Removing BAO-peak Shifts with Local Density Transforms
Nuala McCullagh, Mark C. Neyrinck, Istv\'an Szapudi, Alexander S., Szalay

TL;DR
This paper investigates how local density transforms, like the logarithm, can reduce BAO peak shifts caused by large-scale flows, improving the accuracy of cosmological measurements.
Contribution
It demonstrates that applying a log-density transform significantly diminishes BAO peak shifts in the correlation function, offering a new method to correct for bulk flow distortions.
Findings
Log-density correlation shows smaller BAO peak shift at low redshift.
Displaced-initial-density field further reduces peak shift.
Reciprocal density pushes the peak outward, increasing shift.
Abstract
Large-scale bulk flows in the Universe distort the initial density field, broadening the baryon-acoustic-oscillation (BAO) feature that was imprinted when baryons were strongly coupled to photons. Additionally, there is a small shift inward in the peak of the conventional overdensity correlation function, a mass-weighted statistic. This shift occurs when high density peaks move toward each other. We explore whether this shift can be removed by applying to the density field a transform (such as a logarithm) that gives fairer statistical weight to fluctuations in underdense regions. Using configuration-space perturbation theory in the Zel'dovich approximation, we find that the log-density correlation function shows a much smaller inward shift in the position of the BAO peak at low redshift than is seen in the overdensity correlation function. We also show that if the initial, Lagrangian…
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