Revisiting sterile neutrino dark matter in gauged $U(1)_{B-L}$ model

TL;DR

This paper reevaluates sterile neutrino dark matter within a gauged U(1)_{B-L} model, refining the parameter space by detailed density evolution analysis, which aligns with cosmological constraints and reveals new production mechanisms.

Contribution

It provides a more accurate calculation of sterile neutrino production and gauge coupling constraints, highlighting the importance of scalar contributions previously neglected.

Findings

Smaller gauge coupling needed for freeze-in sterile neutrinos.

Excluded large parameter space due to free-streaming constraints.

Identified dominant production of N from Z' pairs at B-L breaking scale.

Abstract

We reexamine sterile neutrino dark matter in gauged $U(1)_{B-L}$ model. Improvements have been made by tracing and careful evaluation of the evolution of the number densities of sterile neutrinos $N$ and extra neutral gauge bosons $Z'$. As a result, the cosmologically-interesting gauge coupling of $U(1)_{B-L}$ for freeze-in sterile neutrinos turns out to be smaller than the values reported in the literature. This avoids the overproduction of $Z'$ so that it is consistent with the big bang nucleosynthesis and the cosmic microwave background constraints on the effective number of neutrino species. Similarly, the free-streaming length constraints exclude a large parameter space derived in previous studies. In addition to known freeze-in pair production of $N$ from the standard model fermion pairs, we find the case that $N$ is dominantly produced from a pair of $Z'$ at the temperature characterized by the $B-L$ breaking scalar mass. Thus, the naive truncation of the $U(1)_{B-L}$ scalar contribution made in the literature is not valid.