1996
DOI: 10.1016/s0921-5093(96)10302-6
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Band gaps of doped and undoped films of molecular icosahedra

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Cited by 35 publications
(62 citation statements)
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“…Combined photoemission and inverse photoemission were undertaken to study the molecular orbital placement of both occupied and unoccupied orbitals of the adsorbed molecules on Au(111) surfaces. All inverse photoemission (IPES) spectra were obtained with the electron gun at normal incidence and the detector positioned at 45° off the surface normal, as described elsewhere [8,9]. Both high resolution and angle-resolved photoemission studies were undertaken.…”
Section: Methodsmentioning
confidence: 99%
“…Combined photoemission and inverse photoemission were undertaken to study the molecular orbital placement of both occupied and unoccupied orbitals of the adsorbed molecules on Au(111) surfaces. All inverse photoemission (IPES) spectra were obtained with the electron gun at normal incidence and the detector positioned at 45° off the surface normal, as described elsewhere [8,9]. Both high resolution and angle-resolved photoemission studies were undertaken.…”
Section: Methodsmentioning
confidence: 99%
“…The evidence for metallic mercury, from the Hg 5d 5/2 core level widths does not suggest that mercury atoms may form a lattice which weakly interacts with orthocarborane lattice, or Hg may form a wetting surfactant layer and a layer between the Cu substrate and orthocarborane molecular fi lm which would easily explain a uniform shift in the molecular orbital photoemission binding energies. In this regard, Hg is very different from the more homo geneous mixtures formed with some metals and molecularly chemisorbed species [14][15][16][38][39][40][41][42][43][44][45][46][47][48][49].…”
Section: Figurementioning
confidence: 98%
“…Following the adsorption of closo-1,2-dicarbadodecaborane, C 2 B 10 ·H 12 (orthocarborane) on Cu(100)at 180 K, the highest occupied molecular orbital (HOMO) appears in the pho toemission spectra at an initial binding energy of 5.7 eV below the Fermi level, while the lowest unoccupied molecular orbital (LUMO) is observed at roughly 4.25 eV with respect to the Fermi level (E − E F ) [14,15,33]. This HOMO-LUMO gap is generally consistent with theory [14][15][16]33].…”
Section: Mercury Interactions With Molecular Carborane Fi Lmsmentioning
confidence: 99%
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