Higher-order initial conditions with massive neutrinos
Willem Elbers, Carlos S. Frenk, Adrian Jenkins, Baojiu Li, Silvia, Pascoli

TL;DR
This paper demonstrates that higher-order Lagrangian perturbation theory can effectively incorporate massive neutrino effects into initial conditions, significantly improving the accuracy of cosmological simulations for upcoming large-scale structure surveys.
Contribution
It introduces a method to include neutrino effects in higher-order ICs, enabling more precise simulations that meet the accuracy requirements of future surveys.
Findings
Higher-order ICs reduce errors below 1% for matter power spectrum.
First-order Zel'dovich ICs produce errors exceeding 1% at late times.
2LPT and 3LPT agree within 1% at redshift zero.
Abstract
The discovery that neutrinos have mass has important consequences for cosmology. The main effect of massive neutrinos is to suppress the growth of cosmic structure on small scales. Such growth can be accurately modelled using cosmological -body simulations, but doing so requires accurate initial conditions (ICs). There is a trade-off, especially with first-order ICs, between truncation errors for late starts and discreteness and relativistic errors for early starts. Errors can be minimized by starting simulations at late times using higher-order ICs. In this paper, we show that neutrino effects can be absorbed into scale-independent coefficients in higher-order Lagrangian perturbation theory (LPT). This clears the way for the use of higher-order ICs for massive neutrino simulations. We demonstrate that going to higher order substantially improves the accuracy of simulations. To match…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Neutrino Physics Research · Particle physics theoretical and experimental studies
