Cavity‐Induced Enhancement of Magneto‐Optic Effects in Monolayer Transition Metal Dichalcogenides
Source abstract
Abstract
Abstract Monolayer transition metal dichalcogenides represent a class of 2D direct‐bandgap semiconductors, which do not support magneto‐optical (MO) effects in the absence of magnetic field due to time reversal symmetry. Magnetic exchange field (MEF) has been demonstrated to be able to generate MO effects in monolayer transition metal dichalcogenides, causing Faraday rotation of several tenths of degree without the need of magnetic field. Here, the possibility of enhancing the MO effects of monolayer transition metal dichalcogenides upon MEF using a cavity structure is investigated. It is identified that the Faraday rotation (FR) angle can be boosted by choosing the proper thickness of optical cavity due to its resonant characteristics. In particular, unlike the conventional bulky magnetic materials always with fixed MO effects, the FR angle here can be manipulated by the chemical potential, enabling a route of engineering the MO effects in monolayer transition metal dichalcogenides. The results suggest 2D layered semiconductors being the possible building blocks in nonreciprocal MO devices.
Source: crossref · Quality: baseline
Research context
OpenAlex topics: 2D Materials and Applications · Perovskite Materials and Applications · Multiferroics and related materials
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Key Laboratory of Radio Frequency and Micro‐Nano Electronics of Jiangsu Province College of Electronic and Optical Engineering & College of Microelectronics Nanjing University of Posts and Telecommunications Nanjing Jiangsu 210046 China
College of Physics and Materials Science Henan Normal University Henan 453007 China
Funding
National Natural Science Foundation of China · Natural Science Foundation of Jiangsu Province · Nanjing University of Posts and Telecommunications
References (51)
Show source-provided references
1. 10.1038/nature0423510.1038/nature04235 ↗
2. 10.1103/PhysRevLett.101.19640510.1103/PhysRevLett.101.196405 ↗
3. 10.1126/science.110289610.1126/science.1102896 ↗
4. 10.1038/nphoton.2016.4510.1038/nphoton.2016.45 ↗
5. 10.1126/science.115279310.1126/science.1152793 ↗
6. 10.1126/science.120269110.1126/science.1202691 ↗
7. 10.1021/nn201622e10.1021/nn201622e ↗
8. 10.1038/nphys181610.1038/nphys1816 ↗
9. 10.1103/PhysRevB.84.23541010.1103/PhysRevB.84.235410 ↗
10. 10.1063/1.360559310.1063/1.3605593 ↗
11. 10.1021/nl300572y10.1021/nl300572y ↗
12. 10.1021/nl301633510.1021/nl3016335 ↗
13. 10.1063/1.354363310.1063/1.3543633 ↗
14. 10.1038/ncomms1121610.1038/ncomms11216 ↗
15. 10.1063/1.494571510.1063/1.4945715 ↗
16. 10.1088/1367-2630/15/11/11300310.1088/1367-2630/15/11/113003 ↗
17. 10.1103/PhysRevLett.105.13680510.1103/PhysRevLett.105.136805 ↗
18. 10.1126/science.125014010.1126/science.1250140 ↗
19. 10.1038/nnano.2016.28210.1038/nnano.2016.282 ↗
20. 10.1038/nnano.2012.9610.1038/nnano.2012.96 ↗
21. 10.1038/nnano.2012.9510.1038/nnano.2012.95 ↗
22. 10.1038/ncomms188210.1038/ncomms1882 ↗
23. 10.1038/nnano.2013.15110.1038/nnano.2013.151 ↗
24. 10.1021/nl903868w10.1021/nl903868w ↗
25. 10.1038/nphys320310.1038/nphys3203 ↗
26. 10.1038/nnano.2016.21310.1038/nnano.2016.213 ↗
27. 10.1103/PhysRevB.94.04541510.1103/PhysRevB.94.045415 ↗
28. 10.1103/PhysRevLett.114.03740110.1103/PhysRevLett.114.037401 ↗
29. 10.1103/PhysRevLett.117.07740210.1103/PhysRevLett.117.077402 ↗
30. 10.1103/PhysRevLett.117.18740110.1103/PhysRevLett.117.187401 ↗
31. 10.1038/nmat493110.1038/nmat4931 ↗
32. 10.1021/acs.jpclett.7b0178610.1021/acs.jpclett.7b01786 ↗
33. 10.1103/PhysRevB.89.15542910.1103/PhysRevB.89.155429 ↗
34. 10.1103/PhysRevLett.119.12740310.1103/PhysRevLett.119.127403 ↗
35. 10.1103/PhysRevB.85.11543810.1103/PhysRevB.85.115438 ↗
36. 10.1038/nphoton.2014.30410.1038/nphoton.2014.304 ↗
37. 10.1038/ncomms1332810.1038/ncomms13328 ↗
38. 10.1038/nphoton.2017.8610.1038/nphoton.2017.86 ↗
39. 10.1039/C6RA21314F10.1039/C6RA21314F ↗
40. 10.1103/PhysRevB.82.12512010.1103/PhysRevB.82.125120 ↗
41. 10.1103/PhysRevB.73.24541110.1103/PhysRevB.73.245411 ↗
42. 10.1103/PhysRevB.92.12140310.1103/PhysRevB.92.121403 ↗
43. 10.1103/PhysRevLett.110.06680310.1103/PhysRevLett.110.066803 ↗
44. 10.1038/ncomms1361210.1038/ncomms13612 ↗
45. 10.1002/adma.20150258510.1002/adma.201502585 ↗
46. 10.1038/nmat368710.1038/nmat3687 ↗
47. 10.1103/PhysRevLett.119.13740110.1103/PhysRevLett.119.137401 ↗
48. 10.1063/1.155942210.1063/1.1559422 ↗
49. 10.1103/PhysRevB.63.16531810.1103/PhysRevB.63.165318 ↗
50. 10.1063/1.247199310.1063/1.2471993 ↗
51. 10.1063/1.480830210.1063/1.4808302 ↗