2010
DOI: 10.1063/1.3319778
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Valence ionized states of iron pentacarbonyl and η5-cyclopentadienyl cobalt dicarbonyl studied by symmetry-adapted cluster-configuration interaction calculation and collision-energy resolved Penning ionization electron spectroscopy

Abstract: Valence ionized states of iron pentacarbonyl Fe(CO)(5) and eta(5)-cyclopentadienyl cobalt dicarbonyl Co(eta(5)-C(5)H(5))(CO)(2) have been studied by ultraviolet photoelectron spectroscopy, two-dimensional Penning ionization electron spectroscopy (2D-PIES), and symmetry-adapted cluster-configuration interaction calculations. Theory provided reliable assignments for the complex ionization spectra of these molecules, which have metal-carbonyl bonds. Theoretical ionization energies agreed well with experimental ob… Show more

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Cited by 11 publications
(13 citation statements)
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“…This indicates a smaller fraction of the Auger contributions to bands B and C. The overlap of the continuum wavefunctions, ρ α 2 , is also considerably smaller in bands B and C than in band A. In their quantum chemistry calculations, Fukuda et al 3 estimated the Fe-character of the 10e to be 77%. We use this value to calibrate the relative A α values to the Fecharacter and include the values in Table I.…”
Section: Discussionmentioning
confidence: 93%
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“…This indicates a smaller fraction of the Auger contributions to bands B and C. The overlap of the continuum wavefunctions, ρ α 2 , is also considerably smaller in bands B and C than in band A. In their quantum chemistry calculations, Fukuda et al 3 estimated the Fe-character of the 10e to be 77%. We use this value to calibrate the relative A α values to the Fecharacter and include the values in Table I.…”
Section: Discussionmentioning
confidence: 93%
“…The features between 8.5 and 10.5 eV (band A) are attributed to the 10e and 3e molecular orbitals, which are principally Fe 3d in character. 3,5 The photolines above 14 eV are typically attributed to the ligands. 5,2, 3 Baerends et al 2 and Fukuda et al 3 assigned the photolines between 13 and 17 eV (band B) to the CO(5σ ) and CO(1π ) orbitals, and those from 17 and 20 eV (band C) to the CO(4σ ) orbital.…”
Section: Resultsmentioning
confidence: 99%
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