Summary
Recently available data for the EXAFS at theL 3-edge of rhenium metal have been used to account for the origin ofL α andL β satellites on the basis of Hayasi’s theory. The calculated wave-lengths for the satellites are in good agreement with the experimental results and are compared with the values calculated from multiple-ionization theory. The present study reveals that the plasmon level behaves like a quasi-stationary state in the emission of the satellites.
Riassunto
Recentemente dati disponibili per l’EXAFS all’estremitàL 3 del metallo renio sono stati usati per spiegare l’origine di satelliti di tipoL α eL β tenendo conto della teoria di Hayasi. Le lunghezze d’onda calcolate per i satelliti sono in buon accordo con i risultati sperimentali e sono confrontate con i valori calcolati per la teoria di ionizzazione multipla. Il presente studio rivela che il livello di plasmon si comporta nell’emissione di satelliti come uno stato quasi stazionario.
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Shrivastava, B.D., Landge, P.R. Extended X-ray absorption fine structure and theL α andL β satellites of rhenium. Nuov Cim B 49, 118–123 (1979). https://doi.org/10.1007/BF02737479
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DOI: https://doi.org/10.1007/BF02737479