Quasiparticle tunneling and 1/f charge noise in ultrastrongly coupled superconducting qubit and resonator
Source abstract
Abstract
We report on an experimentally observed doubly split spectrum and its split-width fluctuation due to charge fluctuation in an ultrastrongly coupled superconducting qubit and resonator. From an analysis of the circuit model Hamiltonian, we found that the doubly split spectrum and split-width fluctuation are caused by discrete charge hops due to quasiparticle tunneling and a continuous background charge fluctuation in islands of a flux qubit. During 70 h of spectrum measurement, the split width fluctuated but the middle frequency of the split was constant. This observation indicates that the quasiparticles in our device mainly tunnel in one particular junction, as expected from the energy difference between quasiparticle states, during this 70 h. The background offset charge obtained from the split width has the $1/f$ noise characteristic.
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Research context
OpenAlex topics: Quantum and electron transport phenomena · Quantum Information and Cryptography · Quantum Computing Algorithms and Architecture
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Department of Physics, Tokyo University of Science, 1–3 Kagurazaka, Shinjuku, Tokyo 162–0825, Japan
RIKEN Center for Quantum Computing (RQC), 2–1 Hirosawa, Wako, Saitama 351–0198, Japan
Advanced ICT Research Institute, National Institute of Information and Communications Technology, 4-2-1, Nukuikitamachi, Koganei, Tokyo 184-8795, Japan
Funding
New Energy and Industrial Technology Development Organization · Japan Science and Technology Agency
References (58)
Show source-provided references
1. 10.1103/PhysRevA.69.06232010.1103/PhysRevA.69.062320 ↗
2. 10.1038/s42254-018-0006-210.1038/s42254-018-0006-2 ↗
3. 10.1146/annurev-conmatphys-031119-05060510.1146/annurev-conmatphys-031119-050605 ↗
4. 10.1038/s41586-019-1666-510.1038/s41586-019-1666-5 ↗
5. 10.1103/PhysRevLett.93.26700710.1103/PhysRevLett.93.267007 ↗
6. 10.1103/PhysRevB.89.02050310.1103/PhysRevB.89.020503 ↗
7. 10.1103/PhysRevB.85.17452110.1103/PhysRevB.85.174521 ↗
8. 10.1088/1361-6633/ab3a7e10.1088/1361-6633/ab3a7e ↗
9. 10.1103/PhysRevLett.121.15770110.1103/PhysRevLett.121.157701 ↗
10. 10.1063/5.002973510.1063/5.0029735 ↗
11. 10.1103/PhysRevB.100.14050310.1103/PhysRevB.100.140503 ↗
12. 10.1038/ncomms293610.1038/ncomms2936 ↗
13. 10.1103/PhysRevB.77.18050210.1103/PhysRevB.77.180502 ↗
14. 10.1103/PhysRevB.74.06451510.1103/PhysRevB.74.064515 ↗
15. 10.1103/PhysRevB.84.06451710.1103/PhysRevB.84.064517 ↗
16. 10.1038/1971810.1038/19718 ↗
17. 10.1103/PhysRevA.76.04231910.1103/PhysRevA.76.042319 ↗
18. 10.1063/1.220755510.1063/1.2207555 ↗
19. 10.1103/PhysRevLett.53.31910.1103/PhysRevLett.53.319 ↗
20. 10.1103/PhysRevLett.88.05040310.1103/PhysRevLett.88.050403 ↗
21. 10.1038/s41567-018-0097-910.1038/s41567-018-0097-9 ↗
22. 10.1103/PhysRevLett.95.25700210.1103/PhysRevLett.95.257002 ↗
23. 10.1103/PhysRevLett.113.12360110.1103/PhysRevLett.113.123601 ↗
24. 10.1103/PhysRevB.91.19543410.1103/PhysRevB.91.195434 ↗
25. 10.1103/RevModPhys.91.02500510.1103/RevModPhys.91.025005 ↗
26. 10.1103/PhysRevLett.108.12050110.1103/PhysRevLett.108.120501 ↗
27. 10.1038/s41534-020-00294-x10.1038/s41534-020-00294-x ↗
28. 10.1038/srep4425110.1038/srep44251 ↗
29. 10.1103/PhysRevLett.107.19040210.1103/PhysRevLett.107.190402 ↗
30. 10.1103/PhysRevB.91.06450310.1103/PhysRevB.91.064503 ↗
31. 10.7566/JPSJ.88.06101110.7566/JPSJ.88.061011 ↗
32. 10.1088/1367-2630/aaeeea10.1088/1367-2630/aaeeea ↗
33. 10.1103/PhysRevA.97.03382310.1103/PhysRevA.97.033823 ↗
34. 10.1038/nphys390610.1038/nphys3906 ↗
35. 10.1103/PhysRevA.95.05382410.1103/PhysRevA.95.053824 ↗
36. 10.1038/nphys173010.1038/nphys1730 ↗
37. 10.7717/peerj.45310.7717/peerj.453 ↗
38. 10.1103/PhysRevLett.123.19050210.1103/PhysRevLett.123.190502 ↗
39. 10.1103/PhysRevB.91.09451710.1103/PhysRevB.91.094517 ↗
40. 10.1103/PhysRevB.73.17452610.1103/PhysRevB.73.174526 ↗
41. 10.1103/PhysRevLett.111.24360210.1103/PhysRevLett.111.243602 ↗
42. 10.1103/PhysRevA.80.03210910.1103/PhysRevA.80.032109 ↗
43. 10.1038/nphys390510.1038/nphys3905 ↗
44. 10.1103/PhysRevLett.113.24700110.1103/PhysRevLett.113.247001 ↗
45. 10.1103/PhysRevLett.92.06680210.1103/PhysRevLett.92.066802 ↗
46. 10.1103/PhysRevB.53.823410.1103/PhysRevB.53.8234 ↗
47. 10.1103/PhysRevLett.69.199710.1103/PhysRevLett.69.1997 ↗
48. 10.1126/science.aah584410.1126/science.aah5844 ↗
49. 10.1126/science.280.5367.123810.1126/science.280.5367.1238 ↗
50. 10.1063/1.36008310.1063/1.360083 ↗
51. 10.1103/PhysRevA.81.04231110.1103/PhysRevA.81.042311 ↗
52. 10.1016/S1361-8415(98)80009-110.1016/S1361-8415(98)80009-1 ↗
53. 10.1103/PhysRevLett.35.43210.1103/PhysRevLett.35.432 ↗
54. 10.1038/s41567-019-0534-410.1038/s41567-019-0534-4 ↗
55. 10.1038/srep1605510.1038/srep16055 ↗
56. 10.1103/PhysRevApplied.12.01405210.1103/PhysRevApplied.12.014052 ↗
57. 10.1063/1.369207310.1063/1.3692073 ↗
58. 10.1063/1.490793510.1063/1.4907935 ↗