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
Related works
- Is new version of
- Discussion Paper: arXiv:2408.16171 (arXiv)
Funding
- National Science Foundation
- PHY-2110455
Dates
- Accepted
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2024-11-07Accepted
- Available
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2024-11-07Posted
- Available
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2024-12-04Published