Addressing the Hubble tension with Sterile Neutrino Dark Matter

One of the promising dark matter (DM) candidates is a keV scale sterile neutrino. In the early universe the observed relic of the sterile neutrino DM is generated via the $\mathit{\text{Dodelson-Widrow}}$ mechanism. However, this production scenario is severely constraint by various astrophysical observations. Many non-standard interactions between active (${\nu }_a$) and sterile (${\nu }_s$) neutrino have been proposed to evade these astrophysical bounds. Here, we study sterile neutrino in the context of a mass-varying scenario by coupling both active and sterile neutrino to a scalar field. This novel mechanism opens up a new parameter space that generates the observed DM relic and alleviates the $\mathit{\text{Hubble}}\mathit{\text{tension}}$. We find that the resulting parameter space can be fully probed by future X-ray missions.