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dc.contributor.authorGřondilová, Jana
dc.contributor.authorRickart, M.
dc.contributor.authorMistrík, Jan
dc.contributor.authorPostava, Kamil
dc.contributor.authorVišňovský, Štefan
dc.contributor.authorLopušník, Radek
dc.contributor.authorDemokritov, S.O.
dc.contributor.authorHillebrands, B.
dc.date.accessioned2007-06-29T13:02:23Z
dc.date.available2007-06-29T13:02:23Z
dc.date.issued2002
dc.identifier.citationJournal of Applied Physics. 2002, vol. 91, issue 10, p. 8246-8248.en
dc.identifier.issn0021-8979
dc.identifier.issn1089-7550
dc.identifier.urihttp://hdl.handle.net/10084/60823
dc.language.isoenen
dc.publisherAmerican Institute of Physicsen
dc.relation.ispartofseriesJournal of Applied Physicsen
dc.relation.urihttps://doi.org/10.1063/1.1452224en
dc.titleAnisotropy of magneto-optical spectra in ultrathin Fe/Au/Fe bilayersen
dc.typearticleen
dc.identifier.locationNení ve fondu ÚKen
dc.description.abstract-enMolecular beam epitaxy grown Au(5 nm)/Fe(1.1 nm)/Au(t)/Fe(1.1 nm)/Au(100 nm)/Fe(1 nm)/MgO(001) structures with t between 1 and 2.5 nm were the subject of optical and magneto-optical (MO) ellipsometry studies at photon energies between 1.5 and 5.4 eV. Both the optical ellipsometry and MO polar Kerr rotation spectra can be explained with a multilayer model based on the bulk optical and MO data for Fe and Au. However, the longitudinal MO Kerr effect spectra depart from the model prediction showing an additional well-resolved structure between 3 and 4 eV. This demonstrates a stronger effect of interfaces on the electronic properties at in-plane magnetization in ultrathin magnetic films. On a macroscopic level the effect can be accounted for by a reduced symmetry of the linear MO tensor.en
dc.identifier.doi10.1063/1.1452224
dc.identifier.wos000175576400140


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