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dc.contributor.authorBance, S
dc.contributor.authorOezelt, H
dc.contributor.authorSchrefl, T
dc.contributor.authorCiuta, G
dc.contributor.authorDempsey, NM
dc.contributor.authorGivord, D
dc.contributor.authorWinklhofer, M
dc.contributor.authorHrkac, G
dc.contributor.authorZimanyi, G
dc.contributor.authorGutfleisch, O
dc.contributor.authorWoodcock, TG
dc.contributor.authorShoji, T
dc.contributor.authorYano, M
dc.contributor.authorKato, A
dc.contributor.authorManabe, A
dc.date.accessioned2016-04-27T12:53:58Z
dc.date.issued2014-05-09
dc.description.abstractThe coercive field and angular dependence of the coercive field of single-grain Nd$_{2}$Fe$_{14}$B permanent magnets are computed using finite element micromagnetics. It is shown that the thickness of surface defects plays a critical role in determining the reversal process. For small defect thicknesses reversal is heavily driven by nucleation, whereas with increasing defect thickness domain wall de-pinning becomes more important. This change results in an observable shift between two well-known behavioral models. A similar trend is observed in experimental measurements of bulk samples, where a Nd-Cu infiltration process has been used to enhance coercivity by modifying the grain boundaries. When account is taken of the imperfect grain alignment of real magnets, the single-grain computed results appears to closely match experimental behaviour.en_GB
dc.description.sponsorshipWe acknowledge the financial support from the Technology Research Association of Magnetic Materials for High Efficient Motors (MagHEM).en_GB
dc.identifier.citationVol. 104 (18), article 182408en_GB
dc.identifier.doi10.1063/1.4876451
dc.identifier.urihttp://hdl.handle.net/10871/21281
dc.language.isoenen_GB
dc.publisherAmerican Institute of Physics (AIP)en_GB
dc.subjectCoercive forceen_GB
dc.subjectDomain wallsen_GB
dc.subjectNucleationen_GB
dc.subjectMagnetsen_GB
dc.subjectInfiltrationen_GB
dc.titleInfluence of defect thickness on the angular dependence of coercivity in rare-earth permanent magnetsen_GB
dc.typeArticleen_GB
dc.date.available2016-04-27T12:53:58Z
dc.descriptionThis is the final version of the article. Available from the American Institute of Physics via the DOI in this record.en_GB
dc.identifier.journalApplied Physics Lettersen_GB


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