The Shift of the Baryon Acoustic Oscillation Scale: A Simple Physical Picture
Blake D. Sherwin, Matias Zaldarriaga

TL;DR
This paper explains the physical reasons behind the observed shift of the BAO scale to smaller values in simulations, emphasizing the role of overdense regions and providing analytic expressions that align with simulation results.
Contribution
It offers a simple physical picture and analytic formulas for the non-linear BAO scale shift, clarifying the effects of overdensities and bias, and supports the effectiveness of reconstruction methods.
Findings
The BAO scale shift is mainly due to overdense regions acting as positively curved universes.
Analytic expressions accurately predict the non-linear shift observed in simulations.
Reconstruction methods can effectively reverse the BAO scale shift.
Abstract
A shift of the baryon acoustic oscillation (BAO) scale to smaller values than predicted by linear theory was observed in simulations. In this paper, we try to provide an intuitive physical understanding of why this shift occurs, explaining in more pedagogical detail earlier perturbation theory calculations. We find that the shift is mainly due to the following physical effect. A measurement of the BAO scale is more sensitive to regions with long wavelength overdensities than underdensities, because (due to non-linear growth and bias) these overdense regions contain larger fluctuations and more tracers and hence contribute more to the total correlation function. In overdense regions the BAO scale shrinks because such regions locally behave as positively curved closed universes, and hence a smaller scale than predicted by linear theory is measured in the total correlation function. Other…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
