Martinez Alvarez V M, Coutinho-Filho M D
J Phys Condens Matter. 2019 May 15;31(19):195603. doi: 10.1088/1361-648X/ab0714. Epub 2019 Feb 14.
The ground state (GS) properties of the quasi-one-dimensional AB Hubbard model are investigated taking the effects of charge and spin quantum fluctuations on equal footing. In the strong-coupling regime, a functional integral representation allows us to derive a low-energy Lagrangian suitable to describe the ferrimagnetic phase at half filling and the phases in the hole-doped regime. At half filling, a perturbative spin-wave analysis allows us to find the GS energy, sublattice magnetizations, and total spin per unit cell in the Lieb ferrimagnetic GS of the effective quantum Heisenberg model, in very good agreement with previous results. In the challenging hole doping regime away from half filling, we derive the corresponding [Formula: see text] Hamiltonian. Under the assumption that charge and spin quantum correlations are decoupled, the evolution of the second-order spin-wave modes in the doped regime unveils the occurrence of spatially modulated spin structures and the emergence of phase separation in the presence of resonating-valence-bond states. We also calculate the doping-dependent GS energy and total spin per unit cell, including both Zeeman and orbital contributions, in which case it is shown that the spiral ferrimagnetic order collapses at a critical hole concentration. Notably, our analytical results in the doped regime are in very good agreement with density matrix renormalization group studies, where our assumption of spin-charge decoupling is numerically supported by the formation of charge-density waves in anti-phase with the modulation of the magnetic structure.
在平等考虑电荷和自旋量子涨落效应的情况下,研究了准一维AB哈伯德模型的基态(GS)性质。在强耦合 regime 中,泛函积分表示使我们能够推导出一个低能拉格朗日量,适用于描述半填充时的亚铁磁相和空穴掺杂 regime 中的相。在半填充时,微扰自旋波分析使我们能够在有效量子海森堡模型的Lieb亚铁磁GS中找到GS能量、亚晶格磁化强度和每个晶胞的总自旋,与先前的结果非常吻合。在远离半填充的具有挑战性的空穴掺杂 regime 中,我们推导出了相应的[公式:见文本]哈密顿量。在电荷和自旋量子关联解耦的假设下,掺杂 regime 中二阶自旋波模式的演化揭示了空间调制自旋结构的出现以及在存在共振价键态时相分离的出现。我们还计算了依赖于掺杂的GS能量和每个晶胞的总自旋,包括塞曼和轨道贡献,在这种情况下表明螺旋亚铁磁序在临界空穴浓度处崩塌。值得注意的是,我们在掺杂 regime 中的分析结果与密度矩阵重整化群研究非常吻合,其中我们的自旋 - 电荷解耦假设在数值上得到了与磁结构调制反相的电荷密度波形成的支持。