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首页> 外文期刊>Physical Review, B. Condensed Matter >Spin-density waves and reorientation effects in thin epitaxial Cr films covered with ferromagnetic and paramagnetic layers
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Spin-density waves and reorientation effects in thin epitaxial Cr films covered with ferromagnetic and paramagnetic layers

机译:覆盖有铁磁和顺磁层的外延Cr薄膜中的自旋密度波和取向效应

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摘要

We report about synchrotron and neutron-scattering studies investigating incommensurate spin-density waves (I-SDW's) in epitaxially grown thin Cr(001) films, including surface and interface effects. These studies show that thin ferromagnetic cap layers of Fe, Ni, and Co with a thickness of only 2-3 nm have a strong effect on the propagation and orientation of the I-SDW's in Cr. For thick Cr films there exist essentially only transverse I-SDW's propagating parallel to the:film plane with the spins oriented normal to the planet and at right angles to the in-plane magnetization of the ferromagnetic cap layers. With decreasing Cr thickness a different transverse I-SDW grows at the expense of the in-plane ones, now propagating normal to the plane and with spins parallel or antiparallel to the film magnetization. At a Cr thickness of about 250 Angstrom, the transverse out-of-plane I-SDW completely dominates the phase diagram of Cr. All other domains are suppressed and a spin-flip transition does not occur above 10 K in strong contrast to bulk. For in-plane propagation of the T-SDW we find a coexisting commensurate spin-density wave (C-SDW) which vanishes during the reorientation to. out-of-plane propagation with Cr thickness. Finally,for Cr thicknesses well below the period of the I-SDW, the Cr can only order as a C-SDW. The behavior of the SDW's in thin Cr films with ferromagnetic cap layers can be understood in terms of competing interactions at the rough interfaces inducing frustration and by finite-size and strain effects. We have also investigated the effect of Cu and Pd cap layers on the SDW. The Cu cover is similar to a Cr/vacuum interface, whereas the effect of the Pd cover is intermediate between the ferromagnetic layers and Cu. [S0163-1829(99)11513-3]. [References: 63]
机译:我们报告同步子和中子散射研究调查外延生长的薄Cr(001)薄膜中不适当的自旋密度波(I-SDW),包括表面和界面效应。这些研究表明,厚度仅为2-3 nm的铁,镍和钴的薄铁磁盖层对I-SDW在Cr中的传播和取向有很大影响。对于厚铬膜,基本上只存在平行于膜平面的横向I-SDW,其自旋方向垂直于行星,并且与铁磁盖层的面内磁化强度成直角。随着Cr厚度的减小,不同的横向I-SDW以平面内的I-SDW为代价增长,现在垂直于平面传播,并且自旋平行于或反平行于薄膜磁化强度。在大约250埃的Cr厚度下,横向面外I-SDW完全占据了Cr的相图。与体积形成鲜明对比的是,所有其他域均被抑制,并且在10 K以上不会发生自旋翻转转变。对于T-SDW的面内传播,我们发现了一个共存的自旋密度波(C-SDW),在重新定向时消失。 Cr厚度的面外传播。最后,对于Cr厚度远低于I-SDW周期的Cr,Cr只能作为C-SDW订购。 SDW在具有铁磁帽盖层的Cr薄膜中的行为可以通过在粗糙界面上的竞争相互作用(导致挫败感)以及有限尺寸和应变效应来理解。我们还研究了铜和钯盖层对SDW的影响。 Cu覆盖层类似于Cr /真空界面,而Pd覆盖层的作用介于铁磁层和Cu之间。 [S0163-1829(99)11513-3]。 [参考:63]

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