ar X iv : h ep - p h / 02 09 12 7 v 1 1 2 Se p 20 02 Neutrino factories — Physics potential and present status
نویسنده
چکیده
The observation of atmospheric neutrinos (See, e.g., Ref.[1]) and solar neutrinos (See, e.g., Ref.[2, 3]) gives the information on the mass squared differences and the mixings, which can be written in the three flavor framework of neutrino oscillations as (|∆m32|, θ23) and (∆m21, θ12), where I have adopted the standard parametrization [4] for the 3× 3 MNSP [5, 6] matrix. On the other hand, the CHOOZ result [7] tells us that |θ13| has to be small (sin 2θ13 <∼ 0.1). So the MNSP matrix looks like
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