Khα1,2 hypersatellites of 3d transition metals and their photoexcitation energy dependence

R. Diamant, S. Huotari, K. Hämäläinen, R. Sharon, C. C. Kao, and M. Deutsch
Phys. Rev. A 79, 062511 – Published 25 June 2009

Abstract

Hollow atoms in which the K shell is empty while the outer shells are populated allow studying a variety of important and unusual properties of atoms. The diagram x-ray emission lines of such atoms, the Khα1,2 hypersatellites (HSs), were measured for the 3d transition metals, Z=2330, with a high energy resolution using photoexcitation by monochromatized synchrotron radiation. Good agreement with ab initio relativistic multiconfigurational Dirac-Fock calculations was found. The measured HS intensity variation with the excitation energy yields accurate values for the excitation thresholds, excludes contributions from shake-up processes, and indicates domination near threshold of a nonshake process. The Z variation of the HS shifts from the diagram line Kα1,2, the Khα1Khα2 splitting, and the Khα1/Khα2 intensity ratio, derived from the measurements, are also discussed with a particular emphasis on the QED corrections and Breit interaction.

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  • Received 15 December 2008

DOI:https://doi.org/10.1103/PhysRevA.79.062511

©2009 American Physical Society

Authors & Affiliations

R. Diamant1, S. Huotari2, K. Hämäläinen3,*, R. Sharon1, C. C. Kao4, and M. Deutsch1

  • 1Department of Physics, Bar-Ilan University, Ramat-Gan 52900, Israel
  • 2ESRF, 6 rue Jules Horowitz, BP 220, F-38043 Grenoble Cedex, France
  • 3Department of Physics, University of Helsinki, P.O. Box 64, FI-00014 Helsinki, Finland
  • 4NSLS, Brookhaven National Laboratory, Upton, New York 11973, USA

  • *keijo.hamalainen@helsinki.fi

See Also

K-shell diagram and hypersatellite spectra of 4d transition elements

R. Diamant, S. Huotari, K. Hämäläinen, R. Sharon, C. C. Kao, V. Honkimäki, T. Buslaps, and M. Deutsch
Phys. Rev. A 79, 062512 (2009)

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Vol. 79, Iss. 6 — June 2009

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