PIRSA:24120022

Video URL

https://pirsa.org/24120022

The speed of sound in the EFTofLSS

Nascimento, C. (2024). The speed of sound in the EFTofLSS. Perimeter Institute for Theoretical Physics. https://pirsa.org/24120022

Nascimento, Caio. The speed of sound in the EFTofLSS. Perimeter Institute for Theoretical Physics, Dec. 10, 2024, https://pirsa.org/24120022 

          @misc{ scivideos_PIRSA:24120022,
            doi = {10.48660/24120022},
            url = {https://pirsa.org/24120022},
            author = {Nascimento, Caio},
            keywords = {Cosmology},
            language = {en},
            title = {The speed of sound in the EFTofLSS},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2024},
            month = {dec},
            note = {PIRSA:24120022 see, \url{https://scivideos.org/index.php/pirsa/24120022}}
          }

Caio Nascimento University of Washington

Talk numberPIRSA:24120022
DOI10.48660/24120022
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

The Effective Field Theory of Large Scale Structure (EFTofLSS) has found tremendous success as a perturbative framework for the evolution of large scale structure, and it is now routinely used to compare theoretical predictions against cosmological observations. The model for the total matter field includes one nuisance parameter at 1-loop order, the effective sound speed, which can be extracted by matching the EFT to full N-body simulations. In this talk we explore two different directions related to the effective sound speed. We first show that its emergence can be understood even without effective field theory ingredients, through a perturbative framework that solves the Vlasov-Poisson system of equations directly in phase space. However, we will argue that the EFT is necessary to ensure self-consistency. We then discuss how one can estimate the effective sound speed, via separate universe techniques, with analytic calculations. The estimate is in good agreement with simulation results, and we show it can be used to extract the cosmology dependence of the effective sound speed and to shed light on what cosmic structures shape its value.