| Hauptseite > Publikationsdatenbank > Enhanced Rashba spin-orbit splitting in Bi/Ag(111) and Pb/Ag(111) surface alloys from first principles > print |
| 001 | 56541 | ||
| 005 | 20230426083228.0 | ||
| 024 | 7 | _ | |a 10.1103/PhysRevB.75.195414 |2 DOI |
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| 084 | _ | _ | |2 WoS |a Physics, Condensed Matter |
| 100 | 1 | _ | |a Bihlmayer, G. |b 0 |u FZJ |0 P:(DE-Juel1)130545 |
| 245 | _ | _ | |a Enhanced Rashba spin-orbit splitting in Bi/Ag(111) and Pb/Ag(111) surface alloys from first principles |
| 260 | _ | _ | |a College Park, Md. |b APS |c 2007 |
| 300 | _ | _ | |a 195414 |
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| 440 | _ | 0 | |a Physical Review B |x 1098-0121 |0 4919 |v 75 |
| 500 | _ | _ | |a Record converted from VDB: 12.11.2012 |
| 520 | _ | _ | |a We present first-principles calculations of a (root 3x root 3) R30 degrees Bi/Ag (111)-ordered surface alloy, which has recently been investigated experimentally using angle-resolved photoemission spectroscopy. The surface states in the L-projected bulk band gap show a Rashba-type spin-orbit splitting which is three times larger than what has been observed on a clean Bi (111) surface. This large enhancement can be explained by the strong distortion of the surface-state wave function which is caused by the substantial outward buckling of the Bi atom. Also, in a similar surface alloy, Pb/Ag (111), a strong Rashba-type splitting was found by our calculations. The comparison to the experimental data is more difficult due to the presence of a second, close-by surface state. We discuss the dependence of the two-dimensional band structure on the surface corrugation and compare to the experimental findings. |
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| 700 | 1 | _ | |a Chulkov, E. V. |b 2 |0 P:(DE-HGF)0 |
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| 856 | 7 | _ | |u http://dx.doi.org/10.1103/PhysRevB.75.195414 |
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