% IMPORTANT: The following is UTF-8 encoded. This means that in the presence
% of non-ASCII characters, it will not work with BibTeX 0.99 or older.
% Instead, you should use an up-to-date BibTeX implementation like “bibtex8” or
% “biber”.
@ARTICLE{Krupin:5501,
author = {Krupin, O. and Bihlmayer, G. and Döbrich, K. and Prieto,
J. E. and Starke, K. and Gorovikov, S. and Blügel, S. and
Kevan, S. and Kaindl, G.},
title = {{R}ashba effect at the surfaces of rare-earth metals and
their monoxides},
journal = {New journal of physics},
volume = {11},
issn = {1367-2630},
address = {[Bad Honnef]},
publisher = {Dt. Physikalische Ges.},
reportid = {PreJuSER-5501},
pages = {013035},
year = {2009},
note = {Financial support through Deutsche Forschungsgemeinschaft,
projects STA 413/3-1, BI 823-1/1 and SfB-290) TP6, is
gratefully acknowledged. This work was also supported by the
US DOE under grant DE-FG02-04ER46158. The Advanced Light
Source is operated under US DOE contract DE-AC03-76SF00098
at Lawrence Berkeley National Laboratory. JEP acknowledges
financial support by the A-v Humboldt foundation and by the
MEC program 'Ramon y Cajal'. We gratefully acknowledge
Christian Schubler-Langeheine for designing and setting up
the photoemission endstation used during the experiments at
BessyII.},
abstract = {We present a systematic study of the Rashba-type spin-orbit
interaction at the (0001) surfaces of rare-earth metals and
their surface monoxides, specifically of Tb metal and the
O/Tb, O/Lu and O/Y surfaces. By means of photoemission
experiments and ab initio band-structure calculations, we
uncover the influence of this interaction on the surface
electronic structure. In turn, the dramatic impact of the
charge-density distribution of the surface/interface states
on the strength of the Rashba-type spin splitting is
demonstrated. We discuss the Rashba effect at magnetic and
non-magnetic rare-earth surfaces, and compare with cases
where it is negligible. The difference between the Rashba
effect and magnetic linear dichroism in photoemission is
pointed out to help avoid possible confusion in connection
with the simultaneous appearance of these two effects at a
magnetic surface.},
keywords = {J (WoSType)},
cin = {IAS-1 / IFF-1 / JARA-FIT / JARA-HPC},
ddc = {530},
cid = {I:(DE-Juel1)IAS-1-20090406 / I:(DE-Juel1)VDB781 /
$I:(DE-82)080009_20140620$ / $I:(DE-82)080012_20140620$},
pnm = {Grundlagen für zukünftige Informationstechnologien},
pid = {G:(DE-Juel1)FUEK412},
shelfmark = {Physics, Multidisciplinary},
typ = {PUB:(DE-HGF)16},
UT = {WOS:000262932800001},
doi = {10.1088/1367-2630/11/1/013035},
url = {https://juser.fz-juelich.de/record/5501},
}