001     43289
005     20200423204004.0
017 _ _ |a This version is available at the following Publisher URL: http://prl.aps.org
024 7 _ |2 DOI
|a 10.1103/PhysRevLett.92.046801
024 7 _ |2 WOS
|a WOS:000188747600039
024 7 _ |2 Handle
|a 2128/1403
024 7 _ |a altmetric:21813003
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037 _ _ |a PreJuSER-43289
041 _ _ |a eng
082 _ _ |a 550
084 _ _ |2 WoS
|a Physics, Multidisciplinary
100 1 _ |0 P:(DE-HGF)0
|a von Bergmann, K.
|b 0
245 _ _ |a Spin-Polarized Electron Scattering at Single Oxygen Adsorbates on a Magnetic Surface
260 _ _ |a College Park, Md.
|b APS
|c 2004
300 _ _ |a 046801
336 7 _ |a Journal Article
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336 7 _ |a ARTICLE
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336 7 _ |a JOURNAL_ARTICLE
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336 7 _ |a article
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400 1 _ |a Bergmann, K.
440 _ 0 |0 4925
|a Physical Review Letters
|v 92
|x 0031-9007
|y 4
500 _ _ |a Record converted from VDB: 12.11.2012
520 _ _ |a Scanning tunneling spectroscopy (STS) on the system of isolated oxygen atoms adsorbed on the double layer of Fe on W(110) shows highly anisotropic spatial oscillations in the local density of states in the vicinity of the adsorbates. We explain this in terms of a single-particle model as electron waves being scattered by the potential induced by the presence of the oxygen atoms. Analysis of the wavelength of the standing electron waves and comparison with ab initio spin-resolved electronic structure calculations reveal that minority-spin bands of d-like symmetry are involved in the scattering process. By applying spin-polarized STS, we observe this standing wave pattern on one particular type of magnetic domain of Fe on W(110) only, thereby proving that the standing electron waves are highly spin polarized.
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700 1 _ |0 P:(DE-HGF)0
|a Bode, M.
|b 1
700 1 _ |0 P:(DE-HGF)0
|a Kubetzka, A.
|b 2
700 1 _ |0 P:(DE-Juel1)VDB3766
|a Heide, M.
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700 1 _ |0 P:(DE-Juel1)130548
|a Blügel, S.
|b 4
|u FZJ
700 1 _ |0 P:(DE-HGF)0
|a Wiesendanger, R.
|b 5
773 _ _ |0 PERI:(DE-600)1472655-5
|a 10.1103/PhysRevLett.92.046801
|g Vol. 92, p. 046801
|p 046801
|q 92<046801
|t Physical review letters
|v 92
|x 0031-9007
|y 2004
856 7 _ |u http://dx.doi.org/10.1103/PhysRevLett.92.046801
|u http://hdl.handle.net/2128/1403
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