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Updated: May 30, 2026

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The Generation of Higher-order Laguerre-Gauss Optical Beams for High-precision Interferometry
Published on: August 12, 2013
Development of stable monolithic wide-field Michelson interferometers
Xiaoke Wan1, Jian Ge, Zhiping Chen
1Department of Astronomy, University of Florida, Bryant Space Science Center, Gainesville, Florida 32611, USA. xwan@astro.ufl.edu
Applied Optics
|July 21, 2011
Summary
Stable monolithic Michelson interferometers are crucial for exoplanet detection. Matching thermal expansion coefficients (CTEs) ensures interferometer stability, enabling precise radial velocity (RV) measurements for astronomical research.
Area of Science:
- Optics and Photonics
- Astronomy and Astrophysics
- Materials Science
Background:
- Wide-field Michelson interferometers are vital for high-precision remote sensing and astronomical applications.
- Stable monolithic Michelson interferometers are essential for accurate radial velocity (RV) measurements in exoplanet detection.
- Interferometer stability is critically dependent on minimizing thermal distortion.
Purpose of the Study:
- To present a novel design for a stable monolithic Michelson interferometer.
- To detail the design, fabrication, and testing processes for this interferometer.
- To demonstrate its suitability for high-precision radial velocity measurements.
Main Methods:
- Thermal stress analysis to identify critical design requirements.
- Material selection based on matching coefficients of thermal expansion (CTEs) using BK7 and LAK7.
- Fabrication and rigorous testing of the monolithic interferometer.
Main Results:
- A novel monolithic interferometer design free from thermal distortion was developed.
- The interferometer exhibits a field angle of 23.8° and thermal sensitivity of -2.6×10(-6)/°C near 550 nm.
- This sensitivity corresponds to approximately 800 m/s/°C in the RV scale.
Conclusions:
- Matching CTEs is critical for interferometer stability, enabling precise RV measurements.
- The developed low-cost interferometer demonstrates high stability for long-term operation in RV instruments.
- This technology supports ongoing exoplanet searching and characterization efforts.

