Strong anisotropies in MBE-grown Co/Cr(001): Ferromagnetic-resonance and magneto-optical Kerr-effect studies

Ferromagnetic-resonance (FMR) and magneto-optical Kerr-effect (MOKE) studies of molecular-beam-epitaxy grown Co/Cr(001) superlattices and single layers are presented. The FMR measurements were performed in different sample orientations and in a broad frequency range (9-92 GHz). Magneto-optical Kerr-...

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Veröffentlicht in:Physical review. B, Condensed matter Condensed matter, 1995-02, Vol.51 (5), p.2920-2929
Hauptverfasser: Schreiber, F, Frait, Z, Zeidler, T, Metoki, N, Donner, W, Zabel, H, Pelzl, J
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Sprache:eng
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Zusammenfassung:Ferromagnetic-resonance (FMR) and magneto-optical Kerr-effect (MOKE) studies of molecular-beam-epitaxy grown Co/Cr(001) superlattices and single layers are presented. The FMR measurements were performed in different sample orientations and in a broad frequency range (9-92 GHz). Magneto-optical Kerr-effect hysteresis loops were detected in polar and in longitudinal configuration. The in-plane anisotropy parameters, K sub 1 and K sub 2 , the out-of-plane anisotropy (i.e. the effective magnetization including the surface anisotropy, K sub s ), and the g factor were determined for these samples, which exhibit an anomalous out-of-plane lattice expansion of the hcp Co(1120) on bcc Cr(001) as a precursor of a structural phase transition. Due to the strong in-plane anisotropy the switching of the magnetization to out-of-plane easy axis can occur at lower thicknesses (approx14 A) than the change of sign of the effective magnetization (approx21 A). In the intermediate thickness range a peculiar situation can be found with the orientation of the magnetization along the surface normal lying energetically between the in-plane easy and hard axis. Taking into account these effects and a reduced magnetic moment, K sub s approx0.76 erg/cm exp 2 is found. For thin Co layers the g factor is found to be increased in comparison with the bulk value. This indicates modifications of the electronic properties accompanied with the considerable structural changes.
ISSN:0163-1829
1095-3795
DOI:10.1103/PhysRevB.51.2920