2002
DOI: 10.1103/physrevb.66.134427
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Oxygen adsorption on Fe/W(110) and Co/W(110) thin films: Surface magnetic properties

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Cited by 29 publications
(22 citation statements)
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References 33 publications
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“…2 are also displayed. Our UPS spectra for CoO agree well with those for CoO(100), 8 CoO films on Au(111) 9 and CoO films on Au(001). 11 The energy positions of the UPS structures seen for CoO agree well with those seen for NiO, and are very close to A-E.…”
Section: Oxygen Interaction With Co Filmssupporting
confidence: 84%
“…2 are also displayed. Our UPS spectra for CoO agree well with those for CoO(100), 8 CoO films on Au(111) 9 and CoO films on Au(001). 11 The energy positions of the UPS structures seen for CoO agree well with those seen for NiO, and are very close to A-E.…”
Section: Oxygen Interaction With Co Filmssupporting
confidence: 84%
“…A positive asymmetry indicates that minority electrons dominate in the surface vacuum region of the clusters, agreeing with SPMDS studies of thin Fe films [8]- [10]. High positive asymmetries have been reported before for thin Fe films on various substrates including GaAs (15 %) [8], MgO(100) (9 %) [9], Ag(100) (6 %) [9], and W(110) (24 %) [7]. However, these values are not directly comparable to the asymmetry reported here for a number of reasons.…”
Section: Resultssupporting
confidence: 68%
“…3 (a) at ~14 eV is due to both electrons involved in the AN transition originating from the Fermi level, E F . The shoulder just below E F (corresponding to binding energies of a few eV) is due to emission from surface states of the Si(111) 7x7 reconstruction [4] and also Fe 3d electrons [7]. The shoulder at ~10.5 eV arises from emission of Si atomic 3p states found at the surface and in the bulk, and at low kinetic energies emission is dominated by true secondary electrons.…”
Section: Resultsmentioning
confidence: 99%
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“…The surface spin polarization shows characteristic behaviors at low oxygen exposures, 4-8 but it decreases with exposure Ͼ10 L ͑Refs. 5-8͒ and almost disappears at Ͼ50 L. 7,8 This however looks somewhat strange considering the fact that there are stable ferromagnetic Fe oxides ͑Fe 3 O 4 , ␥-Fe 2 O 3 ͒. Actually, a number of studies have indicated the formation of Fe 3 O 4 by room temperature oxidation for O 2 exposures Ͼ10 L. 9,10 In the present letter, we report a high negative spin polarization observed for the topmost surface of an Fe͑001͒/ MgO͑100͒ film oxidized at room temperature.…”
mentioning
confidence: 96%