Optical spring tracking for enhancing quantum-limited interferometers
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.
Authors
- T. R. Corbitt (ORCID: https://orcid.org/0000-0002-5520-8541)
- T. J. Cullen (ORCID: https://orcid.org/0000-0001-8075-4088)
- Garrett D. Cole (ORCID: https://orcid.org/0000-0001-7149-3218)
- Scott Aronson (ORCID: https://orcid.org/0000-0001-7080-8177)
- R. Pagano (ORCID: https://orcid.org/0000-0001-8362-0130)
Institutions
- California Institute of Technology (US)
- Thorlabs (Germany) (DE)
Publication Details
- Journal
- Optics Letters
- Published
- 2024-11-07
- DOI
- https://doi.org/10.1364/ol.540195
- Citations
- 5
- Primary Topic
- Pulsars and Gravitational Waves Research
- Type
- article
- Field-Weighted Citation Impact
- 1.66
Funders
- National Science Foundation