Home > Publications database > Strong spin-orbit fields and Dyakonov-Perel spin dephasing in supported metallic films > print |
001 | 824918 | ||
005 | 20230426083140.0 | ||
024 | 7 | _ | |a 10.1103/PhysRevB.94.180406 |2 doi |
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024 | 7 | _ | |a 2469-9950 |2 ISSN |
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100 | 1 | _ | |a Long, Nguyen Hoang |0 P:(DE-Juel1)143632 |b 0 |e Corresponding author |u fzj |
245 | _ | _ | |a Strong spin-orbit fields and Dyakonov-Perel spin dephasing in supported metallic films |
260 | _ | _ | |a Woodbury, NY |c 2016 |b Inst. |
336 | 7 | _ | |a article |2 DRIVER |
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520 | _ | _ | |a Spin dephasing by the Dyakonov-Perel mechanism in metallic films deposited on insulating substrates is revealed, and quantitatively examined by means of density functional calculations combined with a kinetic equation. The surface-to-substrate asymmetry, probed by the metal wave functions in thin films, is found to produce strong spin-orbit fields and a fast Larmor precession, giving a dominant contribution to spin decay over the Elliott-Yafet spin relaxation up to a thickness of 70 nm. The spin dephasing is oscillatory in time with a rapid (subpicosecond) initial decay. However, parts of the Fermi surface act as spin traps, causing a persistent tail signal lasting 1000 times longer than the initial decay time. It is also found that the decay depends on the direction of the initial spin polarization, resulting in a spin-dephasing anisotropy of 200% in the examined cases. |
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700 | 1 | _ | |a Bauer, David |0 P:(DE-Juel1)130526 |b 2 |
700 | 1 | _ | |a Zimmermann, Bernd |0 P:(DE-Juel1)131065 |b 3 |u fzj |
700 | 1 | _ | |a Mokrousov, Yuriy |0 P:(DE-Juel1)130848 |b 4 |u fzj |
700 | 1 | _ | |a Blügel, Stefan |0 P:(DE-Juel1)130548 |b 5 |u fzj |
773 | 1 | 8 | |a 10.1103/physrevb.94.180406 |b American Physical Society (APS) |d 2016-11-22 |n 18 |p 180406 |3 journal-article |2 Crossref |t Physical Review B |v 94 |y 2016 |x 2469-9950 |
773 | _ | _ | |a 10.1103/PhysRevB.94.180406 |g Vol. 94, no. 18, p. 180406 |0 PERI:(DE-600)2844160-6 |n 18 |p 180406 |t Physical review / B |v 94 |y 2016 |x 2469-9950 |
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