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核壳纳米颗粒中壳层驱动的磁稳定性

Shell-driven magnetic stability in core-shell nanoparticles.

作者信息

Nogués J, Skumryev V, Sort J, Stoyanov S, Givord D

机构信息

Institució Catalana de Recerca i Estudis Avançats and Departament de Física, Universitat Autònoma de Barcelona, 08193 Bellaterra, Barcelona, Spain.

出版信息

Phys Rev Lett. 2006 Oct 13;97(15):157203. doi: 10.1103/PhysRevLett.97.157203.

Abstract

The magnetic properties of ferromagnetic-antiferromagnetic Co-CoO core-shell nanoparticles are investigated as a function of the in-plane coverage density from 3.5% to 15%. The superparamagnetic blocking temperature, the coercivity, and the bias field radically increase with increasing coverage. This behavior cannot be attributed to the overall interactions between cores. Rather, it can be semiquantitatively understood by assuming that the shells of isolated core-shell nanoparticles have strongly degraded magnetic properties, which are rapidly recovered as nanoparticles come into contact.

摘要

研究了铁磁-反铁磁Co-CoO核壳纳米颗粒的磁性与面内覆盖密度(从3.5%到15%)之间的函数关系。超顺磁阻塞温度、矫顽力和偏置场随覆盖度的增加而急剧增加。这种行为不能归因于核之间的整体相互作用。相反,通过假设孤立核壳纳米颗粒的壳层具有严重退化的磁性,而当纳米颗粒相互接触时磁性会迅速恢复,可以对这种行为进行半定量理解。

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