journal article·2022-05-02Open access

Searching for the Kardar-Parisi-Zhang phase in microcavity polaritons

A. Ferrier, A. Zamora, G. Dagvadorj, M. H. Szymańska

Physical Review B· Volume 105· Issue 20

Abstract

Recent approximate analytical work has suggested that, at certain values of the external pump, the optical parametric oscillator (OPO) regime of microcavity polaritons may provide a long-sought realization of Kardar-Parisi-Zhang (KPZ) physics in 2D. Here, by solving the full microscopic model numerically using the truncated Wigner method, we prove that this predicted KPZ phase for OPO is robust against the appearance of vortices or other effects. For those pump strengths, spatial correlations in the direction perpendicular to the pump, and the distribution of phase fluctuations, match closely to the forms characteristic of the KPZ universality. This strongly indicates the viability of observing KPZ behavior in future polariton OPO experiments.
Source: openalex_inverted_index · Quality: baseline

Research context

OpenAlex topics: Strong Light-Matter Interactions · Plasmonic and Surface Plasmon Research · Quantum Information and Cryptography

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

References (41)

Show source-provided references
1. 10.1103/PhysRevLett.56.88910.1103/PhysRevLett.56.889 ↗
2. 10.1143/JPSJ.66.6710.1143/JPSJ.66.67 ↗
3. 10.1103/PhysRevE.82.03190310.1103/PhysRevE.82.031903 ↗
4. 10.1103/PhysRevLett.79.151510.1103/PhysRevLett.79.1515 ↗
5. 10.1103/PhysRevE.64.03610110.1103/PhysRevE.64.036101 ↗
6. 10.1140/epjb/e2005-00235-y10.1140/epjb/e2005-00235-y ↗
7. 10.1038/srep0003410.1038/srep00034 ↗
8. 10.1007/s10955-012-0503-010.1007/s10955-012-0503-0 ↗
9. 10.1103/PhysRevLett.124.06060110.1103/PhysRevLett.124.060601 ↗
10. 10.1209/0295-5075/105/5000110.1209/0295-5075/105/50001 ↗
11. 10.1103/PhysRevB.89.04530910.1103/PhysRevB.89.045309 ↗
12. 10.1103/PhysRevX.5.01101710.1103/PhysRevX.5.011017 ↗
13. 10.1103/PhysRevB.91.04530110.1103/PhysRevB.91.045301 ↗
14. 10.1103/PhysRevB.92.15530710.1103/PhysRevB.92.155307 ↗
15. 10.1088/0034-4885/79/9/09600110.1088/0034-4885/79/9/096001 ↗
16. 10.1103/PhysRevB.94.10452010.1103/PhysRevB.94.104520 ↗
17. 10.1103/PhysRevB.94.10452110.1103/PhysRevB.94.104521 ↗
18. 10.1103/PhysRevLett.118.08530110.1103/PhysRevLett.118.085301 ↗
19. 10.1103/PhysRevB.97.19545310.1103/PhysRevB.97.195453 ↗
20. 10.1103/PhysRevB.103.04530210.1103/PhysRevB.103.045302 ↗
21. 10.1209/0295-5075/132/6700410.1209/0295-5075/132/67004 ↗
22. 10.1103/PhysRevLett.121.08570410.1103/PhysRevLett.121.085704 ↗
23. 10.1103/PhysRevLett.125.26570110.1103/PhysRevLett.125.265701 ↗
24. 10.1103/PhysRevLett.125.21530110.1103/PhysRevLett.125.215301 ↗
25. 10.1038/nmat503910.1038/nmat5039 ↗
26. 10.1103/PhysRevX.5.04102810.1103/PhysRevX.5.041028 ↗
27. 10.1103/PhysRevX.7.04100610.1103/PhysRevX.7.041006 ↗
28. 10.1103/PhysRevB.98.16530710.1103/PhysRevB.98.165307 ↗
29. 10.1103/PhysRevB.71.11530110.1103/PhysRevB.71.115301 ↗
30. 10.1103/RevModPhys.85.29910.1103/RevModPhys.85.299 ↗
31. 10.1103/PhysRevB.72.12533510.1103/PhysRevB.72.125335 ↗
32. 10.1103/PhysRevB.79.16530210.1103/PhysRevB.79.165302 ↗
33. 10.1103/PhysRevLett.121.09530210.1103/PhysRevLett.121.095302 ↗
34. 10.1103/PhysRevLett.125.09530110.1103/PhysRevLett.125.095301 ↗
35. 10.1103/PhysRevB.89.13431010.1103/PhysRevB.89.134310 ↗
36. 10.1038/nphys166810.1038/nphys1668 ↗
37. 10.1103/PhysRevA.76.04380710.1103/PhysRevA.76.043807 ↗
38. 10.1103/PhysRevE.77.03113410.1103/PhysRevE.77.031134 ↗
39. 10.1103/PhysRevE.92.01010110.1103/PhysRevE.92.010101 ↗
40. 10.1103/PhysRevLett.109.17060210.1103/PhysRevLett.109.170602 ↗
41. 10.1103/PhysRevE.88.04211810.1103/PhysRevE.88.042118 ↗