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Phys. Rev. B 56, 12238–12242 (1997)

Energy dependence of Cu L2,3 satellites using synchrotron excited x-ray-emission spectroscopy

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M. Magnuson, N. Wassdahl, and J. Nordgren
Department of Physics, Uppsala University, P.O. Box 530, S-751 21 Uppsala, Sweden

Received 15 May 1997; published in the issue dated 15 November 1997

The L2,3 x-ray emission of Cu metal has been measured using monochromatic synchrotron radiation. The self-absorption effect in the spectra is shown to be very small in our experimental geometry. From the quantitative analysis of spectra recorded at different excitation energies, the L3/L2 emission intensity ratio and the partial Auger width are extracted. High-energy satellite features on the L3 emission line are separated by a subtraction procedure. The satellite intensity is found to be slowly increasing for excitation energies between the L3, L2, and L1 core-level thresholds due to shake-up and shake-off transitions. As the excitation energy passes the L2 threshold, a step of rapidly increasing satellite intensity of the L3 emission is found due to additional Coster-Kronig processes.

© 1997 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevB.56.12238
DOI:
10.1103/PhysRevB.56.12238
PACS:
78.70.En, 32.30.Rj