Dynamical preparation of a steady off-diagonal long-range order state in the Hubbard model with a local non-Hermitian impurity
Source abstract
Abstract
The cooperation between non-Hermiticity and interaction brings about a lot of counterintuitive behaviors, which are impossible to exist in the framework of the Hermitian system. We study the effect of a non-Hermitian impurity on the Hubbard model in the context of $\ensuremath{\eta}$ symmetry. We show that the non-Hermitian Hubbard Hamiltonian can respect a full real spectrum even if a local non-Hermitian impurity is applied to. The balance between dissipation of single fermion and on-site pair fluctuation results in a highest-order coalescing state with off-diagonal long-range order (ODLRO). Based on the characteristic of high-order EP, the critical non-Hermitian Hubbard model allows the generation of such a steady superconducting-like state through the time evolution from an arbitrary initial state, including the vacuum state. Remarkably, this dynamic scheme is insensitive to the on-site interaction and entirely independent of the locations of particle dissipation and pair fluctuation. Our results lay the groundwork for the dynamical generation of a steady ODLRO state through the critical non-Hermitian strongly correlated system.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Quantum Mechanics and Non-Hermitian Physics · Quantum, superfluid, helium dynamics · Quantum chaos and dynamical systems
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
References (65)
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1. 10.1080/00018732.2014.93350210.1080/00018732.2014.933502 ↗
2. 10.1103/PhysRevLett.68.58010.1103/PhysRevLett.68.580 ↗
3. 10.1103/PhysRevLett.116.13390310.1103/PhysRevLett.116.133903 ↗
4. 10.1103/PhysRevLett.121.02680810.1103/PhysRevLett.121.026808 ↗
5. 10.1103/PhysRevLett.121.13680210.1103/PhysRevLett.121.136802 ↗
6. 10.1103/PhysRevX.8.03107910.1103/PhysRevX.8.031079 ↗
7. 10.1038/nphys432310.1038/nphys4323 ↗
8. 10.1103/PhysRevLett.121.20300110.1103/PhysRevLett.121.203001 ↗
9. 10.1103/PhysRevLett.121.02640310.1103/PhysRevLett.121.026403 ↗
10. 10.1103/PhysRevB.98.03514110.1103/PhysRevB.98.035141 ↗
11. 10.1103/PhysRevB.99.12110110.1103/PhysRevB.99.121101 ↗
12. 10.1126/science.aaw820510.1126/science.aaw8205 ↗
13. 10.1103/PhysRevLett.123.12360110.1103/PhysRevLett.123.123601 ↗
14. 10.1103/PhysRevLett.123.17040110.1103/PhysRevLett.123.170401 ↗
15. 10.1103/PhysRevB.99.08110210.1103/PhysRevB.99.081102 ↗
16. 10.1103/PhysRevLett.123.09060310.1103/PhysRevLett.123.090603 ↗
17. 10.1103/PhysRevLett.123.06640510.1103/PhysRevLett.123.066405 ↗
18. 10.1038/s41467-018-08254-y10.1038/s41467-018-08254-y ↗
19. 10.1103/PhysRevLett.123.01680510.1103/PhysRevLett.123.016805 ↗
20. 10.1103/PhysRevLett.123.06640410.1103/PhysRevLett.123.066404 ↗
21. 10.1103/PhysRevLett.122.18530110.1103/PhysRevLett.122.185301 ↗
22. 10.1103/PhysRevB.101.04513010.1103/PhysRevB.101.045130 ↗
23. 10.1103/PhysRevResearch.2.03301810.1103/PhysRevResearch.2.033018 ↗
24. 10.1103/PhysRevLett.118.04570110.1103/PhysRevLett.118.045701 ↗
25. 10.1103/PhysRevB.98.08512610.1103/PhysRevB.98.085126 ↗
26. 10.1103/PhysRevB.102.08111510.1103/PhysRevB.102.081115 ↗
27. 10.1103/PhysRevLett.123.09770110.1103/PhysRevLett.123.097701 ↗
28. 10.1038/nphys107310.1038/nphys1073 ↗
29. 10.1103/PhysRevA.78.04230710.1103/PhysRevA.78.042307 ↗
30. 10.1038/nature1652210.1038/nature16522 ↗
31. 10.1103/PhysRevB.96.08510410.1103/PhysRevB.96.085104 ↗
32. 10.1103/PhysRevB.102.16513610.1103/PhysRevB.102.165136 ↗
33. 10.1103/PhysRevB.100.15513010.1103/PhysRevB.100.155130 ↗
34. 10.1023/B:CJOP.0000044002.05657.0410.1023/B:CJOP.0000044002.05657.04 ↗
35. 10.1088/1751-8113/45/44/44401610.1088/1751-8113/45/44/444016 ↗
36. 10.1126/science.aar770910.1126/science.aar7709 ↗
37. 10.1103/PhysRevB.101.04541510.1103/PhysRevB.101.045415 ↗
38. 10.1038/nature1860510.1038/nature18605 ↗
39. 10.1038/nature1860410.1038/nature18604 ↗
40. 10.1038/nature2240410.1038/nature22404 ↗
41. 10.1103/PhysRevLett.112.20390110.1103/PhysRevLett.112.203901 ↗
42. 10.1103/PhysRevA.93.03380910.1103/PhysRevA.93.033809 ↗
43. 10.1038/nature2328010.1038/nature23280 ↗
44. 10.1038/nature2328110.1038/nature23281 ↗
45. 10.1103/PhysRevX.6.02100710.1103/PhysRevX.6.021007 ↗
46. 10.1103/PhysRevB.99.24140310.1103/PhysRevB.99.241403 ↗
47. 10.1103/PhysRevA.99.06361610.1103/PhysRevA.99.063616 ↗
48. 10.1103/PhysRevB.101.22430110.1103/PhysRevB.101.224301 ↗
49. 10.1038/s41467-019-09757-y10.1038/s41467-019-09757-y ↗
50. 10.1103/PhysRevLett.123.03060310.1103/PhysRevLett.123.030603 ↗
51. 10.1103/PhysRevLett.122.07700210.1103/PhysRevLett.122.077002 ↗
52. 10.1126/science.119729410.1126/science.1197294 ↗
53. 10.1038/nmat396310.1038/nmat3963 ↗
54. 10.1103/PhysRevB.89.18451610.1103/PhysRevB.89.184516 ↗
55. 10.1038/s41567-018-0134-810.1038/s41567-018-0134-8 ↗
56. 10.1088/1367-2630/ab3acf10.1088/1367-2630/ab3acf ↗
57. 10.1038/s41567-019-0698-y10.1038/s41567-019-0698-y ↗
58. 10.1103/PhysRevLett.125.13700110.1103/PhysRevLett.125.137001 ↗
59. 10.1103/PhysRevX.4.04100110.1103/PhysRevX.4.041001 ↗
60. 10.1126/science.aaa743210.1126/science.aaa7432 ↗
61. 10.1103/RevModPhys.34.69410.1103/RevModPhys.34.694 ↗
62. 10.1103/PhysRevLett.63.214410.1103/PhysRevLett.63.2144 ↗
63. 10.1103/PhysRevA.85.01210610.1103/PhysRevA.85.012106 ↗
64. 10.1103/PhysRevA.94.05383410.1103/PhysRevA.94.053834 ↗
65. 10.1103/PhysRevB.98.08530610.1103/PhysRevB.98.085306 ↗