Models of maximal atmospheric neutrino mixing

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dc.creatorGrimus, W.
dc.creatorLavoura, L.
dc.date2003-10-03
dc.date.accessioned2026-07-25T18:54:49Z
dc.descriptionWe discuss two types of neutrino mass matrices which both give $θ_{23} = 45^\circ$, i.e., a maximal atmospheric mixing angle. We review three models, based on the seesaw mechanism and on simple extensions of the scalar sector of the Standard Model, where those mass matrices are obtained from symmetries.
dc.description10 pages, plain LaTeX; talk presented by W. Grimus at the XXVII International Conference of Theoretical Physics, Ustron, Poland, 15-21 September 2003
dc.identifierhttps://arxiv.org/abs/hep-ph/0310050
dc.identifierhttp://arxiv.org/abs/hep-ph/0310050
dc.identifierActa Phys.Polon. B34 (2003) 5393-5404
dc.identifier.urihttps://dspace.dare.co.zw/handle/123456789/59657
dc.subjectHigh Energy Physics - Phenomenology
dc.titleModels of maximal atmospheric neutrino mixing
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