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Spin-Canting-Induced Band Reconstruction in the Dirac Material Ca_{1-x}Na_{x}MnBi_{2}.
Physical Review Letters ( IF 8.6 ) Pub Date : 2020-04-03 , DOI: 10.1103/physrevlett.124.137201
R Yang 1 , M Corasaniti 1 , C C Le 2 , Z Y Liao 3, 4 , A F Wang 5 , Q Du 5, 6 , C Petrovic 5, 6 , X G Qiu 3, 4, 7 , J P Hu 3, 8, 9 , L Degiorgi 1
Affiliation  

The ternary AMnBi_{2} (A is alkaline as well as rare-earth atom) materials provide an arena for investigating the interplay between low-dimensional magnetism of the antiferromagnetic MnBi layers and the electronic states in the intercalated Bi layers, which harbor relativistic fermions. Here, we report on a comprehensive study of the optical properties and magnetic torque response of Ca_{1-x}Na_{x}MnBi_{2}. Our findings give evidence for a spin canting occurring at T_{s}∼50-100  K. With the support of first-principles calculations we establish a direct link between the spin canting and the reconstruction of the electronic band structure, having immediate implications for the spectral weight reshuffling in the optical response, signaling a partial gapping of the Fermi surface, and the dc transport properties below T_{s}.

中文翻译:

狄拉克材料Ca_ {1-x} Na_ {x} MnBi_ {2}中自旋引起的能带重构。

三元AMnBi_ {2}(A是碱性原子以及稀土原子)材料为研究反铁磁MnBi层的低维磁性与插层Bi层中的电子态之间的相互作用提供了场所,Bi层中包含相对论性费米子。在这里,我们对Ca_ {1-x} Na_ {x} MnBi_ {2}的光学性质和磁转矩响应进行了全面研究。我们的发现提供了在T_ {s}〜50-100 K处发生自旋倾斜的证据。在第一性原理计算的支持下,我们在自旋倾斜与电子能带结构的重建之间建立了直接联系,对光学响应中的光谱权重转换,表明费米表面出现了部分缺口,并且直流传输特性低于T_ {s}。
更新日期:2020-03-30
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