Coherent quantum network of superconducting qubits as a highly sensitive detector of microwave photons for searching of galactic axions
We propose a novel approach to detect a low power microwave signal with a frequency of the order of several GHz based on a coherent collective response of quantum states occurring in a superconducting qubits network (SQN). An SQN composes of a large number of superconducting qubits embedded in a low-dissipative superconducting resonator. Our theory predicts that an SQN interacting with the off-resonance microwave radiation, demonstrates the collective alternating current Stark effect that can be measured even in the limit of single photon counting. A design of the layout of three terminals SQN detectors containing 10 flux qubits weakly coupled to a low-dissipative R-resonator and T-transmission line was developed. The samples were fabricated by Al-based technology with Nb resonator. The SQN detector was tested in terms of microwave measurements of scattering parameters and two-tone spectroscopy. A substantial shift of the frequency position of the transmission coefficient drop induced by a second tone pump signal was observed, and this effect clearly manifests a nonlinear multiphoton interaction between the second-tone microwave pump signal and an array of qubits.
Funding
Highly sensitive detection of single microwave photons with coherent quantum network of superconducting qubits for searching galactic axions
European Commission
Find out more...History
School
- Science
Department
- Physics
Published in
IEEE Transactions on Applied SuperconductivityVolume
33Issue
5Source
Applied Superconductivity Conference 2022 (ASC 2022)Publisher
IEEEVersion
- VoR (Version of Record)
Rights holder
© The AuthorsPublisher statement
This is an Open Access Article. It is published by IEEE under the Creative Commons Attribution 4.0 International Licence (CC BY). Full details of this licence are available at: https://creativecommons.org/licenses/by/4.0/Acceptance date
2023-03-22Publication date
2023-04-06Copyright date
2023ISSN
1051-8223eISSN
1558-2515Publisher version
Language
- en