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Thickness dependence of linear and quadratic magneto-optical Kerr effect in ultrathin Fe(001) films

Authors :
Buchmeier, M.
Schreiber, R.
Bürgler, D. E.
Schneider, C. M.
Source :
Phys. Rev. B 79, 064402 (2009)
Publication Year :
2008

Abstract

Magneto-optical Kerr effect (MOKE) magnetometry is one of the most widely employed techniques for the characterization of ferromagnetic thin-film samples. Some information, such as coercive fields or anisotropy strengths can be obtained without any knowledge of the optical and magneto-optical (MO) properties of the material. On the other hand, a quantitative analysis, which requires a precise knowledge of the material's index of refraction n and the MO coupling constants K and G is often desirable, for instance for the comparison of samples, which are different with respect to ferromagnetic layer thicknesses, substrates, or capping layers. While the values of the parameters n and the linear MO coupling parameter K reported by different authors usually vary considerably, the relevant quadratic MO coupling parameters G of Fe are completely unknown. Here, we report on measurements of the thickness dependence (0-60nm) of the linear and quadratic MOKE in epitaxial bcc-Fe(001) wedge-type samples performed at a commonly used laser wavelength of 670nm. By fitting the thickness dependence we are able to extract a complete set of parameters n, K, (G11 - G12), and G44 for the quantitative description of the MOKE of bcc-Fe(001). We find sizable different n, K, and G parameters for films thinner than about 10nm as compared to thicker films, which is indicative of a thickness dependence of the electronic properties or of surface contributions to the MOKE. The effect size of the quadratic MOKE is found to be about a third of the record values recently reported for Co2FeSi.<br />Comment: 8 pages, 5 figures

Details

Database :
arXiv
Journal :
Phys. Rev. B 79, 064402 (2009)
Publication Type :
Report
Accession number :
edsarx.0803.1599
Document Type :
Working Paper
Full Text :
https://doi.org/10.1103/PhysRevB.79.064402