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The role of next-nearest neighbours for the existence conditions of subsurface spin waves in magnetic films

机译:次近邻在磁性膜中地下自旋波存在条件中的作用

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摘要

Spin-wave energies and respective band structures throughout the two-dimensional Brillouin zone are investigated in magnetic (cubic) thin films for the surface orientations sc(110), bcc(110) and fcc(110). We apply the Heisenberg localized spin model assuming exchange nearest (NN) and next-nearest (NNN) neighbour interactions and elucidate the role of the geometrical disposition of the NN and NNN neighbourhoods for the emergence of surface (SSW) and subsurface spin waves (SSSW). The necessary condition for the emergence of SSSW is found to require the NNN bonds to be cut at the surface obliquely thereto. [References: 11]
机译:研究了在磁性(立方)薄膜中表面取向sc(110),bcc(110)和fcc(110)的整个二维布里渊区的自旋波能量和各自的能带结构。我们应用海森堡局部自旋模型,假设交换最近(NN)和近邻(NNN)邻居相互作用,并阐明了NN和NNN邻域的几何布置对于表面(SSW)和地下自旋波(SSSW)的出现的作用)。发现SSSW出现的必要条件要求在倾斜的表面上切断NNN键。 [参考:11]

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