Presentation + Paper
5 March 2021 2 μm ultra-low relative intensity noise and frequency noise of single frequency fiber laser for next-generation gravitational wave detectors
Qian Zhang, Yubin Hou, Weihua Song, Xi Wang, Zhigang Peng, Xu Chen, Carl Blair, Ju Li, Chunnong Zhao, Pu Wang
Author Affiliations +
Abstract
We demonstrated an ultra-low noise polarization-maintaining (PM) single frequency fiber laser (SFFL) at 2 μm. By suppressing the pump relative intensity noise (RIN) using a feedback loop control, the RIN and frequency noise of the SFFL are simultaneously reduced, and the reduction is about 3 - 15 dB and 3 - 8.4 dB, respectively. After two stage Tm3+-doped PM fiber amplifier, the output power reached about 5 W. Meanwhile, the frequency noise almost has no increases, which is still below 100 Hz/√Hz after 13 Hz. And the frequency-tunable range is approximately 2 GHz with frequency response of 46 MHz/V.
Conference Presentation
© (2021) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Qian Zhang, Yubin Hou, Weihua Song, Xi Wang, Zhigang Peng, Xu Chen, Carl Blair, Ju Li, Chunnong Zhao, and Pu Wang "2 μm ultra-low relative intensity noise and frequency noise of single frequency fiber laser for next-generation gravitational wave detectors", Proc. SPIE 11665, Fiber Lasers XVIII: Technology and Systems, 116650D (5 March 2021); https://doi.org/10.1117/12.2579001
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KEYWORDS
Fiber lasers

Sensors

Fiber amplifiers

Ferroelectric materials

Laser sources

LIGO

Optical amplifiers

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