The evolution of inner-shell multielectronic X-ray spectra from threshold to saturation for low- to high-Z atoms

R. Diamant, S. Huotari, K. Hämäläinen, R. Sharon, C. C. Kao, M. Deutsch

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Abstract

Inter- and intra-shell electronic correlations in an atom are manifested in, and can be studied through, the X-ray emission spectra of multielectronic transitions. We have measured the spectra of Khα1,2 hypersatellites (HS), Kα3,4 satellites (S), and the 3d electron shake-up satellites (D) accompanying the Kα1,2 diagram lines, and their evolution from the double-ionization threshold, for selected 4- and 5-row elements of the periodic table. These spectra originate in the [1 s]-1, [2p]-1, and [3d]-1 spectator two-electron transitions [1 s]-2→[1s2p]-1, [1s2p]-1→[2p]-2, and [1s3d]-1→[2p3d]-1 respectively. Photoexcitation by monochromatized synchrotron radiation together with high-resolution crystal spectrometers were employed. Ab initio relativistic multiconfigurational Dirac-Fock (RMCDF) calculations reproduce the spectra very well for all transitions, with the HS spectra showing a strong dependence on QED effects. The excitation thresholds were determined accurately. The threshold-to-saturation energy range of the intensity was found to depend strongly on the principal quantum number n of the spectator hole. For example, for Cu, ranges of 2%, 10%, and 60% of the threshold energy are found for the D, S and HS spectra, respectively. Only the D spectrum's evolution conforms to the Thomas model, indicating a dominant shake up/off process. The S and HS spectra seem to be dominated by the knockout ("two-step-one") process near threshold. The S spectra show a two-regime behavior. Near threshold both shape and intensity vary with excitation energy, and above that only intensity changes are observed. The lower-than-expected Khα1/Khα2 intensity ratio found for Z=23-30 and 39-46 indicates that the angular momenta coupling scheme at the regime intermediate between the LS coupling at low-Z and the jj coupling at high-Z may not be fully accounted for by the prevailing theory.

Original languageEnglish
Pages (from-to)1434-1446
Number of pages13
JournalRadiation Physics and Chemistry
Volume75
Issue number11 SPEC. ISS.
DOIs
StatePublished - Nov 2006

Bibliographical note

Funding Information:
Contributions by, and discussions with, O. Gang, M. Fritsch (Bar-Ilan), S. Galambosi, H. Sutinen (Helsinki), L. Berman, W. Caliebe, Z. Yin (BNL), V. Honkimäki, T. Buslaps and J.-P. Rueff (ESRF) are gratefully acknowledged. We thank NSLS for beamtime at X21 and X25, and ESRF for beamtime at ID15B and ID16. This work was supported by The Israel Science Foundation, Jerusalem (M.D.) and the Academy of Finland (contracts 201291 and 205967 for KH).

Funding

Contributions by, and discussions with, O. Gang, M. Fritsch (Bar-Ilan), S. Galambosi, H. Sutinen (Helsinki), L. Berman, W. Caliebe, Z. Yin (BNL), V. Honkimäki, T. Buslaps and J.-P. Rueff (ESRF) are gratefully acknowledged. We thank NSLS for beamtime at X21 and X25, and ESRF for beamtime at ID15B and ID16. This work was supported by The Israel Science Foundation, Jerusalem (M.D.) and the Academy of Finland (contracts 201291 and 205967 for KH).

FundersFunder number
Academy of Finland201291, 205967
Israel Science Foundation

    Keywords

    • Multielectronic transitions
    • Shake up
    • X-ray hypesatellites
    • X-ray satellites

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