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

Alam, Md Shahin, Fakhredine, Amar, Ahmed, Mujeeb, Tanwar, P. K., Yang, Hung-Yu, Tafti, Fazel, Cuono, Giuseppe, Islam, Rajibul, Singh, Bahadur, Lynnyk, Artem, Autieri, Carmine, Matusiak, Marcin

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.

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