Holographic Observation of Magnetic Fine-Structures in New Magnetic Materials

Holographic Observation of Magnetic Fine-Structures in New Magnetic Materials
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新型磁性材料中磁性精细结构的全息观察

DOI:
10.1017/s1431927602101371
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发表时间:
2002
影响因子:
2.8
通讯作者:
T. Suzuki
T. Suzuki
中科院分区:
工程技术4区
文献类型:
--
作者:
T. Tanji;S. Hasebe;T. Suzuki

文献摘要

被引文献

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用电子全息术观察到了新的磁性材料,金属多层膜(Co/Cu)和颗粒膜(Fe-Zr)。巨磁电阻效应(GMR)是由于导电电子的自旋相关散射引起的,这种散射是由于相邻铁磁层之间通过磁性间隔层(多层膜)或磁性基质中相邻铁磁颗粒之间的磁耦合(颗粒膜)引起的。然而,到目前为止,这种耦合的直接观察几乎没有报道。
New magnetic materials, metal multilayers (Co/Cu) and granular films (Fe-Zr), have been observed by electron holography. Giant magnetoresistance (GMR) is attributed to the spin-dependent scattering of conduction electrons, which arises from the magnetic coupling between each adjacent ferromagnetic layers through a nonmagnetic spacer layer (multilayers), or between neighboring ferromagnetic particles in nonmagnetic matrix (granular films). Direct observation of such a coupling, however, has hardly been reported so far.