1991
DOI: 10.1103/physrevb.44.13747
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C60bonding and energy-level alignment on metal and semiconductor surfaces

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Cited by 324 publications
(128 citation statements)
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“…The peak that appears at 1.9 eV has been identified as an exciton from HOMO to LUMO derived states. Both satellite features are still visible for 1.3 ML C 60 but they are not present in the 0.9 ML film, which is consistent with the fact that chemisorption of the C 60 molecules in the first layer involves mixing of the molecular and substrate levels in the initial and final states [27]. For 0.9 ML C 60 , the C 1s peak displays an asymmetric line shape.…”
Section: Resultssupporting
confidence: 67%
“…The peak that appears at 1.9 eV has been identified as an exciton from HOMO to LUMO derived states. Both satellite features are still visible for 1.3 ML C 60 but they are not present in the 0.9 ML film, which is consistent with the fact that chemisorption of the C 60 molecules in the first layer involves mixing of the molecular and substrate levels in the initial and final states [27]. For 0.9 ML C 60 , the C 1s peak displays an asymmetric line shape.…”
Section: Resultssupporting
confidence: 67%
“…The energy difference between E A and E I (the conductivity gap) is reduced by a factor of 2 when comparing the energy levels of an isolated molecule with those of a C 60 monolayer on Ag (111). Values taken from [13,21,[34][35][36][37][38][39] In the system depicted by Fig. 1c, the metal stabilizes the charged state of the C 60 -ion, since the metal effectively screens the ion.…”
Section: Introductionmentioning
confidence: 99%
“…27,28 The XPS spectrum, therefore, is made up of an intense peak from the original ejected photoelectron, and a number of peaks on the high binding energy side of the main peak due to the energy loss for excitation of …”
Section: Resultsmentioning
confidence: 99%
“…27,28 The XPS spectrum, therefore, is made up of an intense peak from the original ejected photoelectron, and a number of peaks on the high binding energy side of the main peak due to the energy loss for excitation of 32 all visible in the spectrum. (b) Molecular energy levels of C 60 (neglecting core hole ionization) (after Refs.…”
Section: Resultsmentioning
confidence: 99%