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Microscopic origin of subthermal magnons and the spin Seebeck effect

机译:亚热磁振子的微观起源和自旋塞贝克效应

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Recent experimental evidence points to low-energy magnons as the primary contributors to the spin Seebeck effect. This spectral dependence is puzzling since it is not observed on other thermocurrents in the same material. Here, we argue that the physical origin of this behavior is the magnon–magnon scattering mediated by phonons, in a process which conserves the number of magnons. To assess the importance and features of this kind of scattering, we derive the effective magnon–phonon interaction from a microscopic model, including band energy, a screened electron–electron interaction and the electron–phonon interaction. Unlike higher order magnon-only scattering, we find that the coupling with phonons induce a scattering which is very small for low-energy (or subthermal) magnons but increases sharply above a certain energy—rendering magnons above this energy poor spin-current transporters.
机译:最近的实验证据表明,低能磁振子是自旋塞贝克效应的主要贡献者。这种光谱依赖性令人困惑,因为在同一材料中的其他热电流上没有观察到这种依赖性。在这里,我们认为,这种行为的物理起源是声子介导的马农-马农散射,在此过程中可以节省马农的数量。为了评估这种散射的重要性和特征,我们从微观模型中得出了有效的磁振子-声子相互作用,包括能带,已筛选的电子-电子相互作用和电子-声子相互作用。与仅使用高阶磁振子的散射不同,我们发现,与声子的耦合会引起散射,对于低能(或亚热)磁振子,散射很小,但在特定能量之上会急剧增加,使磁振子在这种能量贫乏的自旋电流输运体之上产生。

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