1994
DOI: 10.1002/qua.560520114
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Core photoionization satellites in fullerence and related model systems

Abstract: The so-called shake-up satellites accompanying C1, photoionization in Cm have been studied theoretically by means of INDO/CI. It is found that the lowest shake-up satellites in Cm correspond to global charge-transfer excitations that move charge from the opposite side of the fullerene cage to the core-hole region, whereas higher-energy satellites tend to move charge from regions nearer to the core hole. Analogies are drawn, with, on the one hand, smaller model molecules such as napthalene and acenaphtylene and… Show more

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Cited by 11 publications
(6 citation statements)
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“…27,28 The use of the ECH approximation in the XPS shake-up satellites has already been illustrated in several semiempirical computations. [48][49][50] The combination of the ECH approximation and the TDDFT technique provides an efficient and accurate procedure for the computations of all possible multiple valence electron excitations with inclusion of the electron correlation. 27,28 The applicability of the ECH-TDDFT approach has been demonstrated by Brena et al in the studies of the XPS shake-up satellites of benzene, metal free phthalocyanine, and nickel phthalocyanines.…”
Section: 47mentioning
confidence: 99%
“…27,28 The use of the ECH approximation in the XPS shake-up satellites has already been illustrated in several semiempirical computations. [48][49][50] The combination of the ECH approximation and the TDDFT technique provides an efficient and accurate procedure for the computations of all possible multiple valence electron excitations with inclusion of the electron correlation. 27,28 The applicability of the ECH-TDDFT approach has been demonstrated by Brena et al in the studies of the XPS shake-up satellites of benzene, metal free phthalocyanine, and nickel phthalocyanines.…”
Section: 47mentioning
confidence: 99%
“…C 1s→LUMO x-ray-absorption spectra for the indicated samples, at a resolution of 0.16 eV (Maxwell et al, , 1998. The inset is a Zϩ1 calculation (Enkvist et al, 1993;Lunell et al, 1994) of the LUMO wave function, which should be applicable to XAS (Wä stberg et al, 1994;Nyberg et al, 1999). The angle of incidence of the light is indicated for the monolayer systems, whereas no angle dependence has been observed for thick films.…”
Section: C 60 : Placing and Characterizing The Core-excited Statementioning
confidence: 99%
“…The fact that a Zϩ1 description captures the essential aspects of the 1s XAS data (Wä stberg et al, 1994;Nyberg et al, 1999) strongly suggests that this description is accurate in its main details. Calculations of similar quality within a Jahn-Teller picture have not been carried out at this time, presumably due to computational difficulties, but one surmises that the results, for example, of the LUMO probability distribution in the core-excited state should be similar in its major details to that found in a Zϩ1 model (Bagus and Schaeffer, 1972;Domcke and Cederbaum, 1977;Å gren et al, 1981;Enkvist et al, 1993;Å gren, 1994, 1999;Lunell et al, 1994).…”
Section: C 60 : Placing and Characterizing The Core-excited Statementioning
confidence: 99%
“…A high resolution scan of the shake-up features for a layer (∼17 ML) of C 60 is shown in Figure 1. Lunell and Enkvist et al 32,34 were able to assign the observed peaks in an experimental spectrum to particular transitions in the Huckel molecular orbital structure, shown in Figure 1b, and the theoretically predicted peak center of mass are shown in red in Figure 1a. Almost all of the shake-up structures correspond to some transition to the 5t 1u * (LUMO) level, giving a clear picture of the valence band characteristics of C 60 .…”
Section: Resultsmentioning
confidence: 91%