On the signature of the baryon-dark matter relative velocity in the two and three-point galaxy correlation functions
Zachary Slepian, Daniel Eisenstein

TL;DR
This paper explores how baryon-dark matter relative velocity affects galaxy correlation functions, revealing signatures in the 3PCF that can help correct BAO scale shifts for more accurate cosmological measurements.
Contribution
It introduces a configuration-space framework to identify the relative velocity signature in galaxy correlations and proposes a computationally efficient method to isolate this effect.
Findings
Relative velocity causes a shift in the BAO scale in the galaxy-galaxy correlation function.
Distinctive signatures of the relative velocity are identified in the 3PCF, especially in the l=1 multipole.
A simplified 3PCF compression scheme effectively isolates the relative velocity signature.
Abstract
We develop a configuration-space picture of the relative velocity between baryons and dark matter that clearly explains how it can shift the BAO scale in the galaxy-galaxy correlation function. The shift occurs because the relative velocity is non-zero only within the sound horizon and thus adds to the correlation function asymmetrically about the BAO peak. We further show that in configuration space the relative velocity has a localized, distinctive signature in the three-point galaxy correlation function (3PCF). In particular, we find that a multipole decomposition is a favorable way to isolate the relative velocity in the 3PCF, and that there is a strong signature in the l=1 multipole for triangles with 2 sides around the BAO scale. Finally, we investigate a further compression of the 3PCF to a function of only one triangle side that preserves the localized nature of the relative…
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