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    Nature of momentum- and orbital-dependent magnetic fluctuations in Sr2RuO4

    Maria Chatzieleftheriou1,2, Alexander N. Rudenko3, Yvan Sidis4, Silke Biermann1,5,6, and Evgeny A. Stepanov1,5

    Phys. Rev. B 112, 195118 – Published 13 November, 2025

    DOI: https://doi.org/10.1103/ts6y-zb6m

    Abstract

    The quasi-two-dimensional material Sr2RuO4 is a paradigmatic example of a correlated system that exhibits unconventional superconductivity and intriguing magnetic properties. The interplay between these two effects and the resulting strength and nature of spin fluctuations and their role for the properties of the compound have sparked significant debates. Here, elaborating a theory that self-consistently incorporates spatial magnetic fluctuations into a realistic many-body description, we show that these fluctuations significantly reduce many-body correlations in the system, thereby preventing magnetic ordering in Sr2RuO4, in agreement with experimental observations. Our conclusion is supported by a theoretical calculation of the spin susceptibility that closely matches the experimental results. We obtain finite peaks at the incommensurate wave vectors, a broad dome-shaped structure centered around the Γ point, and a diminished magnetic response at the edges of the BZ. We identify the orbital character of the unusual dome structure as resulting predominantly from the 2D-like xy orbital, which is believed to be responsible for the superconductivity.

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