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Magnetic interactions in strongly correlated systems: Spin and orbital contributions

机译:强相关系统中的磁相互作用:自旋和轨道贡献

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We present a technique to map an electronic model with local interactions (a generalized multi-orbital Hubbard model) onto an effective model of interacting classical spins, by requiring that the thermodynamic potentials associated to spin rotations in the two systems are equivalent up to second order in the rotation angles, when the electronic system is in a symmetry-broken phase. This allows to determine the parameters of relativistic and nonrelativistic magnetic interactions in the effective spin model in terms of equilibrium Green's functions of the electronic model. The Hamiltonian of the electronic system includes, in addition to the non-relativistic part, relativistic single-particle terms such as the Zeeman coupling to an external magnetic field, spin orbit coupling, and arbitrary magnetic anisotropies; the orbital degrees of freedom of the electrons are explicitly taken into account. We determine the complete relativistic exchange tensors, accounting for anisotropic exchange, Dzyaloshinskii-Moriya interactions, as well as additional non-diagonal symmetric terms (which may include-dipole dipole interaction). The expressions of all these magnetic interactions are determined in a unified framework, including previously disregarded features such as the vertices of two-particle Green's functions and non-local self-energies. We do not assume any smallness in spin-orbit coupling, so our treatment is in this sense exact. Finally, we show how to distinguish and address separately the spin, orbital and spin-orbital contributions to magnetism, providing expressions that can be computed within a tightbinding Dynamical Mean Field Theory. (C) 2015 Elsevier Inc. All rights reserved.
机译:通过要求与两个系统中的自旋旋转相关的热力学势能等于二阶,我们提出了一种将具有局部相互作用的电子模型(广义的多轨道哈伯德模型)​​映射到相互作用的经典自旋的有效模型上的技术当电子系统处于对称破缺状态时,在旋转角度上的变化。这允许根据电子模型的平衡格林函数来确定有效自旋模型中相对论和非相对论磁相互作用的参数。电子系统的哈密顿量除非相对论部分外,还包括相对论单粒子术语,例如与外部磁场的塞曼耦合,自旋轨道耦合和任意磁各向异性。明确考虑了电子的轨道自由度。我们确定了完整的相对论交换张量,其中考虑了各向异性交换,Dzyaloshinskii-Moriya相互作用以及其他非对角对称项(可能包括偶极子偶极子相互作用)。所有这些磁性相互作用的表达都在一个统一的框架中确定,包括以前忽略的特征,例如两粒子格林函数的顶点和非局部自能。我们不认为自旋轨道耦合有任何细微差别,因此在这种意义上我们的处理是精确的。最后,我们展示了如何区分和解决自旋,轨道和自旋轨道对磁性的贡献,提供了可以在紧密绑定的动力学平均场论中计算的表达式。 (C)2015 Elsevier Inc.保留所有权利。

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