Please use this identifier to cite or link to this item: https://doi.org/10.1088/0953-8984/12/18/310
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dc.titleA superferromagnetic approach for rapidly quenched Y60Fe30Al10 alloys
dc.contributor.authorWang, L.
dc.contributor.authorDing, J.
dc.contributor.authorLi, Y.
dc.contributor.authorKong, H.Z.
dc.contributor.authorFeng, Y.P.
dc.contributor.authorWang, X.Z.
dc.date.accessioned2014-10-16T09:14:42Z
dc.date.available2014-10-16T09:14:42Z
dc.date.issued2000-05-08
dc.identifier.citationWang, L., Ding, J., Li, Y., Kong, H.Z., Feng, Y.P., Wang, X.Z. (2000-05-08). A superferromagnetic approach for rapidly quenched Y60Fe30Al10 alloys. Journal of Physics Condensed Matter 12 (18) : 4253-4262. ScholarBank@NUS Repository. https://doi.org/10.1088/0953-8984/12/18/310
dc.identifier.issn09538984
dc.identifier.urihttp://scholarbank.nus.edu.sg/handle/10635/95692
dc.description.abstractThe structural and magnetic properties of Y60Fe30Al10 melt-spun ribbons have been studied in this work. The experimental results indicate that Y60Fe30Al10 melt-spun ribbons are not homogeneous, i.e. Fe rich clusters are present. The magnetization curves for the ribbons melt spun at 5 and 30 m s-1 were analysed with a model based on superferromagnetism. It was found that this superferromagnetic model can be well applied to the ribbon melt spun at 30 m s-1. The Curie transition temperature TC system was confirmed by the plot of inverse susceptibility versus temperature. For the ribbon melt spun at 5 m s-1, inter-cluster interactions were much stronger and the microstructure was not uniform. Zero-field cooling and field cooling curves showed the cluster behaviour clearly. The Mössbauer results supported the existence of Fe rich clusters and interactions between clusters. © 2000 IOP Publishing Ltd.
dc.sourceScopus
dc.typeArticle
dc.contributor.departmentPHYSICS
dc.contributor.departmentMATERIALS SCIENCE
dc.description.doi10.1088/0953-8984/12/18/310
dc.description.sourcetitleJournal of Physics Condensed Matter
dc.description.volume12
dc.description.issue18
dc.description.page4253-4262
dc.description.codenJCOME
dc.identifier.isiut000087231700011
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