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The Generation of Higher-order Laguerre-Gauss Optical Beams for High-precision Interferometry
Published on: August 12, 2013
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Design and Construction of the Optical Bench Interferometer for the Taiji Program.
Wei Tao1,2,3, Xiaoqin Deng1,2,3, Yuqing Diao1,2,3
1Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences, Changchun 130033, China.
Sensors (Basel, Switzerland)
|November 25, 2023
Summary
A novel two-sided optical bench interferometer (OBI) was developed for space gravitational wave detection. This advanced OBI meets the stringent noise requirements for the Taiji Program, crucial for detecting cosmic ripples.
Area of Science:
- Astrophysics and Cosmology
- Optical Engineering
- Gravitational Wave Detection
Background:
- Space-based gravitational wave detection requires highly sensitive interferometers.
- The Taiji Program aims to detect gravitational waves in space, necessitating specialized instrumentation.
- Existing interferometers may not meet the specific demands for space missions.
Purpose of the Study:
- To design and construct a full-function two-sided optical bench interferometer (OBI).
- To meet the practical requirements of the Taiji Program for space gravitational wave detection.
- To achieve low noise levels essential for detecting gravitational waves in space.
Main Methods:
- Designed a two-sided OBI with main optical paths on the A-side and auxiliary components on the B-side.
- Utilized hydrogen-oxygen catalytic stress-free bonding technology for construction.
- Employed a self-designed precision mechanical clamping mechanism and beam position measuring device for alignment.
Main Results:
- Successfully constructed two functional OBIs.
- Controlled position and angle errors of the interference beam within 30 μm and 50 μrad.
- Stability tests in a vacuum tank on a vibration isolation platform showed OBI noise below 10 pm/√Hz (0.1 Hz to 1 Hz).
Conclusions:
- The developed OBI meets the noise budget requirements for the Taiji Pathfinder in the middle- and high-frequency bands.
- The stress-free bonding technology and precision alignment mechanisms are effective for constructing sensitive optical instruments.
- This OBI design is a significant advancement for future space-based gravitational wave observatories.

