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Modeling Giant Magnetoresistance and Relative Permeability in Granular Films

Published online by Cambridge University Press:  03 September 2012

M.R. Parker
Affiliation:
The University of Alabama, Department of Electrical Engineering
J.A. Barnard
Affiliation:
The University of Alabama, Department of metallurgical and Materials Engineering Tuscaloosa, AL 35487–0202
S. Hossain
Affiliation:
The University of Alabama, Department of Electrical Engineering
D. Seale
Affiliation:
The University of Alabama, Department of Electrical Engineering
M. Tan
Affiliation:
The University of Alabama, Department of metallurgical and Materials Engineering Tuscaloosa, AL 35487–0202
A. Waknis
Affiliation:
The University of Alabama, Department of metallurgical and Materials Engineering Tuscaloosa, AL 35487–0202
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Abstract

A Model for the field dependence of giant Magnetoresistance (GMR) in ‘granular’ co-sputtered alloy thin films (based on a relatively simple spin-dependent scattering concept appropriate to superparamagnetic and weakly ferromagnetic films) is applied to new experimental data from the Co90Fe10-Ag system. The Model and the experimental data can be shown to compare very well with the help of a single adjustable parameter related to spin correlation of adjacent Co-Fe clusters. A careful fit of field-dependent MR data and theory leads to a fairly reliable determination of spin-cluster radius. An analysis of the relative permeability of granular GMR films derived from the generalized form of the Clausius-Mossoti relationship is also presented. For a non-Magnetic Matrix the effective relative permeability is shown to be materials independent. The permeability model is applied to Co-Au granular films.

Type
Research Article
Copyright
Copyright © Materials Research Society 1993

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References

[1] Barnard, J.A., Waknis, A., Tan, M., Haftek, E., Parker, M.R., and Watson, M.L., J. Mag. Mag. Mat. 114, 203 (1992).Google Scholar
[2] Barnard, J.A., Hossain, S., Parker, M.R., Waknis, A., and Watson, M.L., J. Appl. Phys., in press.Google Scholar
[3] Watson, M.L., Barnard, J.A., Hossain, S., and Parker, M.R., J. Appl. Phys., in press.Google Scholar
[4] Berkowitz, A.E., Mitchell, J.R., Carey, M.J., Young, A.P., Zhang, S., Spada, F.E., Parker, F.T., Hutten, A., and Thomas, G., Phys. Rev. Lett. 68, 3745 (1992).Google Scholar
[5] Xiao, J.Q., Jiang, J.S., and Chien, C.L., Phys. Rev. Lett. 68, 3749 (1992).Google Scholar
[6] Jiang, J.S., Xiao, J.Q., and Chien, C.L., Appl. Phys. Lett. 61, 2362 (1992).Google Scholar
[7] Parker, M.R., Barnard, J.A., Seale, D., and Waknis, A., J. Appl. Phys., in press.Google Scholar
[8] Gittleman, J.L., Goldstein, Y., and Bozowski, S., Phys. Rev. B 5, 3609 (1972).Google Scholar
[9] Parker, M.R., National Storage Industry Consortium Report: Advanced Technology Program, 1993.Google Scholar
[10] Parker, M.R., Proc. 13th Intl. Colloquium on Magnetic Films and Surfaces, Glasgow, p. 119, (Aug. 1991).Google Scholar