Abstract
We propose a model which uses the seesaw mechanism and the lepton number L¯=LeLμLτ to achieve the neutrino mass spectrum m1=m2 and m3=0, together with a lepton mixing matrix U with Ue3=0. In this way, we accommodate atmospheric neutrino oscillations. A small mass splitting m1>m2 is generated by breaking L¯ spontaneously and using Babu’s two-loop mechanism. This allows us to incorporate either the “just so” or the LOW solution of the solar-neutrino problem, with maximal mixing, into the model. The resulting mass matrix has three parameters only, since L¯ breaking leads exclusively to a non-zero ee matrix element.
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