Spin-Orbit Components of Resonant Satellite Photoionization of Atomic Cu
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Abstract
A new approach of the study on the spin-orbit components of resonant satellite photoionization has been carried out from many-body perturbation theory. The 3d8 4s2 (1G, 3F,1D) satellite lines of atomic Cu are resonantly enhanced and separated by the spin-orbit splitting at the energy of the 3p63d104s → 3p5 (2 P1/2, 2 P3/2) 3d10 4s2 transitions. The calculated results showing that the spin-orbit splitting leads to the separation of resonant peaks of satellite lines are in good agreement with experiment.
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Cite this article:
LIU Jin-chao. Spin-Orbit Components of Resonant Satellite Photoionization of Atomic Cu[J]. Chin. Phys. Lett., 1996, 13(12): 899-901.
LIU Jin-chao. Spin-Orbit Components of Resonant Satellite Photoionization of Atomic Cu[J]. Chin. Phys. Lett., 1996, 13(12): 899-901.
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LIU Jin-chao. Spin-Orbit Components of Resonant Satellite Photoionization of Atomic Cu[J]. Chin. Phys. Lett., 1996, 13(12): 899-901.
LIU Jin-chao. Spin-Orbit Components of Resonant Satellite Photoionization of Atomic Cu[J]. Chin. Phys. Lett., 1996, 13(12): 899-901.
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