Optical spring tracking for enhancing quantum-limited interferometers
Abstract
Modern interferometers such as LIGO have achieved sensitivities limited by quantum noise, comprising radiation pressure and shot noise. To mitigate this noise, a static system is employed that minimizes the quantum noise within the measurement band. However, since gravitational wave inspiral signals are a single frequency changing over time, only noise at the chirp frequency needs to be minimized. Here we demonstrate a proof-of-principle experiment of dynamically tracking a target signal using an optical spring, resulting in an increased signal-to-noise ratio (SNR). By injecting white noise to simulate excess shot noise, we found the SNR increased by up to a factor of 40 via dynamical tracking when compared to a static configuration.
Copyright and License
© 2024 Optica Publishing Group. All rights, including for text and data mining (TDM), Artificial Intelligence (AI) training, and similar technologies, are reserved.
Funding
National Science Foundation (PHY-2110455).
Data Availability
Data underlying the results presented in this Letter are not publicly available at this time but may be obtained from the authors upon reasonable request.
Additional details
- National Science Foundation
- PHY-2110455
- Accepted
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2024-11-07Accepted
- Available
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2024-11-07Posted
- Available
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2024-12-04Published
- Caltech groups
- LIGO
- Publication Status
- Published