Probes of cosmic inflation: from the CMB to quantum systems
Emilie Hertig - University of Cambridge
Bastos de Senna Nascimento, C. (2024). The speed of sound in the EFTofLSS. Perimeter Institute. https://pirsa.org/24120022
Bastos de Senna Nascimento, Caio. The speed of sound in the EFTofLSS. Perimeter Institute, Dec. 10, 2024, https://pirsa.org/24120022
@misc{ pirsa_PIRSA:24120022,
doi = {10.48660/24120022},
url = {https://pirsa.org/24120022},
author = {Bastos de Senna Nascimento, Caio},
keywords = {Cosmology},
language = {en},
title = {The speed of sound in the EFTofLSS},
publisher = {Perimeter Institute},
year = {2024},
month = {dec},
note = {PIRSA:24120022 see, \url{https://pirsa.org}}
}
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.