✍ Scribed by H. Pulm; C.-M. Liegener; H.-J. Freund
No coin nor oath required. For personal study only.
WC hnvc rccordcd the carbon and mmogen KVV Auger spccrra 01 NaCN. caciLed wiith X-rays. The .spcrLn are inlerpreled on the hns~s or nb rn;uo many-body calculations of the double hole shade energies and fnkznsiks or CN-. The nilrogen (KW) Auger sprr~rum or NLN is more slrnllx IO the N(KV') specwum or N, than the carbon (KVV) Auger speclrum or NnCN is IO Lhc C(KVV) sp~~rrum or CO This nbgerv.IIlon 1s well reproduced by Ihe calculations We conclude LhaL the alrong influence or rhe Ioc~hw~~on of the orblmls in CO on the Auger speclra has dlsappexed in CN-. atrhough the delocahzakn 15 I-IOL -1s pronounLed J\ m V, On the harls or the calculations IL is possible 10 assign sn~clli[c sIrucIure in Ihr N(KVV) Auger hpeclrum or CN -_ 1" cnmpnrlron IC, rhc N( KVV) .augcr specrrum or N;_
📜 SIMILAR VOLUMES
XO~ scattered-wave calculations have been performed to compare the photon energy dependence of rhe valence level photoionization CIOSS sections of molecular CO and N2 and of Ni clusters simulatmg the adsorption of these molecules in the range of the shape resonances. Care has to be taken to avoid mu