Abstract
We compute the μ → e conversion in the type-I seesaw model, as a function of the right-handed neutrino mixings and masses. The results are compared with previous computations in the literature. We determine the definite predictions resulting for the ratios between the μ → e conversion rate for a given nucleus and the rate of two other processes which also involve a μ − e flavour transition: μ → eγ and μ → eee. For a quasi-degenerate mass spectrum of right-handed neutrino masses — which is the most natural scenario leading to observable rates — those ratios depend only on the seesaw mass scale, offering a quite interesting testing ground. In the case of sterile neutrinos heavier than the electroweak scale, these ratios vanish typically for a mass scale of order a few TeV. Furthermore, the analysis performed here is also valid down to very light masses. It turns out that planned μ → e conversion experiments would be sensitive to masses as low as 2 MeV. Taking into account other experimental constraints, we show that future μ → e conversion experiments will be fully relevant to detect or constrain sterile neutrino scenarios in the 2 GeV−1000 TeV mass range.
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Alonso, R., Dhen, M., Gavela, M.B. et al. Muon conversion to electron in nuclei in type-I seesaw models. J. High Energ. Phys. 2013, 118 (2013). https://doi.org/10.1007/JHEP01(2013)118
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DOI: https://doi.org/10.1007/JHEP01(2013)118