Delayed onset of 4d photoemission relative to the giant 4d photoabsorption of La

For the giant 4d photoabsorption of La, both the total photoabsorption spectrum and the N 4.5-derived Auger emission intensity spectrum increase significantly above h ν ≅ 112 eV, with spectral peaks at h ν = 118 and 119 eV, respectively. However, the predominant 4d photoemission partial cross sectio...

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Veröffentlicht in:Solid state communications 1981-02, Vol.37 (6), p.471-474
Hauptverfasser: Aono, M., Chiang, T.-C., Himpsel, F.J., Eastman, D.E.
Format: Artikel
Sprache:eng
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Zusammenfassung:For the giant 4d photoabsorption of La, both the total photoabsorption spectrum and the N 4.5-derived Auger emission intensity spectrum increase significantly above h ν ≅ 112 eV, with spectral peaks at h ν = 118 and 119 eV, respectively. However, the predominant 4d photoemission partial cross section shows a delayed onset of ∼ 4 eV, with a peak at h ν = 121 eV, while the 5s, 5p, and 5d partial cross sections all show a strong resonant enhancement at lower energies, with spectral peaks at h ν = 116.6 eV. These results are compared with a recent many-body calculation for Ce. The photon energy dependence of the La 4d 5 2 /4d 3 2 photo-emission branching ratio is consistent with a “final-state model.”
ISSN:0038-1098
1879-2766
DOI:10.1016/0038-1098(81)90481-6