Open Access Paper
17 November 2017 Highly frequency-stabilized laser for space gravitational wave detector DECIGO/DPF
Aru Suemasa, Ken'ichi Nakagawa, Mitsuru Musha
Author Affiliations +
Proceedings Volume 10563, International Conference on Space Optics — ICSO 2014; 105632V (2017) https://doi.org/10.1117/12.2304209
Event: International Conference on Space Optics — ICSO 2014, 2014, Tenerife, Canary Islands, Spain
Abstract
Direct detections of gravitational wave (GW) by using a long-baseline laser interferometer have been tried in many countries. In Japan, a space-GW detector named DECIGO (Deci-hertz interferometer Gravitational wave detector), and its milestone mission DPF (DECIGO pathfinder) has been promoted. We have developed a spaceborne highly frequency-stabilized light source for DECIGO and DPF with high mechanical stability, long-term stable operation, high-efficiency and compactness. The frequency of an Yb doped fiber DFB laser at 1030 nm was locked to the saturated absorption signal of the iodine molecule (I2) at 515 nm. We have developed the breadboard model 1 (BBM1) of the I2 stabilized Yb:fiber laser, which was installed on a 550x300x20-mm aluminum plate. The frequency noise of the laser was suppressed down to 0.4 Hz/Hz1/2 at 1 Hz which was evaluated from the frequency error signal. In the present paper, we will report the details and performance of the BBM1 of the light source for DECIGO and DPF.
© (2017) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Aru Suemasa, Ken'ichi Nakagawa, and Mitsuru Musha "Highly frequency-stabilized laser for space gravitational wave detector DECIGO/DPF", Proc. SPIE 10563, International Conference on Space Optics — ICSO 2014, 105632V (17 November 2017); https://doi.org/10.1117/12.2304209
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Cited by 2 scholarly publications.
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KEYWORDS
Light sources

Absorption

Sensors

Laser stabilization

Signal detection

Signal to noise ratio

Fiber lasers

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