1979
DOI: 10.1103/physrevlett.43.1829
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Two-Electron Resonance at the3pThreshold of Cu and Ni

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Cited by 185 publications
(32 citation statements)
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“…Furthermore the corresponding satellite structures are located at energies between 10 eV and 15 eV below E F , well outside our range of observations (57). The core level excitation thresholds of the Cu 3p and 3s core electrons are located at 75.0 eV, 77.7 eV and 122.4 eV.…”
Section: Sample Preparation and Orientationsupporting
confidence: 74%
“…Furthermore the corresponding satellite structures are located at energies between 10 eV and 15 eV below E F , well outside our range of observations (57). The core level excitation thresholds of the Cu 3p and 3s core electrons are located at 75.0 eV, 77.7 eV and 122.4 eV.…”
Section: Sample Preparation and Orientationsupporting
confidence: 74%
“…It is well known that the Cu3p core levels locate around -75 eV [4,5,6,7], and we observed them at -76.7 and -75.1 eV in our OD71 sample. Thus, one can expect that such photon energy would enhance the direct transition Cu3p 6 3d 9 +hν→Cu3p 6 3d 8 +e − due to an interference with a super Coster-Kronig Auger decay process described by Cu3p 6 3d 9 +hν→Cu3p 5 3d 10 →Cu3p 6 3d 8 +e…”
supporting
confidence: 61%
“…However, other factors apart from the degree of hybridization, such as the presence of multielectron resonant satellites, may affect the valence-band resonance. 34,35 In addition, overlapping intensity variations due to the appearance of MVV Auger transitions may contribute at the bottom of the band. 28 Nevertheless, the trend in the resonant photoemission results for Co 2 MnSn is analogous to that obtained for Ni 2 10 The resulting theoretically derived PDOS's were convoluted and normalized using the same procedure as that outlined for Co 2 MnSn.…”
Section: Resultsmentioning
confidence: 99%