Home > Publications database > Role of Spin-Orbit Coupling and Hybridization Effects in the Electronic Structure of Ultrathin Bi Films > print |
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017 | _ | _ | |a This version is available at the following Publisher URL: http://prl.aps.org |
024 | 7 | _ | |a 10.1103/PhysRevLett.97.146803 |2 DOI |
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024 | 7 | _ | |a 2128/1449 |2 Handle |
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084 | _ | _ | |2 WoS |a Physics, Multidisciplinary |
100 | 1 | _ | |a Hirahara, T. |b 0 |0 P:(DE-HGF)0 |
245 | _ | _ | |a Role of Spin-Orbit Coupling and Hybridization Effects in the Electronic Structure of Ultrathin Bi Films |
260 | _ | _ | |a College Park, Md. |b APS |c 2006 |
300 | _ | _ | |a 146803 |
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440 | _ | 0 | |a Physical Review Letters |x 0031-9007 |0 4925 |v 97 |
500 | _ | _ | |a Record converted from VDB: 12.11.2012 |
520 | _ | _ | |a The electronic structure of Bi(001) ultrathin films (thickness >= 7 bilayers) on Si(111)-7x7 was studied by angle-resolved photoemission spectroscopy and first-principles calculations. In contrast with the semimetallic nature of bulk Bi, both the experiment and theory demonstrate the metallic character of the films with the Fermi surface formed by spin-orbit-split surface states (SSs) showing little thickness dependence. Below the Fermi level, we clearly detected quantum well states (QWSs) at the M ($) over bar point, which were surprisingly found to be non-spin-orbit split; the films are "electronically symmetric" despite the obvious structural nonequivalence of the top and bottom interfaces. We found that the SSs hybridize with the QWSs near M ($) over bar and lose their spin-orbit-split character. |
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700 | 1 | _ | |a Chulkov, E. V. |b 4 |0 P:(DE-HGF)0 |
700 | 1 | _ | |a Koroteev, S. B. |b 5 |0 P:(DE-HGF)0 |
700 | 1 | _ | |a Echenique, P. M. |b 6 |0 P:(DE-HGF)0 |
700 | 1 | _ | |a Saito, M. |b 7 |0 P:(DE-HGF)0 |
700 | 1 | _ | |a Hasagawa, S. |b 8 |0 P:(DE-HGF)0 |
773 | _ | _ | |a 10.1103/PhysRevLett.97.146803 |g Vol. 97, p. 146803 |p 146803 |q 97<146803 |0 PERI:(DE-600)1472655-5 |t Physical review letters |v 97 |y 2006 |x 0031-9007 |
856 | 7 | _ | |u http://dx.doi.org/10.1103/PhysRevLett.97.146803 |u http://hdl.handle.net/2128/1449 |
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