1996
DOI: 10.1021/ja954237k
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Photoelectron Spectra, Ab Initio SCF MO, and Natural Bond Orbital Studies on Stellenes. Long-Range π/σ Interactions

Abstract: The He I photoelectron spectra of 2,6-dimethylenetricyclo[3.3.01,5.03,7]octane, (stella-2,6-diene) (6), stella-2,6-dione (8), stella-6-en-2-one (10), distella-2,2‘,6,6‘-triene (7), distella-6,6‘-en-2,2‘-dione (9), and distella-2,2‘,6‘-dien-6-one (11) have been recorded. The energy differences between the π ionizations arising from the terminal π bonds amount to 0.9 eV (6) and 0.4 eV (7). An energy difference of 1.1 eV has been found between the 2p lone-pair ionizations of 8. Using Hartree−Fock SCF calculations… Show more

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Cited by 26 publications
(42 citation statements)
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“…They confirm, in particular, the assignment proposed by Gleiter et al 84 for the three outermost and individually resolved ionization lines. On the experimental side, the first two lines (z, y) derived from orbitals 7b 2 and 6b 3 display asymmetric and sharp profiles, with rather clearly apparent vibrational progressions, which is very typical of -levels (see for instance the He I spectra displayed for a variety of polycyclic aromatic hydrocarbons in refs.…”
Section: Ionization Spectrum Of Stdesupporting
confidence: 89%
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“…They confirm, in particular, the assignment proposed by Gleiter et al 84 for the three outermost and individually resolved ionization lines. On the experimental side, the first two lines (z, y) derived from orbitals 7b 2 and 6b 3 display asymmetric and sharp profiles, with rather clearly apparent vibrational progressions, which is very typical of -levels (see for instance the He I spectra displayed for a variety of polycyclic aromatic hydrocarbons in refs.…”
Section: Ionization Spectrum Of Stdesupporting
confidence: 89%
“…The next three levels (u, t, s) very strongly overlap, and lead to a broad and intense band (A) that culminates at *11.9 eV, in quantitative agreement with the He I measurements by Gleiter et al 84 As the simulation of Figure 3b clearly demonstrates, any attempt to analyze separately the ionization intensities characterizing these three orbitals should be regarded as physically irrelevant, with regard to the limited resolution of the currently available spectrometers and the extent of vibrational broadening. Analysis of the bands recorded at binding energies around *12.5 eV is problematic, because of the presence at these binding energies of a rather intense signal, which Gleiter et al 84 ascribed to water contamination. Without this experimental artefact, the line (q) related to orbital 5b 1 should have normally been individually identified in a He I spectrum.…”
Section: Ionization Spectrum Of Stdesupporting
confidence: 88%
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