1984
DOI: 10.1088/0022-3719/17/20/018
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Calculation of Mg atom-metals XPS and Auger shifts using a ΔSCF excited atom model

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1986
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Cited by 23 publications
(13 citation statements)
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“…For both Be and Mg, the calculated core-electron binding energies are within 0.3 eV of experimental values. [45][46][47][48][49][50][51][52][53] Finally we turn our attention to the prediction of coreelectron binding energies of adsorbed molecules. We have carried out calculations for four molecules, H 2 O, OH, CO and HCOO, on Cu(111).…”
Section: Resultsmentioning
confidence: 99%
“…For both Be and Mg, the calculated core-electron binding energies are within 0.3 eV of experimental values. [45][46][47][48][49][50][51][52][53] Finally we turn our attention to the prediction of coreelectron binding energies of adsorbed molecules. We have carried out calculations for four molecules, H 2 O, OH, CO and HCOO, on Cu(111).…”
Section: Resultsmentioning
confidence: 99%
“…Figure 1 d shows the fine XPS spectra of Mg. The peak of Mg 1s located at 1303.6 eV can be observed in the spectrum of the ZnMgO film, and deviates from the peak of Mg (1303.3 eV) [ 31 ], which indicates that Mg loses the outer electrons. Further, in Figure 1 e, the binding energy of Zn 2p 3/2 in ZnMgO (1021.1 eV) is higher than that of Zn 2p 3/2 in ZnO (1021.0 eV), revealing that the Zn-O-Mg bonds are formed in ZnMgO film [ 27 ].…”
Section: Resultsmentioning
confidence: 99%
“…Copper‐related peaks were observed at 954.87 eV and 926.1 eV corresponding to Cu 2p1/2 and Cu 2p3/2 spin orbitals, respectively. [ 35 ] Magnesium 1s orbital peak was observed at 1303.99 eV corresponding to metallic Mg. [ 36 ] At 50.63 eV Mg 2p peak was observed. [ 36 ] To confirm the absence of MgO in Cu‐5, Auger KLL was recorded.…”
Section: Resultsmentioning
confidence: 99%
“…[ 35 ] Magnesium 1s orbital peak was observed at 1303.99 eV corresponding to metallic Mg. [ 36 ] At 50.63 eV Mg 2p peak was observed. [ 36 ] To confirm the absence of MgO in Cu‐5, Auger KLL was recorded. The absence of MgO in Cu‐5 was confirmed from the absence of satellite peaks in between 310.45 eV and 305.99 eV corresponding to KLL Auger of Mg. [ 36,37 ] The O 1s spectrum was deconvoluted as two peaks positioned at 531.59 eV and 529.56 eV.…”
Section: Resultsmentioning
confidence: 99%