Technische Universität Berlin , Institut für Chemie, Theoretische Chemie , Sekr. C7, Strasse des 17. Juni 135 , 10623 Berlin , Germany.
J Phys Chem A. 2019 Mar 28;123(12):2361-2378. doi: 10.1021/acs.jpca.8b11959. Epub 2019 Mar 12.
We present unrestricted and generalized Hartree-Fock solutions (UHF and GHF, respectively) for the single-band Hubbard model of an equilateral triangle. Spin-orbit coupling (SOC) is treated self-consistently, and HF stability and properties of different spin structures are studied in detail. The GHF solution switches from noncollinear to collinear when crossing a high-symmetry point in parameter space (spanned by the amplitudes of spin-conserving and spin-dependent hopping, i.e., kinetic energy and SOC, respectively). The collinear GHF solution represents a simple example to disprove the notion that a collinear vector spin density in a Slater determinant necessarily entails a defined spin projection. Spin Hamiltonian parameters for the anisotropic interaction between three spin-1/2 centers are extracted from HF energies and subsequently compared to exact results from effective Hamiltonian theory. This provides an unambiguous benchmark for interpreting broken-symmetry mean-field solutions in terms of spin configurations and puts this semiclassical approach (frequently applied in broken-symmetry density functional theory) on a firmer basis.
我们给出了等边三角形单带 Hubbard 模型的无限制和广义 Hartree-Fock 解(分别为 UHF 和 GHF)。自旋轨道耦合(SOC)被自洽地处理,详细研究了 HF 稳定性和不同自旋结构的性质。当穿过参数空间中的高对称点(由自旋守恒和自旋相关跃迁的幅度,即动能和 SOC 分别跨越)时,GHF 解从非共线切换到共线。共线 GHF 解代表了一个简单的例子,证明了在 Slater 行列式中,共线向量自旋密度必然需要定义的自旋投影的观点是错误的。从 HF 能量中提取了三个自旋为 1/2 中心之间各向异性相互作用的自旋哈密顿参数,然后与有效哈密顿理论的精确结果进行比较。这为根据自旋构型解释破对称平均场解提供了一个明确的基准,并为这种半经典方法(在破对称密度泛函理论中经常应用)奠定了更坚实的基础。