A bstract We analyze the influence of gravitational waves on a Sagnac interferometer formed by the interference of two counter-propagating beams traversing a closed spatial loop. In addition to the well-known Sagnac phase shift, we identify an additional contribution originating from a relative rotation in the polarization vectors. We formulate this effect as a gravitational holonomy associated to the internal Lorentz group. The magnitude of both effects is computed due to gravitational waves generated by a localized source far from the detector, at leading order in the inverse distance. For freely falling observers, the phase shift is zero and the polarization rotation becomes the dominant effect.
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Reza Javadinezhad
Ali Seraj
Journal of High Energy Physics
KU Leuven
Institute for Research in Fundamental Sciences
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Javadinezhad et al. (Wed,) studied this question.
www.synapsesocial.com/papers/69fd7fa1bfa21ec5bbf0834d — DOI: https://doi.org/10.1007/jhep05(2026)046