aiqbench analysis
This research presents a non-linear quantum interferometer utilizing superconducting circuits to surpass the standard shot noise limit, enabling higher sensitivity for detecting dark matter and gravitational waves. By advancing fundamental measurement techniques beyond linear constraints, this work directly expands the capabilities of quantum sensing infrastructure. The development of magnetic field-resilient anharmonic circuits represents a significant step forward in practical quantum hardware design.
Time domain non-linear quantum interferometry
arXiv:2609.13749v1 Announce Type: new Abstract: Interferometry is a powerful method for studying many fundamental phenomena ranging from gravitational waves to anyon excitations. Besides loss of coherence in the interferometer paths, quantum mechanics sets an incompressible bound for linear interferometry arising from the quantum noise of the light beam, called the shot noise limit. Here, we implement a non-linear quantum interferometer that uses a microwave cavity and a magnetic field resilient anharmonic superconducting quantum circuit made of granular aluminum. The circuit enables interferometry beyond the shot noise limit. A direct application of our findings is the detection of dark matter (axions or dark photons), high-frequency gravitational waves or astronomical masers.
Abstract:Interferometry is a powerful method for studying many fundamental phenomena ranging from gravitational waves to anyon excitations. Besides loss of coherence in the interferometer paths, quantum mechanics sets an incompressible bound for linear interferometry arising from the quantum noise of the light beam, called the shot noise limit. Here, we implement a non-linear quantum interferometer that uses a microwave cavity and a magnetic field resilient anharmonic superconducting quantum circuit made of granular aluminum. The circuit enables interferometry beyond the shot noise limit. A direct application of our findings is the detection of dark matter (axions or dark photons), high-frequency gravitational waves or astronomical masers.
Quantum Physics (quant-ph); Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
arXiv:2609.13749 [quant-ph]
(or arXiv:2609.13749v1 [quant-ph] for this version)
https://doi.org/10.48550/arXiv.2609.13749 Focus to learn more arXiv-issued DOI via DataCite (pending registration)
Phys. Rev. A 113, 023706 (2026)
https://doi.org/10.1103/f252-64sy Focus to learn more DOI(s) linking to related resources
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Full text under the publisher's open licence · 219 words
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