
  • Bissinger M; Max-Planck-Institut für Kernphysik, Saupfercheckweg 1, 69117 Heidelberg, Germany.
  • Hirsch M; Lawrence Livermore National Laboratory, 7000 East Avenue, Livermore, California 94550, USA.
  • Ballhausen R; Erlangen Centre for Astroparticle Physics, Friedrich-Alexander-Universität Erlangen-Nürnberg, Erwin-Rommel-Strasse 1, 91058 Erlangen, Germany.
  • Lang M; Remeis-Sternwarte and Erlangen Centre for Astroparticle Physics, Friedrich-Alexander-Universität Erlangen-Nürnberg, Sternwartstrasse 7, 96049 Bamberg, Germany.
  • Gräfe C; Remeis-Sternwarte and Erlangen Centre for Astroparticle Physics, Friedrich-Alexander-Universität Erlangen-Nürnberg, Sternwartstrasse 7, 96049 Bamberg, Germany.
  • Wipf S; Remeis-Sternwarte and Erlangen Centre for Astroparticle Physics, Friedrich-Alexander-Universität Erlangen-Nürnberg, Sternwartstrasse 7, 96049 Bamberg, Germany.
  • Cumbee R; Remeis-Sternwarte and Erlangen Centre for Astroparticle Physics, Friedrich-Alexander-Universität Erlangen-Nürnberg, Sternwartstrasse 7, 96049 Bamberg, Germany.
  • Betancourt-Martinez GL; Institut für Optik und Quantenelektronik, Friedrich-Schiller-Universität Jena, Max-Wien-Platz 1, 07743 Jena, Germany.
  • Park S; NASA Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, Maryland 20771, USA.
  • Yerokhin VA; Department of Astronomy, University of Maryland, College Park, Maryland 20742, USA.
  • Surzhykov A; Institut de Recherche en Astrophysique et Planétologie, 9, avenue du Colonel Roche BP 44346, 31028 Toulouse Cedex 4, France.
  • Stolte WC; Ulsan National Institute of Science and Technology, 50 UNIST-gil, 44919 Ulsan, Republic of Korea.
  • Niskanen J; Peter the Great St. Petersburg Polytechnic University, 195251 St. Petersburg, Russia.
  • Chung M; Physikalisch-Technische Bundesanstalt, Bundesallee 100, 38116 Braunschweig, Germany.
  • Porter FS; Institut für Mathematische Physik, Technische Universität Braunschweig, D-38106 Braunschweig, Germany.
  • Stöhlker T; Advanced Light Source, Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA.
  • Pfeifer T; 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.
  • Wilms J; Department of Physics and Astronomy, University of Turku, FI-20014 Turun Yliopisto, Finland.
  • Brown GV; Ulsan National Institute of Science and Technology, 50 UNIST-gil, 44919 Ulsan, Republic of Korea.
  • Crespo López-Urrutia JR; NASA Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, Maryland 20771, USA.
  • Bernitt S; Institut für Optik und Quantenelektronik, Friedrich-Schiller-Universität Jena, Max-Wien-Platz 1, 07743 Jena, Germany.
Phys Rev Lett ; 125(24): 243001, 2020 Dec 11.
Article em En | MEDLINE | ID: mdl-33412031
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.

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Phys Rev Lett Ano de publicação: 2020 Tipo de documento: Article País de afiliação: Estados Unidos

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Phys Rev Lett Ano de publicação: 2020 Tipo de documento: Article País de afiliação: Estados Unidos