Laser intensity noise suppression for space-borne gravitational wave mission

Laser intensity noise is a main limitation of measurement and sensing missions represented by gravitational wave detection. We develop a noise decomposition model and design the core elements of the feedback loop based on the analysis results. We construct a fiber amplifier system with ultra-low intensity noise in the 0.1 mHz-1 Hz frequency band by the employment of an optoelectronic feedback loop that is specially designed, achieving a relative intensity noise below 6×10<sup>-5</sup>/[email protected] mHz-1 Hz. By precise control of the temperature, we improve the temperature and mechanical stability of the fiber amplifier chain. Although the differential phase noise violates the LISA requirement in the 1 mHz-50 mHz frequency band, it meets the requirement at all other frequencies within the measurement range. The study provides an experimental basis and technologies for precise measurement and sensing systems at ultra-low frequency.

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Publication Details

Journal
Optics Express
Published
2025-06-13
DOI
https://doi.org/10.1364/oe.550808
Citations
6
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
Field-Weighted Citation Impact
6.93

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article

Laser intensity noise suppression for space-borne gravitational wave mission

jiawei wang, Xin Shang, Yaohui Zheng, Shaoping Shi et al.
6 citations
Optics Express
Pulsars and Gravitational Waves Research
6.93
article

Laser intensity noise suppression for space-borne gravitational wave mission

jiawei wang, Xin Shang, Yaohui Zheng, Shaoping Shi, Fan Li, Yuhang Li, Yajun Wang, Wangbao Yin, Long Tian, Zhenglei Ma
article en
6 citations

Abstract

Laser intensity noise is a main limitation of measurement and sensing missions represented by gravitational wave detection. We develop a noise decomposition model and design the core elements of the feedback loop based on the analysis results. We construct a fiber amplifier system with ultra-low intensity noise in the 0.1 mHz-1 Hz frequency band by the employment of an optoelectronic feedback loop that is specially designed, achieving a relative intensity noise below 6×10<sup>-5</sup>/[email protected] mHz-1 Hz. By precise control of the temperature, we improve the temperature and mechanical stability of the fiber amplifier chain. Although the differential phase noise violates the LISA requirement in the 1 mHz-50 mHz frequency band, it meets the requirement at all other frequencies within the measurement range. The study provides an experimental basis and technologies for precise measurement and sensing systems at ultra-low frequency.

Optics ExpressVol. 33(13)
Shanxi University of Traditional Chinese Medicine (CN), Tsinghua University (CN)
National Natural Science Foundation of China, National Key Research and Development Program of China
Climate action
Openalex Percentile: Top 3%
Pulsars and Gravitational Waves Research
6.93
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Laser intensity noise suppression for space-borne gravitational wave mission — jiawei wang, Xin Shang, et al. · Optics Express (2025) | TGRS Research Map | TGRS