Cosmological constraints on a light non-thermal sterile neutrino

TL;DR

This paper uses cosmological data to constrain the properties and existence of a light non-thermal sterile neutrino, exploring its mass, density, and production mechanisms within an extended cosmological model.

Contribution

It provides nearly model-independent constraints on light relics and their properties, and analyzes the compatibility of sterile neutrinos with cosmological observations.

Findings

A 2 eV sterile neutrino can be compatible if thermally distributed with T_s/T_nu < 0.8.

Constraints on non-resonantly produced sterile neutrinos with Delta N_eff < 0.5.

Data allows standard thermalized neutrinos with mass less than 0.9 eV.

Abstract

Although the MiniBooNE experiment has severely restricted the possible existence of light sterile neutrinos, a few anomalies persist in oscillation data, and the possibility of extra light species contributing as a subdominant hot (or warm) component is still interesting. In many models, this species would be in thermal equilibrium in the early universe and share the same temperature as active neutrinos, but this is not necessarily the case. In this work, we fit up-to-date cosmological data with an extended LambdaCDM model, including light relics with a mass typically in the range 0.1 -10 eV. We provide, first, some nearly model-independent constraints on their current density and velocity dispersion, and second, some constraints on their mass, assuming that they consist either in early decoupled thermal relics, or in non-resonantly produced sterile neutrinos. Our results can be used for constraining most particle-physics-motivated models with three active neutrinos and one extra light species. For instance, we find that at the 3 sigma confidence level, a sterile neutrino with mass m_s = 2 eV can be accommodated with the data provided that it is thermally distributed with (T_s/T_nu) < 0.8, or non-resonantly produced with (Delta N_eff) < 0.5. The bounds become dramatically tighter when the mass increases. For m_s < 0.9 eV and at the same confidence level, the data is still compatible with a standard thermalized neutrino.