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Materials for high-performance permanent magnets must have a high Curie temperature, a large spontaneous magnetization and strong uniaxial magnetocrystalline anisotropy. Binary rare earth iron intermetallics are deficient in one or more of these respects. New series of rare-earth intermetallic compounds may be generated from existing series by a process known as gas-phase interstitial modification, whereby interstitial atoms such as nitrogen or carbon are introduced into the structure by reaction of a powder of the intermetallic with an appropriate gas. The interstitials occupy sites adjacent to the rare earth, thereby creating a crystal field that reflects the new local symmetry. They also expand the lattice, which greatly enhances the Fe-Fe exchange interactions, and may increase slightly the iron moment. These effects are discussed in detail for four systems, R 2 Fe 17 N 3-δ , R 2 Fe 17 C 3-δ R(Fe 11 Ti)N 1-δ and R(Fe 11 Ti)C 1-δ (R = rare earth), all of which include compounds with potential for making new parmanent magnets.
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J. M. D. Coey (1991) studied this question.
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