Constraining models for keV sterile neutrinos by quasi-degenerate active neutrinos

Abstract

We present a No-Go theorem for keV sterile neutrino Dark Matter: if sterile neutrinos at the keV scale play the role of Dark Matter, they are typically unstable and their decay produces an astrophysical monoenergetic X-ray line. It turns out that the observational bound on this line is so strong that it contradicts the existence of a quasi-degenerate spectrum of active neutrinos in a seesaw type I framework where the Casas-Ibarra matrix R is real. This is the case in particular for models without CP violation. We give a general proof of this theorem. While the theorem (like every No-Go theorem) relies on certain assumptions, the situation under which it applies is still sufficiently general to lead to interesting consequences for keV neutrino model building. In fact, depending on the outcome of the next generation experiments, one might be able to rule out whole classes of models for keV sterile neutrinos.

14 pages, 1 figure; v.3: error in the compilation of the file corrected (some references did not show properly); Special thanks to D. Boedecker for pointing out that issue to me!

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Cited by in corpus (1)

• Sterile Neutrinos as the Origin of Dark and Baryonic Matter