journal article·2022-07-05Open access

High-pressure control of optical nonlinearity in the polar Weyl semimetal TaAs

Chen Li, Xiang Li, T. Deshpande, Xinwei Li, N. Nair, J. G. Analytis, D. M. Silevitch, T. F. Rosenbaum, D. Hsieh

Physical Review B· Volume 106· Issue 1

Abstract

The transition metal monopnictide family of Weyl semimetals recently has been shown to exhibit anomalously strong second-order optical nonlinearity, which is theoretically attributed to a highly asymmetric polarization distribution induced by their polar structure. We experimentally test this hypothesis by measuring optical second harmonic generation (SHG) from TaAs across a pressure-tuned polar-to-nonpolar structural phase transition. Despite the high-pressure structure remaining noncentrosymmetric, the SHG yield is reduced by more than 60% by 20 GPa as compared to the ambient pressure value. By examining the pressure dependence of distinct groups of SHG susceptibility tensor elements, we find that the yield is primarily controlled by a single element that governs the response along the polar axis. Our results confirm a connection between the polar axis and the giant optical nonlinearity of Weyl semimetals and demonstrate pressure as a means to tune this effect in situ.
Source: openalex_inverted_index · Quality: baseline

Research context

OpenAlex topics: Topological Materials and Phenomena · 2D Materials and Applications · Quantum Mechanics and Non-Hermitian Physics

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

References (38)

Show source-provided references
1. 10.1103/RevModPhys.90.01500110.1103/RevModPhys.90.015001 ↗
2. 10.1103/PhysRevB.83.20510110.1103/PhysRevB.83.205101 ↗
3. 10.1126/science.aaa929710.1126/science.aaa9297 ↗
4. 10.1103/PhysRevX.5.03101310.1103/PhysRevX.5.031013 ↗
5. 10.1038/nphys342510.1038/nphys3425 ↗
6. 10.1103/PhysRevB.86.11513310.1103/PhysRevB.86.115133 ↗
7. 10.1038/ncomms1073510.1038/ncomms10735 ↗
8. 10.1038/nmat478710.1038/nmat4787 ↗
9. 10.1103/PhysRevX.4.03103510.1103/PhysRevX.4.031035 ↗
10. 10.1103/PhysRevX.5.03102310.1103/PhysRevX.5.031023 ↗
11. 10.1103/PhysRevB.84.07512910.1103/PhysRevB.84.075129 ↗
12. 10.1103/PhysRevLett.113.18720210.1103/PhysRevLett.113.187202 ↗
13. 10.1103/PhysRevLett.117.14640310.1103/PhysRevLett.117.146403 ↗
14. 10.1038/nature1827610.1038/nature18276 ↗
15. 10.1103/PhysRevB.94.03520210.1103/PhysRevB.94.035202 ↗
16. 10.1038/s41467-017-02237-110.1038/s41467-017-02237-1 ↗
17. 10.1146/annurev-conmatphys-031218-01371210.1146/annurev-conmatphys-031218-013712 ↗
18. 10.1038/nphys414610.1038/nphys4146 ↗
19. 10.1103/PhysRevLett.122.19740110.1103/PhysRevLett.122.197401 ↗
20. 10.1038/s41467-020-14463-110.1038/s41467-020-14463-1 ↗
21. 10.1038/s41563-019-0297-410.1038/s41563-019-0297-4 ↗
22. 10.1038/s41563-019-0296-510.1038/s41563-019-0296-5 ↗
23. 10.1038/nphys396910.1038/nphys3969 ↗
24. 10.1103/PhysRevB.98.16511310.1103/PhysRevB.98.165113 ↗
25. 10.1103/PhysRevB.97.08520110.1103/PhysRevB.97.085201 ↗
26. 10.1103/PhysRevLett.117.14640210.1103/PhysRevLett.117.146402 ↗
27. 10.1007/s11433-017-9126-610.1007/s11433-017-9126-6 ↗
28. 10.1088/1361-648X/aab5e310.1088/1361-648X/aab5e3 ↗
29. 10.1038/s41598-017-13610-x10.1038/s41598-017-13610-x ↗
30. 10.1016/j.ssc.2016.04.02410.1016/j.ssc.2016.04.024 ↗
31. 10.1107/S002188980800051410.1107/S0021889808000514 ↗
32. 10.1103/PhysRevB.102.07540210.1103/PhysRevB.102.075402 ↗
33. 10.1063/1.489141710.1063/1.4891417 ↗
34. 10.1364/OL.40.00467110.1364/OL.40.004671 ↗
35. 10.1038/s41535-017-0066-z10.1038/s41535-017-0066-z ↗
36. 10.1126/science.aad118810.1126/science.aad1188 ↗
37. 10.1103/PhysRevB.93.03513910.1103/PhysRevB.93.035139 ↗
38. 10.1103/PhysRevB.95.02010210.1103/PhysRevB.95.020102 ↗