A Dynamical Framework for KeV Dirac Neutrino Warm Dark Matter

TL;DR

This paper proposes a dynamical model for keV-scale Dirac sterile neutrinos as warm dark matter, explaining their properties and production mechanisms consistent with structure formation constraints.

Contribution

It introduces a framework where right-handed active neutrinos are composite and sterile neutrinos gain keV masses through extended Technicolor, with a simple dynamical scale setup.

Findings

Framework naturally produces keV sterile neutrinos as warm dark matter.

The model predicts cool dark matter with small free-streaming length.

A toy model illustrating the framework's key features is provided.

Abstract

If the source of the reported $3.5$ keV x-ray line is a sterile neutrino, comprising an $\mathcal{O}(1)$ fraction of the dark matter (DM), then it exhibits the property that its mass times mixing angle is $\sim \mbox{few} \times 10^{-2}$ eV, a plausible mass scale for the active neutrinos. This property is a common feature of Dirac neutrino mixing. We present a framework that dynamically produces light active and keV sterile Dirac neutrinos, with appropriate mixing angles to be the x-ray line source. The central idea is that the right-handed active neutrino is a composite state, while elementary sterile neutrinos gain keV masses similarly to the quarks in extended Technicolor. The entire framework is fixed by just two dynamical scales and may automatically exhibit a warm dark matter (WDM) production mechanism -- dilution of thermal relics from late decays of a heavy composite neutrino -- such that the keV neutrinos may comprise an $\mathcal{O}(1)$ fraction of the DM. In this framework, the WDM is typically quite cool and within structure formation bounds, with temperature $\sim \mbox{few}\times 10^{-2}~T_\nu$ and free-streaming length $\sim$ few kpc. A toy model that exhibits the central features of the framework is also presented.