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In this talk I address the theoretical issue of what new physics is requiredto make $m_\nu \neq 0$. I then discuss what other things may happen besidesneutrino oscillations. In particular I consider a possible new scenario ofleptogenesis in R parity nonconserving supersymmetry.Comment: 7 pages including 1 figure, talk at WHEPP-

How neutrinos get mass and what other things may happen besides oscillations?