journal article·2018-10-01Open access

Deviation from the Kohler’s rule and Shubnikov–de Haas oscillations in type-II Weyl semimetal WTe2: High magnetic field study up to 56 T

Shota Onishi, Rajveer Jha, Atsushi Miyake, Ryuji Higashinaka, Tatsuma D. Matsuda, Masashi Tokunaga, Yuji Aoki

AIP Advances· Volume 8· Issue 10

Abstract

We have measured magnetoresistance of type-II Weyl semimetal WTe2 in high magnetic fields of B//c up to B = 56 T using a high quality single crystal with the residual resistivity ratio 1330. A Kohler plot demonstrates the existence of a deviation from the B2 dependence. Significant deviation from Kohler’s rule appears with increasing temperature, indicating wave-vector k dependent anisotropic carrier scattering, which develops with increasing temperature. The fast-Fourier-transform spectra of the observed large-amplitude Shubnikov–de Haas oscillations confirm the existence of four fundamental and one additional (cyclotron frequency of 255 T) peaks. The amplitude of the latter one increases anomalously with increasing field, confirming this oscillation being due to magnetic breakdown (or magnetic breakthrough) between the two cyclotron orbits of the adjacent hole pockets.
Source: crossref · Quality: baseline

Research context

OpenAlex topics: Topological Materials and Phenomena · 2D Materials and Applications · Advanced Condensed Matter Physics

SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.

Affiliations

Department of Physics, Tokyo Metropolitan University 1 , Hachioji, Tokyo 192-0397, Japan

The Institute for Solid State Physics, University of Tokyo 2 , Kashiwa 277-8581, Japan

Funding

Japan Society for the Promotion of Science

References (20)

Show source-provided references
1. Rev. Mod. Phys. · 2010 · 82 · 304510.1103/revmodphys.82.3045 ↗
2. Rev. Mod. Phys. · 2011 · 83 · 105710.1103/revmodphys.83.1057 ↗
3. Annu. Rev. Condens. Matter Phys. · 2017 · 8 · 33710.1146/annurev-conmatphys-031016-025458 ↗
4. Rev. Mod. Phys. · 2018 · 90 · 01500110.1103/revmodphys.90.015001 ↗
5. Nature · 2015 · 527 · 49510.1038/nature15768 ↗
6. Phys. Rev. B · 2016 · 94 · 241119(R)10.1103/physrevb.94.241119 ↗
7. Phys. Rev. B · 2016 · 94 · 16140110.1103/physrevb.94.161401 ↗
8. Phys. Rev. Lett. · 2015 · 115 · 16660210.1103/physrevlett.115.166602 ↗
9. Phys. Rev. Lett. · 2015 · 114 · 17660110.1103/physrevlett.114.176601 ↗
10. Phys. Rev. Lett. · 2015 · 115 · 05720210.1103/physrevlett.115.057202 ↗
11. Phys. Rev. B · 2015 · 92 · 12515210.1103/physrevb.92.125152 ↗
12. Phys. Rev. B · 2016 · 93 · 12110810.1103/physrevb.93.121108 ↗
13. Nature · 2014 · 514 · 20510.1038/nature13763 ↗
14. Appl. Phys. Lett. · 2015 · 107 · 18241110.1063/1.4935240 ↗
15. Phys. Rev. B · 2015 · 92 · 04110410.1103/physrevb.92.041104 ↗
16. Front. Phys. · 2017 · 12 · 12720310.1007/s11467-016-0629-7 ↗
17. 1989
18. Phys. Rev. · 1969 · 178 · 103710.1103/physrev.178.1037 ↗
19. J. Chem. Thermodynamics · 1992 · 24 · 62710.1016/s0021-9614(05)80034-5 ↗
20. 1984