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 |
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Format: | Artikel |
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. |
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ISSN: | 0163-1829 1095-3795 |
DOI: | 10.1103/PhysRevB.51.2920 |