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Experimental demonstration of deep frequency modulation interferometry.

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    Deep frequency modulation interferometry offers a scalable solution for precise position readout in gravitational wave detectors. This new technique achieves 250 pm/√Hz displacement sensitivity, simplifying complex optical setups.

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    Area of Science:

    • Physics
    • Optics
    • Astronomy

    Background:

    • Gravitational wave detectors require high-precision, large dynamic range interferometric position readout.
    • Existing heterodyne interferometer schemes are complex and lack scalability for multi-channel applications.

    Purpose of the Study:

    • To introduce and experimentally validate deep frequency modulation interferometry as a simpler, scalable alternative.
    • To assess the performance and linearity of this novel interferometric technique.

    Main Methods:

    • Utilizing sinusoidal laser frequency modulation in unequal arm length interferometers.
    • Implementing a non-linear fit algorithm for phase tracking and signal analysis.
    • Testing the technique in Michelson and Mach-Zehnder interferometer configurations.

    Main Results:

    • Demonstrated continuous phase tracking of a moving mirror.
    • Achieved a displacement sensitivity of 250 pm/√Hz at 1 mHz.
    • Measured laser frequency modulation linearity to be within 2% for the tested laser source.

    Conclusions:

    • Deep frequency modulation interferometry is a promising technique for high-precision position sensing.
    • The method offers improved scalability and reduced optical complexity compared to traditional approaches.
    • Experimental validation confirms its potential for gravitational wave detection and other sensitive measurements.