Electronic and crystal structure of the Pt(111)-(√3 × √3)R30°-K system

•Electronic structure of the Pt(111)-(√3 × √3)R30°-K surface is theoretically studied.•The K adsorption modifies the Shockley state of Pt(111) into the K localized state.•The Rashba spin-orbit coupling parameter of this state is surprisingly large.•Its value is greater than that of the Shockley stat...

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Veröffentlicht in:Surface science 2018-12, Vol.678, p.99-105
Hauptverfasser: Koroteev, Yu.M., Chulkov, E.V.
Format: Artikel
Sprache:eng
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Zusammenfassung:•Electronic structure of the Pt(111)-(√3 × √3)R30°-K surface is theoretically studied.•The K adsorption modifies the Shockley state of Pt(111) into the K localized state.•The Rashba spin-orbit coupling parameter of this state is surprisingly large.•Its value is greater than that of the Shockley state on Au(111) and Bi(111).•The K adsorption gives rise to new surface states on the Pt substrate. We present the density functional calculation results for K adsorption on Pt(111) in a (√3 × √3)R30° structure. The site preference, surface relaxation, work function, and electron structure of the system are analyzed. The hcp hollow position is found to be the most favorable for K adsorption. The calculated surface relaxations and adsorption geometry are in agreement with available experimental data. It is demonstrated that the K adsorption leads to the disappearance of a number of platinum surface and resonance states in the energy region above −2 eV and to the appearance of new platinum surface features, as well as bands that are significantly localized at the adsorbate. It is found that the K adsorption 1) transforms the Shockley surface state lying in the bulk band gap near the Γ¯ point on the clean Pt surface into the state localized at the K adlayer and 2) pushes this state up in energy by about 0.17 eV relative to the bottom of the bulk band gap. It is shown that the Rashba spin-orbit strength parameter in this state is surprisingly greater than the respective parameter in the Shockley surface state on Au(111) and Bi(111). [Display omitted]
ISSN:0039-6028
1879-2758
DOI:10.1016/j.susc.2018.04.007