Stability via symmetry breaking in interacting driven systems
Source abstract
Abstract
Photonic and bosonic systems subject to incoherent, wide-bandwidth driving cannot typically reach stable finite-density phases using only nondissipative Hamiltonian nonlinearities; one instead needs nonlinear losses, or a finite pump bandwidth. We describe here a very general mechanism for circumventing this common limit, whereby Hamiltonian interactions can cut-off heating from a Markovian pump, by effectively breaking a symmetry of the unstable, linearized dynamics. We analyze two concrete examples of this mechanism. The first is a new kind of $\mathcal{PT}$ laser, where Hermitian Hamiltonian interactions can move the dynamics between the $\mathcal{PT}$ broken and unbroken phases and thus induce stability. The second uses on-site Kerr or Hubbard type interactions to break the chiral symmetry in a topological photonic lattice, inducing exotic phenomena from topological lasing to the stabilization of Fock states in a topologically protected edge mode.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Mechanical and Optical Resonators · Advanced Fiber Laser Technologies · Nonlinear Photonic Systems
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Department of Physics, University of Chicago, 5640 South Ellis Avenue, Chicago, Illinois 60637, USA
Pritzker School of Molecular Engineering, University of Chicago, Chicago, Illinois 60637, USA
Funding
Air Force Office of Scientific Research · National Science Foundation · Simons Foundation
References (59)
Show source-provided references
1. D. Walls · 199410.1007/978-3-642-79504-6 ↗
2. C. Gardiner · 2004
3. 10.1103/RevModPhys.77.13710.1103/RevModPhys.77.137 ↗
4. 10.1103/RevModPhys.80.127510.1103/RevModPhys.80.1275 ↗
5. 10.1103/PhysRevLett.110.19530110.1103/PhysRevLett.110.195301 ↗
6. 10.1038/nphys107310.1038/nphys1073 ↗
7. 10.1103/PhysRevLett.105.01570210.1103/PhysRevLett.105.015702 ↗
8. 10.1103/RevModPhys.85.29910.1103/RevModPhys.85.299 ↗
9. 10.1103/PhysRevLett.96.23060210.1103/PhysRevLett.96.230602 ↗
10. 10.1103/PhysRevA.96.03382810.1103/PhysRevA.96.033828 ↗
11. 10.1103/PhysRevB.99.06451110.1103/PhysRevB.99.064511 ↗
12. 10.1038/s41586-019-0897-910.1038/s41586-019-0897-9 ↗
13. 10.1103/PhysRevB.92.17430510.1103/PhysRevB.92.174305 ↗
14. 10.1103/PhysRevA.95.04381110.1103/PhysRevA.95.043811 ↗
15. 10.1080/1478644260856412710.1080/14786442608564127 ↗
16. 10.1103/PhysRevLett.80.524310.1103/PhysRevLett.80.5243 ↗
17. 10.1088/0034-4885/70/6/R0310.1088/0034-4885/70/6/R03 ↗
18. 10.1126/science.125847910.1126/science.1258479 ↗
19. 10.1038/nphys292710.1038/nphys2927 ↗
20. 10.1038/srep2488910.1038/srep24889 ↗
21. 10.1126/science.125848010.1126/science.1258480 ↗
22. 10.1038/nphys432310.1038/nphys4323 ↗
23. 10.1103/PhysRevB.78.19512510.1103/PhysRevB.78.195125 ↗
24. 10.1038/s41586-021-03833-410.1038/s41586-021-03833-4 ↗
25. 10.1063/5.004112410.1063/5.0041124 ↗
26. 10.1038/s41566-017-0006-210.1038/s41566-017-0006-2 ↗
27. 10.1103/PhysRevLett.120.11390110.1103/PhysRevLett.120.113901 ↗
28. 10.1038/s41467-018-03434-210.1038/s41467-018-03434-2 ↗
29. 10.1038/s41586-018-0478-310.1038/s41586-018-0478-3 ↗
30. 10.1126/science.aau429610.1126/science.aau4296 ↗
31. 10.1038/s41567-022-01671-310.1038/s41567-022-01671-3 ↗
32. 10.1007/BF0160849910.1007/BF01608499 ↗
33. 10.1063/1.52297910.1063/1.522979 ↗
34. 10.1088/1367-2630/18/9/09500310.1088/1367-2630/18/9/095003 ↗
35. 10.1088/2058-9565/abcfcc10.1088/2058-9565/abcfcc ↗
36. 10.1016/0921-4534(89)90225-610.1016/0921-4534(89)90225-6 ↗
37. 10.1088/1367-2630/15/11/11304110.1088/1367-2630/15/11/113041 ↗
38. 10.1103/PhysRevB.93.15511210.1103/PhysRevB.93.155112 ↗
39. 10.1103/PhysRevLett.112.20390110.1103/PhysRevLett.112.203901 ↗
40. 10.1038/nature2328110.1038/nature23281 ↗
41. 10.1038/nature2328010.1038/nature23280 ↗
42. 10.1038/s41467-018-06477-710.1038/s41467-018-06477-7 ↗
43. 10.1103/PhysRevLett.123.18050110.1103/PhysRevLett.123.180501 ↗
44. 10.1088/1367-2630/ab32ab10.1088/1367-2630/ab32ab ↗
45. 10.1038/s41467-020-19090-410.1038/s41467-020-19090-4 ↗
46. 10.1103/PhysRevA.92.03231910.1103/PhysRevA.92.032319 ↗
47. 10.1088/1751-8121/aa5fbe10.1088/1751-8121/aa5fbe ↗
48. 10.1103/PhysRevA.98.04361510.1103/PhysRevA.98.043615 ↗
49. 10.1103/PhysRevLett.126.02040210.1103/PhysRevLett.126.020402 ↗
50. 10.1103/PhysRevLett.130.12360210.1103/PhysRevLett.130.123602 ↗
51. 10.1038/ncomms1077910.1038/ncomms10779 ↗
52. 10.1103/PhysRevLett.42.169810.1103/PhysRevLett.42.1698 ↗
53. 10.1103/PhysRevB.22.209910.1103/PhysRevB.22.2099 ↗
54. 10.1103/PhysRevX.11.01101510.1103/PhysRevX.11.011015 ↗
55. 10.1038/s41598-020-79915-610.1038/s41598-020-79915-6 ↗
56. 10.1515/nanoph-2020-041510.1515/nanoph-2020-0415 ↗
57. 10.1038/s41586-022-05367-910.1038/s41586-022-05367-9 ↗
58. 10.1103/PhysRevResearch.5.04322910.1103/PhysRevResearch.5.043229 ↗
59. 10.1088/1367-2630/14/7/07300710.1088/1367-2630/14/7/073007 ↗