论文标题
Weyl半cealsi中异常大厅效应的符号变化和异常的NernST效应
Sign change of the anomalous Hall effect and the anomalous Nernst effect in Weyl semimetal CeAlSi
论文作者
论文摘要
我们报告了非共线Weyl Semimetal Cealsi的异常霍尔效应(AHE)和异常的Nernst效应(ANE)数据。测量了磁场的两个不同方向(b)的异常霍尔电导率(σ_ij^a),即b ii a和b ii c的σ_yz^a和σ_xy^a,其中a和c表示晶体学轴。我们发现σ_xy^a和σ_yz^a的符号相反,并且在居里温度(T_C)以下都大。在顺磁性阶段,σ_xy^a增加了更多,并在t〜170 K处进行最大值,而σ_yz^a的绝对值随温度的升高而降低。 σ_xy^a和σ_yz^a之间的符号差的来源归因于在自旋方向的变化下频带结构的重建。此外,在存在AHE中的驼峰并且标量旋转手性的系统中,我们表明K空间拓扑是确定低温和高温下运输特性的重要作用。我们还观察到针对B II c测量的Nernst电导率(α_xy^a)的异常贡献。 α_xy^a/t在磁相及以上T_C时很大,随着温度而缓慢降低。我们能够使用单带玩具模型在顺磁相中重新创建σ_xy^a和α_xy^a/t的温度依赖性,假设在Weyl节点附近的非零浆果曲率。决定性因子似乎是费米水平和韦尔点之间的较小能量距离。
We report the anomalous Hall effect (AHE) and the anomalous Nernst effect (ANE) data for the non-collinear Weyl semimetal CeAlSi. The anomalous Hall conductivity (σ_ij^A) was measured for two different orientations of the magnetic field (B), namely σ_yz^A for B II a and σ_xy^A for B II c, where a and c denote the crystallographic axes. We find that σ_xy^A and σ_yz^A are of opposite sign and both are large below the Curie temperature (T_C). In the paramagnetic phase, σ_xy^A raises even more and goes through a maximum at T ~ 170 K, whereas the absolute value of σ_yz^A decreases with increasing temperature. The origin of the sign difference between σ_xy^A and σ_yz^A was attributed to the reconstruction of the band structure under the variation of the spin orientation. Further, in a system where humps in the AHE are present and scalar spin chirality is zero, we show that the k-space topology plays an important role to determine the transport properties at both low and high temperatures. We also observed the anomalous contribution in the Nernst conductivity (α_xy^A) measured for B II c. α_xy^A/T turns out to be sizeable in the magnetic phase and above T_C slowly decreases with temperature. We were able to recreate the temperature dependences of σ_xy^A and α_xy^A/T in the paramagnetic phase using a single band toy-model assuming a non-zero Berry curvature in the vicinity of the Weyl node. A decisive factor appears to be a small energy distance between the Fermi level and a Weyl point.