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    Next-generation gravitational wave detectors using diffractive optics require precise alignment. A new framework using Gaussian beam modal decomposition clarifies phase changes, ensuring stability for these advanced interferometers.

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    Area of Science:

    • Optics and Gravitational Wave Detection
    • Interferometry with Diffractive Optics

    Background:

    • Next-generation gravitational wave detectors are exploring all-reflective interferometer designs using diffractive elements instead of transmissive optics.
    • This shift introduces new challenges, particularly increased phase noise and stringent alignment stability requirements.

    Purpose of the Study:

    • To develop a framework for analyzing alignment stability in all-reflective interferometers utilizing diffractive elements.
    • To investigate the phase changes associated with beam and grating displacements within such systems using a Gaussian beam model.

    Main Methods:

    • Development of an alignment stability framework based on Gaussian beam modal decomposition.
    • Experimental verification of the phase independence of a diffracted Gaussian beam from its shape.
    • Rigorous time-domain simulations to interpret phase changes derived from modal decomposition.

    Main Results:

    • The modal decomposition framework successfully models small beam or grating displacements.
    • The modal model reveals phase changes that differ from a purely geometric planewave approach.
    • Experimental results confirm that the phase of a diffracted Gaussian beam is independent of its shape.
    • Simulations demonstrate that modal decomposition phase changes align with geometric planewave models when the coordinate system is simultaneously adjusted.

    Conclusions:

    • The developed framework provides a method to analyze alignment stability in diffractive interferometers.
    • Accurate interpretation of phase changes requires careful consideration of the coordinate system in relation to beam displacement.
    • Findings are crucial for the design and stability of future gravitational wave observatories employing diffractive optics.