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arXiv · 2408.16171

Optical Spring Tracking for Enhancing Quantum-Limited Interferometers

Scott Aronson·Ronald Pagano·Torrey Cullen·Garrett D. Cole·Thomas Corbitt
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Abstract

Modern interferometers such as LIGO have achieved sensitivities limited by quantum noise, comprised of 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 dynamically tracking a target signal using an optical spring, resulting in an increased signal to noise ratio (SNR). We report on a SNR increase by up to a factor of 40 when compared to a static configuration.

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Scott Aronson, Ronald Pagano, Torrey Cullen, Garrett D. Cole, Thomas Corbitt. 2024-08-28. Optical Spring Tracking for Enhancing Quantum-Limited Interferometers. https://arxiv.org/abs/2408.16171

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