The effect of relative velocity and density perturbations between baryons and dark matter on the clustering of galaxies
Fabian Schmidt

TL;DR
This paper analyzes how pre-recombination baryon-dark matter perturbations affect galaxy clustering and BAO measurements, providing a comprehensive perturbative framework including new terms in the galaxy power spectrum.
Contribution
It offers a complete perturbative treatment of baryon-CDM perturbations on galaxy clustering, including new terms in the galaxy power spectrum at 1-loop order.
Findings
Relative-density perturbation $oldsymbol{ extdelta_{bc}}$ dominates effects.
Velocity perturbation $oldsymbol{ heta_{bc}}$ contributes to galaxy bias.
New terms in the galaxy power spectrum at 1-loop order are derived.
Abstract
Pre-recombination acoustic oscillations induce non-adiabatic perturbations between baryons and dark matter, corresponding to a constant relative-density and decaying relative-velocity perturbation . Due to their significant large-scale correlations and prominent baryon acoustic oscillation (BAO) features, these modes are potentially important for the use of the BAO as standard ruler. We present a complete treatment of the effects of the baryon-CDM perturbations on galaxy clustering in the context of a rigorous perturbative bias expansion. The leading effects are proportional to and . We estimate the magnitude of these terms through the excursion set approach. The contribution from , which has attracted significant attention recently, contributes at subleading (1-loop) order. The relative-density…
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