New Photodetection Method Using Unbalanced Sidebands for Squeezed Quantum Noise in Gravitational Wave Interferometer
K. Somiya

TL;DR
This paper proposes a novel heterodyne detection method with unbalanced sidebands to achieve quantum-non-demolition measurement in gravitational wave detectors, offering broadband capabilities and potentially surpassing traditional homodyne detection.
Contribution
It introduces a new heterodyne detection scheme with unbalanced sidebands that mimics homodyne quantum-non-demolition effects and enables broadband readout in gravitational wave interferometers.
Findings
Heterodyne detection with unbalanced sidebands can realize quantum-non-demolition effects.
The scheme allows broadband quantum-non-demolition readout.
Potential for improved gravitational wave detection sensitivity.
Abstract
Homodyne detection is one of the ways to circumvent the standard quantum limit for a gravitational wave detector. In this paper it will be shown that the same quantum-non-demolition effect using homodyne detection can be realized by heterodyne detection with unbalanced RF sidebands. Furthermore, a broadband quantum-non-demolition readout scheme can also be realized by the unbalanced sideband detection.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
