An optimal nonlinear method for simulating relic neutrinos

TL;DR

This paper introduces an advanced simulation method for neutrinos in cosmology that reduces shot noise and accurately models small-scale structures, enabling better predictions for future observations.

Contribution

The paper presents a novel neutrino simulation technique that minimizes shot noise and accurately captures nonlinear scales without neglecting neutrino back-reaction.

Findings

Reduces shot noise by a factor of about 100 at z=0 for minimal neutrino masses.

Achieves permille level agreement in matter power spectrum with existing methods.

Allows neutrino simulations with lower particle load and works across all neutrino masses.

Abstract

Cosmology places the strongest current limits on the sum of neutrino masses. Future observations will further improve the sensitivity and this will require accurate cosmological simulations to quantify possible systematic uncertainties and to make predictions for nonlinear scales, where much information resides. However, shot noise arising from neutrino thermal motions limits the accuracy of simulations. In this paper, we introduce a new method for simulating large-scale structure formation with neutrinos that accurately resolves the neutrinos down to small scales and significantly reduces the shot noise. The method works by tracking perturbations to the neutrino phase-space distribution with particles and reduces shot noise in the power spectrum by a factor of $\mathcal{O}\left(10^2\right)$ at $z=0$ for minimal neutrino masses and significantly more at higher redshifts, without neglecting the back-reaction caused by neutrino clustering. We prove that the method is part of a family of optimal methods that minimize shot noise subject to a maximum deviation from the nonlinear solution. Compared to other methods we find permille level agreement in the matter power spectrum and percent level agreement in the large-scale neutrino bias, but large differences in the neutrino component on small scales. A basic version of the method can easily be implemented in existing N-body codes and makes it possible to run neutrino simulations with significantly reduced particle load. Further gains are possible by constructing background models based on perturbation theory. A major advantage of this technique is that it works well for all masses, enabling a consistent exploration of the full neutrino parameter space.