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Journal of the Magnetics Society of Japan
Article . 1995 . Peer-reviewed
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CURIE TEMPERATURE AND BAND STRUCTURE OF METALLIC FERROMAGNETS

Authors: R. SKOMSKI; X.-L. RAO; Q.-N. QI; J.M.D. COEY;

CURIE TEMPERATURE AND BAND STRUCTURE OF METALLIC FERROMAGNETS

Abstract

A soft-spin Heisenberg model is used to investigate the Curie temperature of elementary iron and iron-rich intermetallics such as Sm2Fe17. In the localized limit the mean-field solution of the classical Heisenberg model is reproduced, while quasi-localized perturbation theory accounts for band-structure effects. An extrapolation of this quasi-localized approach yields physically reasonable results, which makes it possible to interpolate between the delocalized band-structure and localized Heisenberg limits. Using Stoner-type magnetic energies derived from paramagnetic band-structure calculations it is argued that the comparatively low Curie temperature of iron-rich rare-earth intermetallics such as R2Fe17 originates from their quasi-weak ferromagnetism. Upon interstitial modification, these materials leave the quasi-weak limit and become nearly strong ferromagnets with enhanced Curie temperature.

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
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