TY - JOUR
T1 - K and K x-ray emission spectra of copper
AU - Deutsch, M.
AU - Hölzer, G.
AU - Härtwig, J.
AU - Wolf, J.
AU - Fritsch, M.
AU - Förster, E.
PY - 1995
Y1 - 1995
N2 - The K1,2 and K1,3 spectra of copper were measured using double- and single-crystal diffractometers whose finite resolution effects were carefully characterized and corrected for. A phenomenological resolution of the spectra into Lorentzians is given, yielding excellent R factors close to 1%. Fits to our detailed relativistic Dirac-Fock and nonrelativistic Hartree-Fock ab initio calculations reveal that the line shapes can be accounted for by the diagram and the single 3d spectator hole transitions only, with R factors of 35 % (the underline below 3d denotes a hole state). The contribution of the 3d spectator transitions to each of the spectra is 2630 %. The K spectrum may also contain a small 0.5% contribution from the 3p spectator transition. The fit residuals of the K spectrum show systematic deviations in the vicinity of the feature, which may be due to exchange interactions or plasmon excitations. Contributions of similar origins to the K spectrum were not detected. Linewidths, energies, and intensities are reported, for the raw as well as the fit-resolved spectra, and critically compared with previous data, where available.
AB - The K1,2 and K1,3 spectra of copper were measured using double- and single-crystal diffractometers whose finite resolution effects were carefully characterized and corrected for. A phenomenological resolution of the spectra into Lorentzians is given, yielding excellent R factors close to 1%. Fits to our detailed relativistic Dirac-Fock and nonrelativistic Hartree-Fock ab initio calculations reveal that the line shapes can be accounted for by the diagram and the single 3d spectator hole transitions only, with R factors of 35 % (the underline below 3d denotes a hole state). The contribution of the 3d spectator transitions to each of the spectra is 2630 %. The K spectrum may also contain a small 0.5% contribution from the 3p spectator transition. The fit residuals of the K spectrum show systematic deviations in the vicinity of the feature, which may be due to exchange interactions or plasmon excitations. Contributions of similar origins to the K spectrum were not detected. Linewidths, energies, and intensities are reported, for the raw as well as the fit-resolved spectra, and critically compared with previous data, where available.
UR - http://www.scopus.com/inward/record.url?scp=0001285775&partnerID=8YFLogxK
U2 - 10.1103/physreva.51.283
DO - 10.1103/physreva.51.283
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AN - SCOPUS:0001285775
SN - 1050-2947
VL - 51
SP - 283
EP - 296
JO - Physical Review A
JF - Physical Review A
IS - 1
ER -