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 – Published 25 June 2009

Abstract

The K-shell diagram (Kα1,2 and Kβ1,3) and hypersatellite (HS) (Khα1,2) spectra of Y, Zr, Mo, and Pd have been measured with high energy-resolution using photoexcitation by 90 keV synchrotron radiation. Comparison of the measured and ab initio calculated HS spectra demonstrates the importance of quantum electrodynamical (QED) effects for the HS spectra. Phenomenological fits of the measured spectra by Voigt functions yield accurate values for the shift of the HS from the diagram lines, the splitting of the HS lines, and their intensity ratio. Good agreement with theory was found for all quantities except for the intensity ratio, which is dominated by the intermediacy of the coupling of the angular momenta. The observed deviations imply that our current understanding of the variation of the coupling scheme from LS to jj across the periodic table may require some revision.

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  • Received 15 December 2008

DOI:https://doi.org/10.1103/PhysRevA.79.062512

©2009 American Physical Society

Authors & Affiliations

R. Diamant1, S. Huotari2, K. Hämäläinen3,*, R. Sharon1, C. C. Kao4, V. Honkimäki2, T. Buslaps2, 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

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 (2009)

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Vol. 79, Iss. 6 — June 2009

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