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We propose a novel mechanism to generate sterile neutrinos ₒ in the early Universe, by converting ordinary neutrinos _ in scattering processes ₒ_ₒₒ. After initial production by oscillations, this leads to an exponential growth in the ₒ abundance. We show that such a production regime naturally occurs for self-interacting ₒ, and that this opens up significant new parameter space where ₒ make up all of the observed dark matter. Our results provide strong motivation to further push the sensitivity of X-ray line searches, and to improve on constraints from structure formation.
Bringmann et al. (Mon,) studied this question.
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