Sterile Neutrinos: Cosmology vs Short-BaseLine Experiments
Maria Archidiacono, Nicolao Fornengo, Carlo Giunti, Steen Hannestad,, and Alessandro Melchiorri

TL;DR
This paper analyzes the compatibility of light sterile neutrinos with cosmological and short baseline experimental data, finding consistent evidence for ~1 eV mass scale and partial thermalization scenarios.
Contribution
It provides a comprehensive combined analysis of cosmological and SBL data, considering partial thermalization, and identifies consistent sterile neutrino mass scales around 1 eV.
Findings
Preference for sterile neutrinos in both (3+1) and (3+2) scenarios.
Evidence at 3.3 sigma for (3+1) model with SBL data.
Mass scale around 1 eV for sterile neutrinos from combined data.
Abstract
Cosmology and short baseline neutrino oscillation data both hint at the existence of light sterile neutrinos with masses in the 1 eV range. Here we perform a detailed analysis of the sterile neutrino scenario using both cosmological and SBL data. We have additionally considered the possibility that the extra neutrino degrees of freedom are not fully thermalised in the early universe. Even when analyzing only cosmological data we find a preference for the existence of massive sterile neutrinos in both (3+1) and (3+2) scenarios, and with the inclusion of SBL data the evidence is formally at the 3.3sigma level in the case of a (3+1) model. Interestingly, cosmological and SBL data both point to the same mass scale of approximately 1 eV. In the (3+1) framework WMAP9+SPT provide a value of the sterile mass eigenstate m_4 = (1.72 \pm 0.65) eV: this result is strenghtened by adding the prior…
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