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The spin susceptibility of strongly correlated Sr 2 RuO 4 is known to display a rich structure in reciprocal space, with a prominent peak at . It is still debated if the resulting incommensurate spin-density-wave fluctuations foster unconventional superconductivity at low temperature or compete therewith. By means of density functional theory combined with dynamical mean-field theory, we reveal the realistic multi-orbital signature of the (dynamic) spin susceptibility beyond existing weak-coupling approaches. The experimental fluctuation spectrum up to 80 meV is confirmed by theory. Furthermore, the peak at Q i is shown to carry nearly equal contributions from each of the Ru orbitals, pointing to a cooperative effect resulting in the dominant spin fluctuations.
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