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We review and remark on models of radiatively induced neutrino Majorana masses and oscillations. It is pointed out that while the models are capable of accounting for the observed solar and atmospheric neutrino oscillations, some of them can also induce neutrinoless double beta decay and μ^--e⁺ conversion in nuclei large enough to be potentially observable in the near future.
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Chang et al. (2000) studied this question.
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