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arXiv 2608.23823cond-mat.supr-concond-mat.mtrl-sci

La₃Ni₂O₇中交织的自旋-电荷条纹序与极性晶格畸变

Intertwined spin-charge stripe order and polar lattice distortion in La$_{3}$Ni$_{2}$O$_{7}$

Xiaoying Li, Wenqian Tu, Run Lv, Li'e Liu, Dingfu Shao, Yuping Sun, Wenjian Lu

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中文总结 AI 辅助

本研究通过第一性原理计算明确La₃Ni₂O₇低压态中自旋、电荷与晶格的紧密交织关系,发现其高压下自旋涨落可能介导超导配对,且最低能a-条纹态可弛豫至极性Am2m结构。

中文摘要 AI 辅助

La₃Ni₂O₇的低温密度波态具有显著的自旋密度波(SDW)序,而近期实验进一步揭示了电荷重新分布以及伴随的晶格对称性降低。然而,自旋、电荷与晶格之间的微观关系仍不明确。我们采用第一性原理计算,研究了La₃Ni₂O₇的电子结构和静态自旋 susceptibility随压力的演化,同时分析了代表性磁构型的能量学与晶格响应。我们将SDW不稳定性追溯至强费米面嵌套,发现高压下的自旋响应与T_C密切相关,这表明存在自旋涨落介导的配对。在考虑的候选磁态中,自旋-电荷-条纹态在能量上更受青睐且动态稳定,表现出显著的局域Ni磁矩和Ni-O键长的歧化。值得注意的是,能量最低的a-条纹态会通过沿b轴的极性畸变自发弛豫至实验提出的极性Am2m结构。这些结果建立了一个统一图像:在低压密度波态中,自旋、电荷与晶格响应紧密交织,而自旋涨落仍是高压下超导的合理组成部分。

英文摘要

The low-temperature density-wave state of La$_3$Ni$_2$O$_7$ hosts pronounced spin-density-wave (SDW) order, while recent experiments further reveal charge redistribution and a concomitant lattice-symmetry lowering. However, the microscopic relationship among spin, charge, and lattice remains unclear. Using first-principles calculations, we investigate the pressure evolution of the electronic structure and static spin susceptibility of La$_3$Ni$_2$O$_7$, together with the energetics and lattice response of representative magnetic configurations. We trace the SDW instability to strong Fermi-surface nesting and find that the high-pressure spin response closely tracks $T_{\mathrm C}$, suggesting spin-fluctuation-mediated pairing. Among the candidate magnetic states considered, the spin-charge-stripe states emerge as energetically favored and dynamically stable, developing pronounced disproportionation of both the local Ni moments and the Ni--O bond lengths. Remarkably, the lowest-energy a-stripe state spontaneously relaxes into the experimentally proposed polar Am2m structure through a polar distortion along the b axis. These results establish a unified picture in which spin, charge, and lattice responses are strongly intertwined in the low-pressure density-wave state, while spin fluctuations remain a plausible ingredient of superconductivity under pressure.

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