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Time delay interferometry with a transfer oscillator.

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    This study demonstrates a new time delay interferometry method using a transfer oscillator for simultaneous laser frequency and clock noise reduction. This technique achieves significant noise suppression, meeting requirements for space-borne gravitational wave detection.

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    Area of Science:

    • Physics
    • Astronomy
    • Metrology

    Background:

    • Accurate frequency measurements are crucial for advanced scientific applications like gravitational wave detection.
    • Laser frequency noise and clock noise are significant challenges in high-precision interferometry.

    Purpose of the Study:

    • To develop and experimentally validate a novel time delay interferometry (TDI) technique for simultaneous reduction of laser frequency noise and clock noise.
    • To assess the performance of this new TDI method for space-borne gravitational wave detection.

    Main Methods:

    • Utilized a transfer oscillator for coherent downconversion of an iodine frequency reference to microwave frequencies using a laser frequency comb.
    • Employed an electrical delay module to introduce large time delays for time delay interferometry.
    • Post-processing techniques were applied to reduce residual noise.

    Main Results:

    • Achieved simultaneous reduction of laser frequency noise by ten orders of magnitude and clock noise by three orders of magnitude in the 0.1 mHz to 0.1 Hz frequency band.
    • Demonstrated noise reduction performance reaching 6 × 10-8 Hz/Hz1/2 at 0.1 mHz and 7 × 10-7 Hz/Hz1/2 at 1 mHz.
    • Confirmed high homology between optical and microwave frequencies with residual downconversion noise below 5 × 10-6 Hz/Hz1/2.

    Conclusions:

    • The developed transfer oscillator-based time delay interferometry effectively reduces both laser frequency and clock noise.
    • The achieved noise reduction performance meets the stringent requirements for future space-borne gravitational wave detectors.
    • This method offers a promising alternative for frequency comb-based TDI in next-generation gravitational wave observatories.