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On the Robustness of the Acoustic Scale in the Low‐Redshift Clustering of Matter

On the Robustness of the Acoustic Scale in the Low‐Redshift Clustering of Matter

We discuss the effects of non-linear structure formation on the signature of acoustic oscillations in the late-time galaxy distribution. We argue that the dominant non-linear effect is the differential motion of pairs of tracers separated by 150 Mpc. These motions are driven by bulk flows and cluster formation and are …