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Transponder-type laser interferometer prototype for spaceborne gravitational wave detectors.

Henglin Mu, Xin Xu, Taoran Le

    Applied Optics
    |March 4, 2024
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    This study introduces a prototype transponder-type laser interferometer for calibrating spaceborne gravitational wave detectors. The system demonstrates high stability, crucial for future missions like LISA.

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    Area of Science:

    • Astrophysics
    • Optical Engineering
    • Metrology

    Background:

    • Spaceborne laser interferometry is vital for gravitational wave detection.
    • Accurate noise calibration is critical for enhancing detector sensitivity.

    Purpose of the Study:

    • To develop and characterize a transponder-type laser interferometer prototype.
    • To assess its suitability for noise calibration in spaceborne gravitational wave detectors.

    Main Methods:

    • Utilized a digital optical phase-locked loop to synchronize master and slave lasers.
    • Established a transponder-type laser interferometer link between two simulated satellites.
    • Analyzed measurement stability and noise characteristics, including Allan deviation and noise spectral density.

    Main Results:

    • Achieved phase locking between master and slave lasers.
    • Demonstrated an Allan deviation of 243.2 pm at 0.429 s for zero drift.
    • Measured a noise spectral density floor of 21 pm/√Hz at 1 Hz.
    • Identified temperature drift as a key performance limitation below 2 mHz.

    Conclusions:

    • The prototype shows promising stability and noise performance for gravitational wave detection.
    • Temperature drift is a significant factor affecting low-frequency performance.
    • The design serves as a valuable reference for missions like LISA and inter-satellite applications.