Majorana bound state cavities
Source abstract
Abstract
Cavities play a fundamental role in optical physics by providing spatiotemporal confinement of energy that facilitates light-matter interactions. They are routinely utilized in a variety of settings, ranging from lasers to spectral filters, to nonlinear wave mixers, and modulators. While their resonant properties make them suitable for sensing, in many applications, like in lasers, it is desired to alleviate their sensitivity in order to make a device more resilient to perturbations. Along these lines there have been several recent reports of using concepts from topological physics in order to design laser arrays that are inherently more robust. Here, we present a class of topological cavities based on Majorana bound states that provide unique scaling features as well as nondegenerate single-mode behaviors. These cavities may lead to a new family of lasers and laser arrays that are robust to defects, fabrication imperfections, and external perturbations.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Topological Materials and Phenomena · Photorefractive and Nonlinear Optics · Quantum Mechanics and Non-Hermitian Physics
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Ming Hsieh Department of Electrical and Computer Engineering, University of Southern California, Los Angeles, California 90089, USA
Funding
Air Force Office of Scientific Research · Multidisciplinary University Research Initiative · Army Research Office · National Science Foundation · Defense Advanced Research Projects Agency · Office of Naval Research · United States-Israel Binational Science Foundation
References (33)
Show source-provided references
1. 10.1103/PhysRevD.13.339810.1103/PhysRevD.13.3398 ↗
2. 10.1016/0550-3213(81)90044-410.1016/0550-3213(81)90044-4 ↗
3. 10.1103/PhysRevLett.52.211110.1103/PhysRevLett.52.2111 ↗
4. 10.1073/pnas.151517311310.1073/pnas.1515173113 ↗
5. 10.1103/PhysRevB.61.1026710.1103/PhysRevB.61.10267 ↗
6. 10.1103/PhysRevLett.86.26810.1103/PhysRevLett.86.268 ↗
7. 10.1103/PhysRevLett.104.04050210.1103/PhysRevLett.104.040502 ↗
8. 10.1103/PhysRevLett.105.17700210.1103/PhysRevLett.105.177002 ↗
9. 10.1103/PhysRevB.85.09451610.1103/PhysRevB.85.094516 ↗
10. 10.1126/science.122236010.1126/science.1222360 ↗
11. 10.1038/nphys242910.1038/nphys2429 ↗
12. 10.1126/science.125932710.1126/science.1259327 ↗
13. 10.1073/pnas.95.1.9810.1073/pnas.95.1.98 ↗
14. 10.1070/1063-7869/44/10S/S2910.1070/1063-7869/44/10S/S29 ↗
15. 10.1016/S0003-4916(02)00018-010.1016/S0003-4916(02)00018-0 ↗
16. 10.1103/PhysRevLett.117.07390110.1103/PhysRevLett.117.073901 ↗
17. 10.1038/s41567-020-1007-510.1038/s41567-020-1007-5 ↗
18. 10.1002/adma.20190438610.1002/adma.201904386 ↗
19. 10.1103/PhysRevLett.125.11740110.1103/PhysRevLett.125.117401 ↗
20. 10.1038/s41565-020-0773-710.1038/s41565-020-0773-7 ↗
21. 10.1103/PhysRevLett.120.11390110.1103/PhysRevLett.120.113901 ↗
22. 10.1038/s41467-018-03434-210.1038/s41467-018-03434-2 ↗
23. 10.1103/PhysRevLett.116.16390110.1103/PhysRevLett.116.163901 ↗
24. 10.1364/OL.41.00428110.1364/OL.41.004281 ↗
25. 10.1103/PhysRevLett.98.18680910.1103/PhysRevLett.98.186809 ↗
26. 10.1126/science.aar400510.1126/science.aar4005 ↗
27. 10.1126/science.aar400310.1126/science.aar4003 ↗
28. 10.1126/science.aao455110.1126/science.aao4551 ↗
29. 10.1038/s41586-020-1981-x10.1038/s41586-020-1981-x ↗
30. 10.1038/s41467-021-23718-410.1038/s41467-021-23718-4 ↗
31. 10.1038/s41567-021-01185-410.1038/s41567-021-01185-4 ↗
32. 10.1103/PhysRevLett.114.22390110.1103/PhysRevLett.114.223901 ↗
33. 10.1103/PhysRevB.87.03542210.1103/PhysRevB.87.035422 ↗