We report the anomalous Hall effect (AHE) and the anomalous Nernst effect (ANE) data for the noncollinear Weyl semimetal CeAlSi. The anomalous Hall conductivity (σA i j ) was measured for two different orientations of the magnetic field (B), namely σA yz for B||a and σA xy for B||c, where a and c denote the crystallographic axes. We find that σA xy and σA yz are of opposite sign and both are large below the Curie temperature (TC). In the paramagnetic phase, σA xy rises even more and goes through a maximum at T ≈ 170 K, whereas the absolute value of σA yz decreases with increasing temperature. The origin of the sign difference between σA xy and σA yz 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 (αA xy) measured for B||c. αA xy/T turns out to be sizeable in the magnetic phase and above TC slowly decreases with temperature. We were able to recreate the temperature dependencies of σA xy and αA xy/T in the paramagnetic phase using a single band toy model assuming a nonzero Berry curvature in the vicinity of theWeyl node. A decisive factor appears to be a small energy distance between the Fermi level and a Weyl point.
Sign change of anomalous Hall effect and anomalous Nernst effect in the Weyl semimetal CeAlSi
Cuono G.;Autieri C.;
2023
Abstract
We report the anomalous Hall effect (AHE) and the anomalous Nernst effect (ANE) data for the noncollinear Weyl semimetal CeAlSi. The anomalous Hall conductivity (σA i j ) was measured for two different orientations of the magnetic field (B), namely σA yz for B||a and σA xy for B||c, where a and c denote the crystallographic axes. We find that σA xy and σA yz are of opposite sign and both are large below the Curie temperature (TC). In the paramagnetic phase, σA xy rises even more and goes through a maximum at T ≈ 170 K, whereas the absolute value of σA yz decreases with increasing temperature. The origin of the sign difference between σA xy and σA yz 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 (αA xy) measured for B||c. αA xy/T turns out to be sizeable in the magnetic phase and above TC slowly decreases with temperature. We were able to recreate the temperature dependencies of σA xy and αA xy/T in the paramagnetic phase using a single band toy model assuming a nonzero Berry curvature in the vicinity of theWeyl node. A decisive factor appears to be a small energy distance between the Fermi level and a Weyl point.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.


