Debye Institute for Nanomaterials Science, Utrecht University, 3584 CA Utrecht, The Netherlands.
Institut de Minéralogie, de Physique des Matériaux et de Cosmochimie, CNRS, Sorbonne Université, MNHN, UMR7590, 75252 Paris Cedex 05, France.
Phys Rev Lett. 2019 Nov 15;123(20):207201. doi: 10.1103/PhysRevLett.123.207201.
The magnitude of the orbital magnetic moment and its role as a trigger of the Verwey transition in the prototypical Mott insulator, magnetite, remain contentious. Using 1s2p resonant inelastic x-ray scattering angle distribution (RIXS-AD), we prove the existence of noncollinear orbital magnetic ordering and infer the presence of dynamical distortion creating a polaronic precursor for the metal to insulator transition. These conclusions are based on a subtle angular shift of the RIXS-AD spectral intensity as a function of the magnetic field orientation. Theoretical simulations show that these results are only consistent with noncollinear magnetic orbital ordering. To further support these claims we perform Fe K-edge x-ray magnetic circular dichroism in order to quantify the Fe average orbital magnetic moment.
轨道磁矩的大小及其作为原型莫特绝缘体磁铁矿中韦尔韦尔转变的触发因素一直存在争议。使用 1s2p 共振非弹性 x 射线散射角分布(RIXS-AD),我们证明了非共线轨道磁有序的存在,并推断出动态变形的存在,为金属到绝缘转变创造了极化子前体。这些结论是基于 RIXS-AD 光谱强度随磁场方向的微妙角度偏移。理论模拟表明,这些结果仅与非共线磁轨道有序一致。为了进一步支持这些说法,我们进行了 Fe K 边 X 射线磁圆二色性测量,以定量测量 Fe 平均轨道磁矩。