1969
DOI: 10.1103/physrevlett.23.1397
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Multiplet Splitting of Core-Electron Binding Energies in Transition-Metal Ions

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Cited by 304 publications
(119 citation statements)
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“…In 3d transition metal compounds, a well separated satellite by spin-exchange interaction can only be seen for the 3s orbital. This is because the multiplet effect in the 3s spectrum is less prominent than in the other core-level spectra and the magnitude of the exchange integral between the 3d and each core-level is the largest for the 3s level [14,15,16]. Then, we also deconvoluted this small peak into two components corresponding to the Mn(1) and Mn(2) components by assuming a relative intensity of 2:3.…”
Section: Resultsmentioning
confidence: 99%
“…In 3d transition metal compounds, a well separated satellite by spin-exchange interaction can only be seen for the 3s orbital. This is because the multiplet effect in the 3s spectrum is less prominent than in the other core-level spectra and the magnitude of the exchange integral between the 3d and each core-level is the largest for the 3s level [14,15,16]. Then, we also deconvoluted this small peak into two components corresponding to the Mn(1) and Mn(2) components by assuming a relative intensity of 2:3.…”
Section: Resultsmentioning
confidence: 99%
“…This phenomenon is termed multiplet SJ>litting of core-level binding energies. It was first reported in molecules by Hedman~ ~~., 10 12 . It has since been studied in transition metal salts 13 -lB and in the valence-band spectra of metal~.…”
Section: This Technique Is Capable Of Yielding Binding Energiesmentioning
confidence: 96%
“…These splittings are considerably reduced from free-ion predictions, and a major source of this reduction appears to be covalent-bondfng effects. 8 The 3p binding energies in these solids also give evidence for splittings, but from both a theoretical and experimental point of view, the interpretation of this data is less straightforward. 8…”
Section: This Is a Library Circulatingmentioning
confidence: 99%
“…8 • 9 Thus, the relative intensities obtained from frozen-orbital MHT calculations on Mn 3 + are: 5 P 1 , 0.66; 5 The P 2 peak would thus probably be too weak to observe. Spectra for MnF 2 in fact show two weaker components (3p(2) and 3p(3)) in addition to 3p(l).…”
Section: Ucrl-19566mentioning
confidence: 99%