The IR-resummed Effective Field Theory of Large Scale Structures
Leonardo Senatore, Matias Zaldarriaga
TL;DR
The authors address BAO-induced residuals in equal-time EFT predictions for the matter power spectrum by introducing an IR-resummation that treats large-scale displacements non-perturbatively within a Lagrangian framework. The method reformulates Eulerian EFT predictions through a displacement-mixing kernel K0 and a mode-mixing matrix M_{||}, yielding IR-safe equal-time correlators and improved BAO damping, with extensions to momentum spectra to account for velocity effects. At two loops, the IR-resummed EFT matches numerical simulations up to k ≈ 0.6 h Mpc^{-1} to within 1%, and one-loop results extend accurate predictions further, while momentum spectra gain enhanced UV reach thanks to velocity treatments and optimized resummation. Real-space BAO predictions and their dependence on EFT parameters are shown to be robust, supporting the method’s potential for precise cosmological inferences from BAO and related statistics.
Abstract
We present a new method to resum the effect of large scale motions in the Effective Field Theory of Large Scale Structures. Because the linear power spectrum in $Λ$CDM is not scale free the effects of the large scale flows are enhanced. Although previous EFT calculations of the equal-time density power spectrum at one and two loops showed a remarkable agreement with numerical results, they also showed a 2% residual which appeared related to the BAO oscillations. We show that this was indeed the case, explain the physical origin and show how a Lagrangian based calculation removes this differences. We propose a simple method to upgrade existing Eulerian calculations to effectively make them Lagrangian and compare the new results with existing fits to numerical simulations. Our new two-loop results agrees with numerical results up to $k\sim 0.6 h/$Mpc to within 1% with no oscillatory residuals. We also compute power spectra involving momentum which is significantly more affected by the large scale flows. We show how keeping track of these velocities significantly enhances the UV reach of the momentum power spectrum in addition to removing the BAO related residuals. We compute predictions for the real space correlation function around the BAO scale and investigate its sensitivity to the EFT parameters and the details of the resummation technique.
